Spectral Reproduction from Scene to Hardcopy II Image Processing
绿色对相机的影响英语作文
绿色对相机的影响英语作文Title: The Impact of Green Light on Cameras。
Introduction:In the realm of photography, light is paramount. It shapes our images, dictates exposure, and influences the overall quality of the final product. Among the various hues of light, green light holds a unique position due to its distinct effects on cameras. This essay delves into the impact of green light on cameras, exploring itssignificance and implications.Spectral Composition:Green light, situated within the visible spectrum, occupies wavelengths ranging approximately from 520 to 570 nanometers. Its prevalence in natural landscapes and artificial environments makes it a common element encountered during photography sessions.Exposure and White Balance:The presence of green light significantly affects exposure settings and white balance calibration. Cameras, designed to capture scenes under natural lighting conditions, may struggle to accurately meter and balance green-dominated environments. Consequently, images captured under such conditions may exhibit color casts, inaccuracies in white balance, and compromised exposure levels.Color Representation:Green light influences color reproduction, particularly in scenes where it predominates. Cameras may struggle to faithfully reproduce other hues present in the scene, leading to color shifts and distortion. This phenomenon poses challenges for photographers striving for accurate color rendition in their images.Image Quality:The impact of green light extends beyond mere color representation. It can influence overall image quality, affecting sharpness, contrast, and dynamic range. Excessive green light may result in reduced image clarity and detail, detracting from the visual appeal of photographs.Artistic Considerations:Despite its technical challenges, green light also presents opportunities for creative expression. Photographers adept at harnessing its unique qualities can leverage it to create captivating images imbued with a sense of vitality and vibrancy. By embracing green light as a creative tool rather than a hindrance, photographers can explore new avenues of artistic experimentation.Mitigation Strategies:To mitigate the adverse effects of green light on cameras, photographers employ various techniques and tools. These may include manual adjustment of exposure settings, custom white balance calibration, and the use of lensfilters designed to counteract specific color casts. Additionally, post-processing software offers a plethora of tools for fine-tuning color balance and correcting inaccuracies introduced by green light.Conclusion:In conclusion, the impact of green light on cameras is multifaceted, encompassing technical challenges, artistic opportunities, and mitigation strategies. Understanding its influence enables photographers to navigate diverse shooting environments effectively, ensuring the creation of compelling and technically proficient images. Despite its complexities, green light remains an integral component of the photographic process, shaping the visual narratives captured through the lens.。
色彩控制(Colorcontrol)
色彩控制(Color control)Red, green, and blue color is yellow, magenta and cyanColor controlThe three basic attributes of color: hue, hue, brightness, saturationFactors affecting color saturationexposureSmoothness of the surface of the subject (silk [cotton])The quality of light (direct scattering)The subtractive (red and yellow)Camera color reproduction - additive color (red green blue)Color temperatureIn the visible spectrum, the spectrum of the light source is the same as the spectrum of an absolute blackbody at a certain temperature (which is theoretically illuminated without reflecting objects), and the temperature of the absolute black body is called the color temperature of the source. Color temperature is not the actual temperature of the light source itself.Different light source attributes, color temperature is alsodifferentColor temperature of luminaireOne is taken under 5600K color temperature (outdoor natural light shooting);The other is 3200K color temperature (taken under indoor light)white balanceIn order to make the scene images unbiased, the color temperature of white objects under different light conditions is uniformly adjusted to 3200K in the camera. It can also be understood that the RGB signal produced by the camera in each scene is equal in amplitude.The white balance should be adjusted once every scene is changed, and the white balance should be adjusted when the same scene changes with the light condition.Color temperatureThe camera can only make a white balance based on a particular color temperatureAvoid mixing lightColour reproduction standardSkin tone is the only real criterion for viewers to judge theoverall color of televisionColour filterIn order to meet the different lighting conditions so as to reproduce the correct color, a few color temperature color filters are added between the zoom lens and the color separation prism. Their spectral response characteristics are used to compensate for changes in spectral properties due to different color temperatures.The camera is based on an 3200K light source, i.e., the color temperature filter is colorless transparent glass. When the color temperature of the light source is 4800K, the blue light component in the spectrum will increase, so it is necessary to add 4800K color temperature filter to reduce the transmittance of blue light, while the total spectral response characteristics remain unchanged, that is, the color temperature is restored to 3200K.The 4800K filter is light orange, and the 7500K filter is orange. The 2850K filter is used to increase the color temperature to 3200K, so it is light blue.Attenuation filter (gray chip)When the camera tube works under strong light, the aperture should be reduced. But sometimes, in order to achieve a certain artistic effect, it is not allowed to reduce the aperture, which needs to be added to the optical path to reduce the luminous flux of the attenuator, that is, attenuation filter. Itstransmittance usually has 100%, 25%, 10% and 1.5% kinds, while spectral response characteristics should be straight.Combination of color filter and ash blockFilter filter selection button shooting environment1 through sunrise, sunset, or indoors2 5600K+1/4ND sunny day3 5600K cloudy or rainy4 5600K+1/16ND very bright environment, snow or seasideWhite balance adjustment step1) set the Gain gain select key in the correct position;2) close the menu;3) OUTPUT/DCC is set to CAM;4) set the WHITE BAL to A or B;5) select the appropriate color filter according to the light conditions of the shooting environment;6) in the same light conditions aligned with a white object, the white area should be at least 70% of the area, pay attention to the screen does not have white high brightness points;7) set the lens to automatic iris mode;8) perform automatic white balance;After the completion of finder will be displayed in the "WHITE:OK **K", said automatic white balance, color temperature is **K.WHITE BAL white balance switch:PRST: when there is no time to set the white balance, the color temperature is determined according to the selected color filter:A/B: when using the automatic white balance function, the color temperature value will be stored in two A or B memories:B (ATW): set the B ORERATION in the menu MODE CH to ATW,This switch is automatically tracking the white balance function. When shooting environment changes, the color temperature will automatically track changes;Full automatic tracking white balanceThe ATW switch is placed on the ON, and the auto tracking white balance function starts. The function is adjusted by the white balance at the brightest point at any moment, so that the white balance of the scene changing continuously is basically correct. This method is used only in emergency situations, and thedrawback is not accurate enough.ATW automatic white balance working conditions:Work at 2500 K ~7000 K color temperature conditions, and the light intensity can not be too strong or too darkWant to have some colors, reference can use this color corresponding to the color as white balanceThe use of manual adjustment of the white balance to achieve certain special effectsColor vision reactionLong wave light: the dilated reaction of the retina; the quickening of blood circulation; the excitability of the mental systemShort wave lightWarm and cold feeling of colorWarm colors and bright colors have a sense of expansion, cool colors and dark colors, a sense of contraction, the color of the advance and retreatCohesion and color balance (after image principle)The foundation of the emotional characteristics of colorPhysiological psychological reactionDaily life experienceCustoms, culture and politics of different nations and societiesgulesActive, energetic and vitalWarm, warm, ideal pursuitGood luck and good life wishesrevolutionAn intense color that stimulates sexual desireyellowLightness is the highest, lightest and brightestCheerful, relaxed, optimistic, naive and romanticNoble dignitygreenWavelengths between red and blue, neither expansion nor contraction, most suitable for the human eye, a quiet and stablefeelingLife, hopeblueCold, indifferentDepressiveShades of blue lead to different moodsPale blue: cool, fresh, elegant and secluded (blended with a white touch)The lightness and saturation of colors are important to feelingsblackTwo factors: the inherent black of the object and the shadow formed by illuminationTerror, evilSorrow, despair, deathA sense of weight and strengthGraveHeavy repression; self closurewhitepureHoly nobilityPeace and quietpeacePale and frigid; morbidDifferent ethnic cultures: Chinese white is a funeral colorCamera color controlColor tone: dominant in space and timeControl method of color tone: internal color block method and external color cover methodInterior color law: to make all the colors within the scene, including the background, clothing, props, to the base palette close, so that it becomes dominant in the areaExternal color cover method: filter, post production, white balance settings, etc.Camera color controlKey colors: special attention that causes vision and brings special emotions.The two element -- unusual, never seen beforeThrough color: color key does not appear many times, but throughout the play, play the role of emphasis and echo。
Spectral
Introduction
Semiclassical theories for spectral statistics have been developed [1, 2, 3] to find an explanation for the observed universality in energy spectra of quantum systems with a chaotic classical limit, the agreement of correlations in energy spectra with those between eigenvalues of random matrices [4]. They are based on semiclassical trace formulas that approximate the density of states in terms of classical trajectories [5]. It has been shown by these theories that in the asymptotic limit of long-range correlations two-point correlation functions do coincide with those of random matrix theory [2, 3]. These results are based on mean properties of periodic orbits [1]. To go beyond the leading asymptotic term requires information about correlations between periodic orbits which are presently not available [6]. One of the expectations, on basis of the random matrix hypothesis [7], is that a perturbation of a chaotic system should not change the statistical distribution of the energy levels of the quantum system, if it does not change the chaotic nature of the classical motion. In the present article we investigate, on the level of the semiclassical approximation, whether the perturbation by a pointlike scatterer has this property. One argument in favour of this invariance is that the semiclassical approximation for the density of states is not changed in leading order of ~ for this perturbation. The influence of the scatterer is described semiclassically by a certain class of trajectories, so-called diffractive orbits that start from the scatterer and return to it. They contribute to the density of states in higher order of ~ than the leading order contribution from periodic orbits. The present article is motivated by the observation in [8] that a scatterer could nevertheless have an influence on spectral statistics. When spectral correlation functions are calculated by using mean properties of diffractive orbits, the so-called diagonal approximation, they show modifications which, in general, do not vanish in the semiclassical limit (~ → 0). In order that this does not lead to deviations from random matrix statistics, these terms have to be cancelled by off-diagonal terms which contain information about correlations between different trajectories. As remarked above, the calculation of correlations between trajectories is an unsolved problem in general systems. For the diffractive orbits that describe the influence of a scatterer, however, off-diagonal terms can be calculated explicitly. This is done in the following sections. The results show that diagonal and off-diagonal terms indeed cancel each other. Furthermore, the results can be used to investigate parametric spectral correlations, i. e. correlations between spectra of the system for different parameter values, where the parameter is the strength of the scatterer. It is shown that the parametric spectral correlations are universal for small changes of the parameter.
可见光光谱 英文
可见光光谱英文The visible light spectrum, encompassing wavelengths ranging from approximately 400 nanometers (nm) to 700 nm,is a narrow slice of the electromagnetic radiation that our eyes are capable of perceiving. This band of wavelengths, although relatively small compared to the vast expanse of the electromagnetic spectrum, plays a pivotal role in our daily lives, shaping our perception of the world around us. At the shorter wavelength end of the visible spectrum, we encounter violet light. Violet waves, with their frequencies exceeding 668 THz, are the highest in energy among all visible colors. As we move towards the red end of the spectrum, wavelengths increase, resulting in lower frequencies and consequently, lower energy levels. Red light, with wavelengths exceeding 700 nm, has the lowest energy among all visible colors.The visible spectrum is not just a random assortment of colors; it is a carefully crafted array of hues that enables us to perceive a wide range of colors. The human eye is equipped with photoreceptors called cones, which are sensitive to specific wavelengths within the visiblespectrum. These cones are primarily sensitive to blue, green, and red light, allowing us to perceive the full range of colors visible to the naked eye.The importance of the visible light spectrum extends beyond our ability to see colors. It plays a crucial role in photosynthesis, the process by which plants convert light energy into chemical energy. Chlorophyll, the green pigment found in plants, is highly absorbent of blue and red light wavelengths, which are essential for photosynthesis. Without the visible light spectrum, photosynthesis would not be possible,严重影响着整个生态系统的运转。
三种谱分解方法的量化对比
IPTC-17944-MSQuantitative Comparison of Three Spectral Decomposition MethodsDonald C.Adams,and David Markus,Saddleback Geosolutions LLC.Copyright2014,International Petroleum Technology ConferenceThis paper was prepared for presentation at the International Petroleum Technology Conference held in Kuala Lumpur,Malaysia,10–12December2014.This paper was selected for presentation by an IPTC Programme Committee following review of information contained in an abstract submitted by the author(s). Contents of the paper,as presented,have not been reviewed by the International Petroleum Technology Conference and are subject to correction by the author(s). The material,as presented,does not necessarily reflect any position of the International Petroleum Technology Conference,its officers,or members.Papers presented at IPTC are subject to publication review by Sponsor Society Committees of IPTC.Electronic reproduction,distribution,or storage of any part of this paper for commercial purposes without the written consent of the International Petroleum Technology Conference is prohibited.Permission to reproduce in print is restricted to an abstract of not more than300words;illustrations may not be copied.The abstract must contain conspicuous acknowledgment of where and by whom the paper was presented.Write Librarian,IPTC,P.O.Box833836,Richardson,TX75083-3836,U.S.A.,faxϩ1-972-952-9435AbstractSeveral time-frequency transform methods have been used for spectral decomposition of seismic data. Comparisons between methods have been largely qualitative with a focus on their relative time and frequency resolutions.Very little has been said about the fidelity of spectral decomposition results relative to the original data and the quantitative differences between methods.This paper provides some analysis of these issues as they relate to three decomposition methods,namely the S-transform(ST),Matching Pursuit(MP)and Empiric Mode Decomposition(EMD).Our quantitative comparison made use of the following methods:●Total energy of the trace vs.time-frequency transform–the ideal spectral decomposition will havetotal energy equal to the input signal.●Marginal time and frequency conditions–the ideal spectral decomposition will satisfy themarginal conditions.The integral of the spectra over frequency will equal the instantaneous energy of the trace and the integral over time will equal the power spectra of the trace.Our analysis used a combination of synthetic and acquired traces and wedge models.The single trace and wedge model results suggest that the characteristics of the spectral decomposition change with the type of time-frequency transform used in the decomposition.●ST wedge model conformed to the bandlimited spike interference model with spacing dependentspectral notches.The single trace marginal conditions were satisfied best with a resolution ratio near1.4at the cost of a little time resolution relative to a default resolution ratio of1.0.●MP wedge model did not have spectral notches and is negatively influenced by the greediness andpath dependence of the process.The single trace marginal condition details however are best satisfied by MP.●EMD wedge model spectrum was very sparse with an apparent relationship between the frequencyof the components and the degree of tuning.The single trace marginal conditions satisfaction is variable and dependent on the model traces having satisfied the underlying assumptions.We recommend the use of marginal condition analysis in parameter selection for spectral decompo-sition and to facilitate better products for quantitative analysis.IntroductionSeveral time-frequency transform methods have been applied under the guise of spectral decomposition for the interpretation of seismic reflection data.Some examples of these methods are the short window Fourier transform,continuous wavelet transform,S-transform,MP,empiric mode decomposition,and quadratic time-frequency distributions.In this study we focused on the quantitative comparison of three methods:the S-transform,MP and empiric mode decomposition.The algorithms used in this study have been extensively tested and adjusted by the authors to minimize distortion and maximize energy conservation with the addition of appropriate scales,and application of additional signal processing techniques,beyond those discussed in the references.S-Transform based spectral decomposition is a hybrid member of the family of methods that includes the short window Fourier and continuous wavelet transforms.The S-transform has the frequency resolution of a Fourier transform with the time resolution of a continuous wavelet transform and an absolute phase reference at the start of the trace(Stockwell et al.,1996).This family of methods comprises the most popular methods used for spectral decomposition.The original S-transform algorithm is described in Stockwell et al.(1996)with its extension to seismic spectral decomposition discussed by Theophanis and Queen(2000).MP based spectral decomposition is the original member of a family of methods that includes exponential pursuit decomposition(EPD)(Castagna et al.,2006),instantaneous spectral analysis(ISA) (Castagna and Sun2003),basis pursuit and many others.These methods are characterized by the use of an over-complete dictionary of waveforms with known spectra to create a piecewise representation of the trace,and then using that information,attempt to construct a time-frequency spectrum representative of the trace.The algorithm involves finding the best waveform match to a segment of the trace and removing it to form a residual trace;then best match to the residual trace is found and removed to form the next residual etc.,recursively applied,until a set of stopping criteria are satisfied leaving a residual signal.The spectra of the extracted shapes are used to build a Wigner-Ville time-frequency spectrum.The most common dictionary used for spectral decomposition is composed of Morlet wavelets;alternatively some proprietary methods possibly including ISA and EPD may use dictionaries based on the characteristics of the seismic traces to be decomposed.The original algorithm is described in Mallat and Zhang(1993)with extensions to seismic spectral decomposition discussed by Liu and Marfurt(2007)and Wang(2007).The original algorithm and its published extensions to seismic data do not conserve energy or satisfy time and frequency marginal conditions as indicated by Mallat and Zhang(1993),the algorithm used in this paper has been modified to maximize energy conservation.Empiric mode decomposition(EMD)is the original member of a family of data driven adaptive non-parametric methods created to analyze highly non-stationary signals associated with ocean waves and other phenomena(Huang et al.1998).The algorithm decomposes a signal into a set of components or intrinsic mode functions(IMF).The first IMF is constructed by averaging the boundaries of the signal envelope to form a residual signal and subtracting it from the original signal to get an empiric mode or IMF.The process continues with the residual signal until a set of stopping criteria are meet.The spectra are calculated from the IMF components and final residual using a process referred to as the Hilbert-Huang Transform(HHT).The resulting spectrum is very sparse,with the number of frequencies at any time sample equal to the number of IMFs.While S-transform and MP produce spectra at all predefined frequencies the HHT produces a set of frequencies vary from sample to sample and are defined by the interaction of the algorithm with the signal.The details of the original algorithm are described in Huang et al.(1998)and its extension to seismic spectral decomposition is discussed by Magrin-Chagnolleau and Baraniuk(1999).Han and van der Baan(2013)compare EMD algorithms for spectral decomposition.The sparseness of the spectra makes its display for publication difficult;in order to facilitate the visualcomparisons in this paper the bins used for EMD-HHT time-frequency display are9times the size of the bins used for MP and S-transform.MethodsPrevious comparisons of spectral decomposition methods,including those by Castagna et al.,(2003), Castagna and Sun,(2006),and Huang and Milkereit(2009),have been based on qualitative comparison of the spectra derived from test signals.Qualitative comparisons are good as far as they go,but they do not provide useful information for the geophysical researcher with regards to the accuracy of the methods relative to original signal.A more quantitative analysis based on Gabor’s uncertainty principal(Hall2006) is useful for understanding time-frequency uncertainty;however,it is limited to methods that use a priori basis functions to transform the signal to the time-frequency domain(Huang and Wu,2008)including the S-transform and MP.Gabor’s uncertainty principal does not apply to nonparametric methods like EMD-HHT.Robust methods are needed for quantifying time-frequency spectrum comparisons that are independent of the underlying math used to create the spectra.We examined several methods referenced in the literature including the Rényi entropy method(Flandrin et al.1994)and methods used in the comparison of quadratic time-frequency distributions(Boashash and Sucic,2003).The usefulness of these methods is limited to the comparison of time-frequency transforms from the same family.Instead,we selected a general set of methods based on the ideal properties of a time-frequency spectrum,paying close regard to Plancherel’s theorem on conservation of total energy,marginal frequency and marginal time conditions relative to the properties of the original signal.Additionally,numerical analysis and examination of the spectral decomposition responses from a wedge model are needed to provide a quantitative context for the use of spectral decompositions methods in exploration seismology.Marginal ConditionsPlancherel’s theorem states that the total energy of the time-frequency power spectrum is equal to the total energy of the signal.Cohen(1989)describes this as an ideal result of a quadratic time-frequency transform.We apply it to spectral decomposition methods in general and can show that we require a close approximation to this result for the methods to be useful in quantitative interpretation.The calculation for the time-frequency power spectrum is given by Equation1;total trace energy is calculated by integrating its instantaneous power.(1)An ideal spectral decomposition time-frequency power spectrum will satisfy the time and frequency marginal conditions.The time marginal condition states that the integral of the time-frequency spectra over frequency is equal to the time-dependent instantaneous power of the trace,given by Equation2 (Cohen,1989).The frequency marginal condition states that the integral of the time-frequency spectra over time will equal the power spectra of the trace,given by Equation3(Cohen,1989).In the equations, P is the energy density,t is time,⍀is frequency,E is total energy of trace x(t)and X(⍀)is the frequency spectrum of the trace.We use the relative size of the errors in the total energy and marginal conditions and their distribution as indicators of the suitability of the spectral decomposition for quantitative analysis(2)(3)Testing for frequency marginal condition is further complicated by the non-stationary nature of seismic traces.Calculation of a reference power spectrum of the trace with a Fourier transform assumes that signalis linear and periodic or stationary(Huang et al.1998),neither of which is strictly true for seismic traces. To illustrate how some of these effects are not negligible for application of a Fourier transform to non-stationary data we recall that:1.There is an inclusion of additional harmonic components to the spectrum that are not present inthe original signal,and these cause energy to be spread over a wider bandwidth than is present in the original signal(Huang et al.1989).2.Since the Fourier transform uses a linear superposition of trigonometric functions;it will addadditional harmonics to simulate deformed wave profiles(Huang et al.1989).3.Signal frequencies that are between Fourier frequencies are spread nonlinearly over severaladjacent Fourier frequencies.Given these limitations,details of the reference spectrum may not be present in the marginal spectrum from the time-frequency transform.In our experience,the marginal spectrum tends to follow the peaks of the Fourier spectrum.The marginal frequency spectrum derived from the Hilbert-Huang transform has a different meaning from the other spectral methods.The presence of a frequency indicates a likelihood of a particular wave occurring somewhere in the time interval and the power represents the total local power of the occurrences (Huang et al.1998).Whereas in the case of the Fourier transform,the presence of a frequency indicates persistence of the frequency over the length of the data(Huang et al.,1998).Wedge ModelAnalysis of wedge models is a useful way of determining seismic(Widess,1973)and attribute(Robertson and Nogami,1984)responses to changes in reflector spacing.For our analysis we demonstrated the time-frequency response changes for each of the spectral decomposition methods.Gridley and Partyka (1998)showed that spectral decomposition based on a short window discrete Fourier transform will have spectral peaks and notches with a frequency spacing related to time thickness of the wedge as described in Equation4;where⌬f is frequency spacing in Hz and⍀T is temporal thickness of the wedge in seconds (Gridley and Partyka,1998).For the common situation in sand-shale sequences where the reflection coefficients above and below the wedge have opposite signs,the locations of the peaks and notches are discussed by Marfurt and Kirlin(2001)and repeated as Equations5and6respectively;where n is a positive integer.The equations are reversed if the reflection coefficients have the same sign.We used a wedge model to examine how spectral decomposition response changed with the type of decomposition algorithm.(4)(5)(6)Our wedge model used a30Hz Ricker wavelet with rock properties derived from clean wet sand and shale in the Lower Miocene of the western Gulf of Thailand.Our model in Figure1is high impedance sand encased in low impedance shale with thickness between0.0and52.8ms TWT.AnalysisFirst we examined two single trace examples consisting of a wavelet interference test trace and a trace from a North Sea dataset.We used them to determine how well the various spectral decomposition methods satisfied the total energy and marginal conditions.Then we examined the wedge model to determine how the decomposition methods responded to a problem of geophysical importance.Single TraceThe first single trace example was based on synthetic traces composed of interfering Ricker wavelets as used by Chakraborty and Okaya (1995)and Castagna and Sun (2006)for qualitative comparison of spectral decomposition methods.Our version of the model in Figure 2consists of eight combinations of wavelets:A.Isolated 40Hz wavelet,B.3Isolated 30Hz wavelets an alternating polarity,C.2adjacent 20Hz wavelets with inner side lobe cancelation and opposing polarity,D.Isolated 10Hz wavelet,E.Coincident 10Hz and 40Hz wavelets,F.2Pairs of coincident 20Hz and 30Hz wavelets with constructive interference between inner 30Hz side lobes,G.Pair of positive 30Hz wavelets with near maximum destructive interference,H.3alternating polarity 30Hz wavelets aligned so that maximum side lobes are coincident with zerocrossing of the trailing wavelet.A similar set of models was used by Huang and Milkereit (2009)in their comparison continuous wavelet transform,S-transform and Hilbert-Huang transform.We take their analysis further by examining Plancherel’s theorem and marginal conditions.The results of our test of Plancherel’s theorem of the conservation of total energy is given in Table 1;where total trace energy is the total energy of the trace prior to spectral decomposition,and the total marginal energy is the total energy in the time-frequency spectrum after spectral decomposition and the ratio of theenergies.Figure 1—Wedge model,used for testing,consisting of a sand (Vp ؍2880m/s,Vs ؍1380m/s,density ؍2.15g/cc)between two shales (Vp ؍2370m/s,Vs ؍980m/s,density ؍2.310g/cc)with a 30Hz Ricker wavelet.The model consists of 250traces and the sand has a thickness range from 0.0to 52.8ms.Time sample spacing is 1.0ms.Figure2—Test trace composed of Ricker wavelets in various states of interference(A–H).Panel A is S-transform with1.4resolution ratio,panel B is matching pursuit and panel C is Hilbert-Huang Transform spectral decomposition of the test signal in panel D.The plots in each panel are clockwise from upper left time marginal condition,time-frequency transform and frequency marginal condition.Blue line is the values derived from the trace and red line is the values derived from the transform.MP,with a ratio of 1.07,has the second best energy conservation results,but we found that the energy ratio is higher than the stop ratio for the residual energy (0.99).We see that the difference is a side effect of the method that results as wavelets are removed from the trace the trace,the spectrum becomes white,causing the dictionary to fit later wavelets poorly,and this results in the creation of energy in the output that is not present in the input trace.The EMD-HHT method with a ratio of 1.72has the worst energy conservation;this is a result of the gaps in the trace violating the algorithmic assumption of a continuous signal and its connection of peaks to peaks and of troughs to troughs across the gaps results in the creation of energy in the gaps as seen in Figure 2.The gaps could be handled by separating the trace into short segments containing the only parts in which we have interest,or by changing to (EEMD)ensemble empirical mode decomposition (Wu and Huang,2009)or another noise assisted method;added noise would help the method track through the gaps as indicated by the smaller ratio for 2000iterations of EEMD-HHT in Table 1.The S-transform method produced both the best and worst results.When the resolution ratio described by Pinnegar and Mansinha (2003)was set to 1.0,a poor result with a ratio of 1.43was obtained,and then a very good result of 1.01was obtained when the resolution ratio is set to 1.4as shown in Table 1and Figure 2.We found that when the resolution ratio is increased,the S-transform favors frequency resolution over time resolution.Examination of the time marginal condition plots in Figure 2showed that all three methods approx-imated the time marginal condition at the peaks of instantaneous energy and that the S-transform and EMD-HHT did poorly in the lows.Consistent with the energy conservation test,the best result is produced by MP.The S-transforms response can be explained by Gabor uncertainty where the lower the frequency that is analyzed,the more that the energy is spread into the gap.We found that the S-transform fit at the peaks can be improved by lowering the resolution ratio at the cost of reduced energy conservation.The frequency marginal conditions test results in Figure 2are interesting.Consistent with expectations from energy conservation,MP does best at satisfying the marginal condition.The EMD-HHT response has a statistical character consistent with the concept of frequency likelihood as discussed above;and the marginal spectrums bandwidth is closest to the spectra of the Ricker wavelets used in the model.Low frequency spectral power is over predicted as a result of the low frequency energy added to the gaps.The S-transform followed the power spectrum at low to intermediate frequencies and slightly over-predicted at high frequencies.The time-frequency spectra of the Ricker wavelets used in the model have symmetric envelopes and the clusters of reflections are also symmetric so therefore we expected the spectral representation from the spectral decompositions to also be symmetric in time;our results for the S-transform and EMD-HHT are consistent with our expectations.As expected from the marginal frequency plots,EMD-HHT showed aTable 1—Plancherel’s Theorem TestRicker Wavelet Combination TraceNorth Sea Trace MethodTotal Trace Energy Total Marginal Energy Ratio Marginal /Trace Total Trace Energy Total Marginal Energy Ratio Marginal /Trace S-Transform(res ϭ1.0)2.4086e103.4420e10 1.4291 2.6834e15 3.8347e15 1.4290S-Transform(res ϭ1.4)2.4086e10 2.4425e10 1.0141 2.6834e15 2.7212e15 1.0141MatchingPursuit2.4086e10 2.5890e10 1.0749 2.6831e15 2.8498e15 1.0621EMD-HHT2.4086e10 4.1534e10 1.7244 2.6834e15 2.5552e150.9522EEMD-HHT (nϭ2000) 2.4086e10 2.7899e10 1.1583 2.6834e15 2.8356e15 1.0567Figure3—Test trace derived from a North Sea seismic data set.Panel A is S-transform with1.4resolution ratio,panel B is matching pursuit and panel C is Hilbert-Huang Transform spectral decomposition of the test signal in panel D.The plots in each panel are clockwise from upper left time marginal condition,time-frequency transform and frequency marginal condition.Blue line is the values derived from the trace and red line is the values derived from the transform.high frequency limit that was lower than the other methods.However,the MP time-frequency spectra are asymmetric and we found this to be a side effect of path dependence and greed of the algorithm.Wavelets A,B and D were well resolved by all methods,whereas wavelets C and F were partially resolved at high frequencies by the S-transform and very poorly resolved by MP,the stacked wavelets in E were best resolved by MP,wavelets in H were only partially resolved by all three methods and the wavelets in G were unresolvable by any of the methods tested.Spectral notches in the S-transform indicated the presence of interfering wavelets.The S-transform results can be improved if resolution ratio is decreased from the1.4used in Figure1.The second single trace example is a seismic trace from amplitude preserving processed North Sea dataset.The trace is3s long sampled at4ms,the data was amplitude preserving processed and has and bandwidth of5-70Hz.The results of our test of Plancherel’s theorem on the North Sea trace are given in Table1.In this case the estimates of total energy of the trace had a small variation between methods due to differences in the padding and tapering imposed by the various methods.The variation is suppressed in the previous example due to the zeros at the ends of the trace.MP with a ratio of1.06had the second poorest energy conservation and the energy ratio was higher than the stop ratio for the residual energy(0.99).The EMD-HHT method with a ratio of0.9522was much better than in the previous synthetic wavelet example and appears to under conserve energy.In this case the EEMD energy ratio after2000iterations was1.06;a ratio higher than1.0was expected due to the incomplete canceling of the random noise.The S-transform method had the best and poorest conservation and is identical to ratios in the first synthetic wavelet example.Examination of the time marginal condition plots in Figure3showed that all three methods approx-imate the time marginal condition at the peaks of instantaneous energy and vary in their ability to follow the troughs.While S-transform and EMD-HHT did more poorly in the troughs,MP seems to do much better,but MP failed to find a complete solution at between2.7and3.0s,and again in other low instantaneous energy parts of the trace.The failure of MP is caused by use of envelope maxima for selection of extraction points as described in published algorithms including Liu and Marfurt(2005)and Wang(2007).As a result the algorithm spent too much of its energy budget attacking residual white noise with large envelope values so that by the time it reached the level of the quiet part of the trace it had already reached its stopping condition of0.99of the original energy removed from the residual trace. Changing the stopping criteria improves the energy extraction at the trace end,but at the expense of producing obvious artifacts in other parts of the spectrum;one such artifact detected were basket weave patterns that were created by removal of wavelets with long time durations when compared to their bandwidth.Basket weave patterns in general would have been more prevalent in the results had wavelet scale(0.3–1.5)and energy removal levels not been optimized to avoid them.EMD-HHT and S-transform produce similar results to each other which include solutions for times between2.7and3.0s.The frequency marginal condition test results in Figure3are interesting.The S-transform approxi-mately satisfied the condition for frequencies between0and70Hz but over predicted energy in frequencies between70Hz and Nyquist.MP results were similar to the S-transform except that MP also over predicted energy in the lows below6Hz.EMD-HHT response has a statistical character which stayed within the apparent bandwidth of the trace and formed a cloud of points centered along the maxima of the reference spectrum and became poorly defined at higher frequencies where there were only a few samples.The time-frequency spectra of all three methods reproduce the major features of the North Sea trace between0.5and2.7s,as seen in Figure3.The S-transform spectrum contains low frequencies before0.5 s as a result of a step change in trace amplitude.MP did not find a complete time-frequency spectrum for the interval between2.7and3.0s where the trace was low amplitude.EMD-HHT produced the most consistent upper limit on frequency bandwidth;and the higher power,high frequency excursions in the S-transform and MP are likely due to Gabor time-frequency uncertainty.All three methods showedFigure4—Power spectra along horizon slices from wedge model in Figure1.The columns from left to right are S-transform with1.0resolution ratio, matching pursuit and Hilbert Huang transform results.The rows from top to bottom are spectra along top positive reflection,zero crossing at center of wedge and bottom negative reflection.apparent frequency attenuation with increasing travel time,however,the amount is method dependent.MP results suggested that the highest attenuation was likely due to the intrinsic path dependence of the solution.S-transform and EMD-HHT methods show similar amounts of attenuation for a fixed frequency. The type of MP spectral distortion seen in the first example was less evident in the real trace;however we expect it to be present.Wedge ModelsApplication of the time-frequency methods to our wedge model produced the diverse set of responses shown in Figure4.These responses were generated by extracting the time-frequency response at each trace along horizon slices located at the peak associated with the top of the wedge,the trough associated with the base of the wedge and the zero crossing associated with centerline of the wedge.The S-transform responses were the bandlimited equivalent to those described by Gridley and Partyka (1998)for wedge models using short windowed discrete Fourier transforms with spectral peaks and notches as described by Equations5and6.The locations of the spectral peaks and notches can be used to infer time thickness of the wedge.MP response was similar to the first harmonic of the S-transform for wedge thicknesses less than30 ms,but when the wedge was thicker than30ms,the energy of the center line horizon is negligible and the top and base responses were smooth with a ridge centered near the30Hz frequency of the Ricker wavelet.Unfortunately the spectra produced by MP are unstable due to the path dependence and greediness of MP algorithm.Several methods have been proposed for multichannel stabilization of MP including those discussed by Wang(2010)and Durka(2007);in general these stabilization methods look for the best common wavelet at a particular time over a group of traces,but they assume also that there are no significant nonlinear time relationships between traces(e.g.faults,bedding,or other abrupt character changes),which may limit their usefulness in typical seismic data containing those features,and furthermore these methods increase the continuity of the spectra but still do not reduce the path dependent distortion recognized in the first example.EMD-HHT produced a focused and simultaneously very sparse response.The spectra were dominated by the responses of the first and second IMF.The obvious feature of the EMD-HHT spectra was the discontinuity or singularity at25ms.This feature was located between tuning(12.6ms TWT)and the position of the instantaneous frequency singularity(31.7ms TWT);the time thickness suggests that it may be associated with the half-wavelength one way time thickness of the wedge which is the approximate point at which side lobes between top and base start to appear as the wedge thickens.If this feature were to be isolated in seismic sections it could provide a useful relative thickness indicator. ConclusionsWe have analyzed the characteristics of S-transform,EMD-HHT,and MP spectral decompositions from the perspective of their potential usefulness in quantitative interpretation:S-transform based methods have desirable characteristics of easy parameter tuning to satisfy Plancher-el’s theorem and a wedge model response consistent with peak and notch characteristics described by Marfurt and Kirlin(2001).S-transform methods approximately satisfy the marginal conditions by following the peaks of the time marginal and approximating the frequency marginal within the bandwidth of the trace.Unfortunately the methods add excess energy to the spectra outside of the data bandwidth.EMD-HHT produced a very sparse time-frequency spectrum with characteristics driven by the signal; its frequency marginal had a statistical appearance with the best limitation on bandwidth.Wedge model response was sparse with only a few IMFs dominating.A major observation was a frequency discontinuity associated with the half-wavelength thickness of the wedge.As EMD-HHT is based on an algorithm it lacks a firm theoretical basis.。
纹理物体缺陷的视觉检测算法研究--优秀毕业论文
摘 要
在竞争激烈的工业自动化生产过程中,机器视觉对产品质量的把关起着举足 轻重的作用,机器视觉在缺陷检测技术方面的应用也逐渐普遍起来。与常规的检 测技术相比,自动化的视觉检测系统更加经济、快捷、高效与 安全。纹理物体在 工业生产中广泛存在,像用于半导体装配和封装底板和发光二极管,现代 化电子 系统中的印制电路板,以及纺织行业中的布匹和织物等都可认为是含有纹理特征 的物体。本论文主要致力于纹理物体的缺陷检测技术研究,为纹理物体的自动化 检测提供高效而可靠的检测算法。 纹理是描述图像内容的重要特征,纹理分析也已经被成功的应用与纹理分割 和纹理分类当中。本研究提出了一种基于纹理分析技术和参考比较方式的缺陷检 测算法。这种算法能容忍物体变形引起的图像配准误差,对纹理的影响也具有鲁 棒性。本算法旨在为检测出的缺陷区域提供丰富而重要的物理意义,如缺陷区域 的大小、形状、亮度对比度及空间分布等。同时,在参考图像可行的情况下,本 算法可用于同质纹理物体和非同质纹理物体的检测,对非纹理物体 的检测也可取 得不错的效果。 在整个检测过程中,我们采用了可调控金字塔的纹理分析和重构技术。与传 统的小波纹理分析技术不同,我们在小波域中加入处理物体变形和纹理影响的容 忍度控制算法,来实现容忍物体变形和对纹理影响鲁棒的目的。最后可调控金字 塔的重构保证了缺陷区域物理意义恢复的准确性。实验阶段,我们检测了一系列 具有实际应用价值的图像。实验结果表明 本文提出的纹理物体缺陷检测算法具有 高效性和易于实现性。 关键字: 缺陷检测;纹理;物体变形;可调控金字塔;重构
Keywords: defect detection, texture, object distortion, steerable pyramid, reconstruction
II
波谱分析英文翻译
Differences in Pulse Spectrum Analysis Between Atopic Dermatitis andNonatopic Healthy ChildrenAbstractObjectives: Atopic dermatitis (AD) is a common allergy that causes the skin to be dry and itchy. It appears at an early age, and is closely associated with asthma and allergic rhinitis. Thus, AD is an indicator that other allergies may occur later. Literatures indicate that the molecular basis of patients with AD is different from that of healthy individuals. According to the classics of Traditional Chinese Medicine, the body constitution of patients with AD is also different. The purpose of this study is to determine the differences in pulse spectrum analysis between patients with AD and nonatopic healthy individuals.Methods: A total of 60 children (30 AD and 30 non-AD) were recruited for this study.A pulse spectrum analyzer (SKYLARK PDS-2000 Pulse Analysis System) was used to measure radial arterial pulse waves of subjects.Original data were then transformed to frequency spectrum by Fourier transformation. The relative strength of each harmonic wave was calculated. Moreover, the differences of harmonic values between patients with AD and non-atopic healthy individuals were compared and contrasted.Results: This study showed that harmonic values and harmonic percentage of C3 (Spleen Meridian, according to Wang’s hypothesis) were significantly different. Conclusions: These results demonstrate that C3 (Spleen Meridian) is a good index for the determination of atopic dermatitis. Furthermore, this study demonstrates that the pulse spectrum analyzer is a valuable auxiliary tool to distinguish a patient who has probable tendency to have AD and/or other allergic diseases.IntroductionAtopic dermatitis (AD) is a common pruritic chronic inflammatory allergic disease. Approximately 10% of all children in the world are affected by atopicdermatitis,typically in the setting of a personal or family history of asthma or allergic rhinitis. It occurs in infancy and early childhood. Sixty percent (60%) of the symptoms manifest in the first year of life, and 85% by 5 years of ag e. Early onset and close association with other atopic conditions, such as asthma and allergic rhinitis, make atopic dermatitis an excellent indicator that other allergies may occur later.A number of observations suggest that there is a molecular basis for atopic dermatitis; these include the findings of genetic susceptibility, immune system deviation, and epidermal barrier dysfunction. Moreover, according to the classics of Traditional Chinese Medicine, the body constitution of atopic dermatitis patients was also different. Establishment of scientific methods using pulse diagnosis will assist the diagnosis and follow-up of AD."Organs Resonance"brought up by Wei-Kung Wang provided a scientific explanation for "pulse condition" and "Qi." Organs, heart, and vessels can produce coupled oscil- lation, which minimize the resistance of blood flow, resulting in better circulation. The changes of radial arterial pulse spectrum can reflect the harmonic energy redistribution of a specific organ. Several of the previous stu dies demonstrate that variations in the harmonics of pulse spectrum can be used in many fields, including diseases, acupuncture,Chinese herbal medications and clinical observation. The new method offers an extraordinary vision of medical investigation by combining pulse spectrum analysis with Traditional Chinese Medicine as well as modern medicine. Wang proposed that the peak values of numbered harmonics might be the representations of each visceral organ,C1 for Liver, C2 for Kidney, C3 for Spleen, etc. Materials and MethodsSubjectsIn total, 60 children (3–15 years of age), comprising 30 with AD (AD group) and 30 nonatopic healthy (non-AD group),participated in the study. The diagnosis of AD was based on the criteria defined by the United Kingdom working party.Nonatopic healthy was defined as those who had no known health problems and no personal or family history of allergic diseases, such as asthma, allergic rhinitis, etc.The experiment protocol was approved by the Institutional Review Board of China Medical University (approval number: DMR97-IRB-087). The written informed consents were obtained from the parents of all participants before they enrolled in this study.Children with a history of major chronic diseases, such as arrhythmia, ardiomyopathy, hypertension, diabetes mellitus, chronic renal failure, hyperthyroidism, difficult asthma,malignancy, and so on were excluded from this study.Those who suffered from any acute disease (e.g., acute upper airway infection or acute gastroenteritis in recent 7days), were also excluded from this experiment. Radial arterial pulse testA pulse spectrum analyzer (SKYLARK PDS-2000 Pulse Analysis System, approved by Department of Health, Executive Yuan, R.O.C. [Taiwan] with a license number 0023302) was used to record radial arterial pulse waves. The pressure transducer of the pulse spectrum analyzer detected artery pressure pulse with 100-Hz sampling rate and 25mm/ sec scanning rate. The output data were stored in digital form in an IBM PC. The subjects were asked to rest for 20 minutes prior to pulse measurements. All procedures were performed in a bright and quiet room with a constant temperature of 258C–268C. Pulses were recorded during 3:00 pm–5:00 pm to avoid the fasting or ingestion effect.Data processingWe transformed original data to spectrum data by Fourier transform as Wang et al described earlier.Briefly, original data were stored as time-amplitude. Mathematics software Matlab 6.5.1 (The MathWorks Inc.) provided Fast Fourier Transformation (FFT) technique to transform time-amplitude data to frequency-amplitude data. Then regular isolated harmonic in a multiple of fundamental frequency appeared.Thefinding gave a spectrum reading up to the 10th harmonic (Cn, n¼0–10). Intensity of harmonics above the 11th became very small and was neglected. Thereafter, the relative harmonic values of each harmonic were calculated ac-cording to Wang’s hypothesis.Harmonic percentage of Cn was defined asStatistical analysisThe experimental data were analyzed by Statistical software SPSS 13.0 for Windows (SPSS Inc.). Comparisons of the harmonic values and the harmonic percentage and the agedistribution between patients with AD and nonatopic healthy individuals were performed using the Student's two samples t test. Comparisons of the sex distribution between patients with AD and nonatopic healthy individuals were performed using the X2 test. Comparisons of the harmonic values and the harmonic percentage between left hand and right hand were performed using the Student's pairedsamples t test. All comparisons were two-tailed, and p<0.05 was considered to be statistically significant.ResultsIn total, 60 children (30 AD and 30 non-AD) participated in the study. The average age of the 60 subjects is 8.02+2.95 years. Baseline characteristics of all participants are shown in Table 1. There is no significant difference in age and gender between the two groups.Relative harmonic values of right radial arterial pulse spectrum analysis are shown in Table 2. Relative harmonic values of left radial arterial pulse spectrum analysis are shown in Table 3. Harmonic percentages of right radial arterial pulse spectrum analysis are shown in Table 4. Harmonic percentages of left radial arterial pulse spectrum analysis are shown in Table 5.In this study, the relative harmonic values of both right and left radial arterial pulse spectrum analysis are lower in the AD group. The relative harmonic values of C3 are significantly different ( p¼0.004, 0.059, respectively). Moreover, when comparingthem by parameter of harmonic percent age, C3 are significantly decreased in the AD group in both right and left radial arterial pulse spectrum analyses ( p¼0.045, 0.036, respectively). These results illustrated the close relationship between C3 (SpleenMeridian) and AD.DiscussionAccording to the theory of Traditional Chinese Medicine,the pathophysiologic mechanisms of AD are "inborn deficiency in body constitution, poor tolerance to environmental stimulants, Spleen Meridian not working well, interiorly generating wet and heat; infected with wind-wetness-heat-evil further, then suffering from those accumulating in skin." AD is a disease involving multiple dysfunctions of the visceral organs (Zang-Fu) rather than a constitutive skin defect.‘‘Spleen wetness’’ is u sually considered a major syndrome of AD, which is compatible with our findings.On the other hand, there are also differences in C0 (Heart Meridian), C1 (Liver Meridian), C4 (Lung Meridian) of right hand ( p¼0.014, 0.005, 0.021, respectively) and C1 (Liver Meridian) of left hand ( p¼0.038) between the two groups.These findings appear to have a close relationship between AD and other visceral organs (Zang-Fu). It requires further research to clarify the clinical meanings of these differences.In the present experiment, the close relationship between C3 (Spleen Meridian, referred toWang’s hypothesis) and AD is illustrated. The result verifies Wang’s hypothesis about the relationship between harmonics and Meridians. Moreover,our experiment also has proved that the pulse spectrum analyzer is a suitable auxiliary tool for diagnosing and following up patients with AD.ConclusionsIn conclusion, it was determined that C3 (Spleen Meridian) is a valued index for the determination of atopic dermatitis. Also, the pulse spectrum analyzer is a practical noninvasive diagnostic tool to allow scientific and objective diagnosis.However, the pulse diagnosis technique is just in the beginning stage. Even though the discovery from the present study seems clear, it deserves further study. AcknowledgmentsThis research was performed in a private clinic for pediatrics specialty, the Hwaishen clinic. The Hwaishen Clinic is acknowledged for their full support of this research. Disclosure StatementNo competing financial interests exi st.bopufenxi2011@。
近红外光谱法英文
近红外光谱法英文Near-Infrared SpectroscopyNear-infrared spectroscopy (NIRS) is a powerful analytical technique that has gained widespread recognition in various scientific and industrial fields. This non-invasive method utilizes the near-infrared region of the electromagnetic spectrum, typically ranging from 700 to 2500 nanometers (nm), to obtain valuable information about the chemical and physical properties of materials. The versatility of NIRS has led to its application in a diverse array of industries, including agriculture, pharmaceuticals, food processing, and environmental monitoring.One of the primary advantages of NIRS is its ability to provide rapid and accurate analysis without the need for extensive sample preparation. Unlike traditional analytical methods, which often require complex sample extraction and processing, NIRS can analyze samples in their natural state, allowing for real-time monitoring and decision-making. This efficiency and non-destructive nature make NIRS an attractive choice for applications where speed and preservation of sample integrity are crucial.In the field of agriculture, NIRS has become an invaluable tool for the assessment of crop quality and the optimization of farming practices. By analyzing the near-infrared spectra of plant materials, researchers can determine the content of various nutrients, such as protein, carbohydrates, and moisture, as well as the presence of contaminants or adulterants. This information can be used to guide precision farming techniques, optimize fertilizer application, and ensure the quality and safety of agricultural products.The pharmaceutical industry has also embraced the use of NIRS for a wide range of applications. In drug development, NIRS can be used to monitor the manufacturing process, ensuring the consistent quality and purity of active pharmaceutical ingredients (APIs) and finished products. Additionally, NIRS can be employed in the analysis of tablet coatings, the detection of counterfeit drugs, and the evaluation of drug stability during storage.The food processing industry has been another significant beneficiary of NIRS technology. By analyzing the near-infrared spectra of food samples, manufacturers can assess parameters such as fat, protein, and moisture content, as well as the presence of adulterants or contaminants. This information is crucial for ensuring product quality, optimizing production processes, and meeting regulatory standards. NIRS has been particularly useful in the analysis of dairy products, grains, and meat, where rapid and non-destructive testing is highly desirable.In the field of environmental monitoring, NIRS has found applications in the analysis of soil and water samples. By examining the near-infrared spectra of these materials, researchers can obtain information about the presence and concentration of various organic and inorganic compounds, including pollutants, nutrients, and heavy metals. This knowledge can be used to inform decision-making in areas such as soil management, water treatment, and environmental remediation.The success of NIRS in these diverse applications can be attributed to several key factors. Firstly, the near-infrared region of the electromagnetic spectrum is sensitive to a wide range of molecular vibrations, allowing for the detection and quantification of a variety of chemical compounds. Additionally, the ability of NIRS to analyze samples non-destructively and with minimal sample preparation has made it an attractive choice for in-situ and real-time monitoring applications.Furthermore, the development of advanced data analysis techniques, such as multivariate analysis and chemometrics, has significantly enhanced the capabilities of NIRS. These methods enable the extraction of meaningful information from the complex near-infrared spectra, allowing for the accurate prediction of sample propertiesand the identification of subtle chemical and physical changes.As technology continues to evolve, the future of NIRS looks increasingly promising. Advancements in sensor design, data processing algorithms, and portable instrumentation are expected to expand the reach of this analytical technique, making it more accessible and applicable across a wider range of industries and research fields.In conclusion, near-infrared spectroscopy is a versatile and powerful analytical tool that has transformed the way we approach various scientific and industrial challenges. Its ability to provide rapid, non-invasive, and accurate analysis has made it an indispensable technology in fields ranging from agriculture and pharmaceuticals to food processing and environmental monitoring. As the field of NIRS continues to evolve, it is poised to play an increasingly crucial role in driving innovation and advancing our understanding of the world around us.。
高光谱遥感信息中的特征提取与应用研究(中英对照)
Spectral Features Extraction in Hyperspectral RS Data andIts Application to Information ProcessingOriented to the demands of hyperspectral RS information processing and applications, spectral features in hyperspectral RS image can be categorized into three scales: point scale, block scale and volume scale. Based on the properties and algorithms of different features, it is proposed that point scale features can be divided into three levels: spectral curve features, spectral transformation features and spectral similarity measure features. Spectral curve features include direct spectra encoding, reflection and absorption features. Spectral transformation features include Normalized Difference of Vegetation Index (NDV I) , derivate spectra and other spectral computation features. Spectral similarity measure features include spectral angle ( SA ) , Spectral Information Divergence ( SID ) , spectral distance, correlation coefficient and so on. Based on analysis to those algorithms, several problems about feature extraction, matching and application are discussed further, and it p roved that quaternary encoding, spectral angle and SID can be used to information processing effectively.1 IntroductionHyperspectral Remote Sensing was one of the most important breakthroughs of Earth Observation System ( EOS) in 1990 s. It overcomes the limitations of conventional aerial and multispectral RS such as less band amount, wide band scope and rough spectral information expression, and can provide RS information with narrow band width, more band amount and fine spectral information, also it can distinguish and identify ground objects from spectral space, so hyperspectral RS has got wide applications in resources, environment, city and ecological fields. Because hyperspectral RS is different from conventional RS information obviously in both information acquisition and information processing, there are many problems should be solved in practice. One of the most important problems isabout spectral features extraction and application in hyperspectral RS data including hyperspectral RS image and standard spectral database. Nowadays, studies on hyperspectral are mainly focused on band selection and dimensionality reduction, image classification, mixed pixel decomposition and others, and studies on spectral features are few. In this paper, spectral features extraction and application will be taken as our central topic in order to provide some useful advices to hyperspectral RS applications.2 Framework of spectral features in hyperspectral RS dataIn general, hyperspectral RS image can be expressed by a spatial-spectral data cube ( Fig. 1). In this data cube, every coverage expressed the image of one band, and each pixel forms a spectral vector composed of albedo of ground object on every band in spectral dimension, and that vector can be visualized by spectral curve ( Fig. 2 ). Many features can be extracted from spectral vector or curve, and spectral features are the key and basis of hyperspectral RS applications. Also each spectral curve in spectral database can be analyzed with same method. Although there are some algorithms to compute spectral features, the framework and system is still not obvious, so we would like to propose a framework for spectral features in hyperspectral RS data including hyperspectral RS image and standard spectral database.2. 1Three scales of spectral featuresAccording to the operational objects of extraction algorithms, spectral features can be categorized into three scales: point-scale,block-scale and volume-Scale.Point scale takes pixel and its spectral curve as operational object and some useful features can be extracted from this spectral vector (or spectral curve).In general, hyperspectral RS image takes spectral vector of each pixel as processing object.Block scale is oriented image block or region. Block is the set of some pixels, and it can be homogeneous or heterogeneous. Homogeneous regions are got by image segmentation and pixels in this region are similar in some given features; heterogeneous region are those image blocks with regular or irregular size, and they are cut from original image directly, for example, an image can be segmented according to quadtree method. In hyperspectral RS image, block scale features can be computed from two aspects. One is to compute texture feature of a block on some characterized bands, and the other is to compute spectral feature of a block. If the block is homogeneous its mean vector can be computed firstly and then spectral of this mean vector can be extracted to describe the block. If the block is heterogeneous, it can be segmented to some homogeneous blocks.Volume scale combines spatial and spectral features in a whole and extracts features in 3D ( row, column and spectra ) space. Here, some 3D operational algorithms are needed, for example, 3D wavelet transformation and high order Artificial Neural Network (ANN ). Because this type of features is difficult to compute and analyze, we don′t research it in current studies.In this paper, we would like to focus on point scale feature, or those features extracted from spectral vector that may be spectral vector of a pixel or mean vector of a block.2. 2Three levels of point scale featuresFrom operation object, algorithm principles, feature properties, application modes and other aspects, we think it is feasible to categorize spectral features into three levels: spectral curve features, spectral transformation features and spectral similarity measure features. They are corresponding to analysis on spectral curve with all bands, data transformation and combination with partof all bands and similarity measure of spectral vectors. In our study, data from OM IS and PHI hyperspectral image, USGS spectral database and typical spectra data in China is experimented and two examples are given in this paper. One is to select three regions from PH I image (Region I is vegetation, Region II is built-up land, and Region III is mixed region of some land covers) , and the other is spectral curve of three ground objects from USGS spectral database, among them S1 is Actinolite_HS22. 3B, S2 is Actinolite_HS116. 3B and S3 is Albite_HS66. 3B, so S1 and S2 are similar and they are different from S3.3 Spectra l curve featuresSpectral curve features are computed by some algorithms based on the spectral curve of certain pixel or ground object, and it can describe shape and properties of the curve. The main methods include direct encoding and feature band analysis.3. 1 Direct encodingThe important idea of spectral curve feature is to emphasize spectral curve shape, so direct encoding is a very convenient method, and binary encoding is used more widely. Its principle is to compare the attribute value at each band of a pixel with a threshold and assign the code of “0”or “1”according to its value. That can be expressed byHere, []s i is code of the ith band, i X is the original attribute valueof this band, and T is the threshold. Generally, threshold is the mean of spectral vector, and it can also be selected by manual method according to curve shape, sometimes median of spectral vector is probably used.Only one threshold is used in binary encoding, so the divided internal is large and precision is low. In order to improve the appoximaty and precision, the quaternary encoding strategy is proposed in this paper. Its primary idea is as follows: ( 1 ) the mean of the total pixel spectral vector is computed and denoted by T 0 , and the attribute is divided into two internal including [min X ,[]()1i if X T s i o else≥⎧=⎨⎩0T ] and [0T , min X ]; (2) the pixels located in the two internalsare determined and the mean of each internal is got and donated by T and TR , so four internals are formed including [min X , TL ], [0T , TR ] and [TR , min X ]; ( 3) each band is assigned one of the code sets{ 0, 1, 2, 3 } according to the internal it is located; (4) to compute the ratio of matched bands number to the total band number as final matching ratio. It p roved that quaternary encoding could describe the curve shape more precisely.If quarternary encoding is used, the ratio of the same region is smaller than binary encoding, but the ratio between different regions decreased dramatically. So quarternary encoding is more effective in measuring the similarity between different pixels.Because direct encoding will disperse the continuous albedo into discrete code, the encoding result is affected by threshold obviously and will lead to information loss. Although its operation is very simple, it is only used to some applications requiring low precision, and the threshold should be selected according to different conditions.3. 2 Spectral absorption or reflection featureDiffering from direct encoding in which all bands are used, spectral absorption or reflection feature only emphasizes those bands where valleys or apexes are located. That means those bands with local maximum or minimum in spectral curve should be determined at first and then further analysis can be done. In general, albedo is used to describe the attribute of a pixel, so those bands with local maximum are reflection apex and those with local minimum are absorption valley.After the location and related parameters are got, the detail analysis can be done. In general two methods are used, one is to give direct encoding and analysis to feature bands, and the other is to compute some quantitative index using feature bands and their parameters.3.3 Encoding of spectra l absorption or reflection features The locations of feature bands are directly used in spectral feature encoding. The following will take absorption feature as anexample. If one band is the location of absorption valley, its code will be “1 ”, otherwise its code is “0 ”. After the encoding is completed further matching and comparison can be done. Because of those uncertainties and errors in hyper spectral imaging process, the locations of feature bands perhaps move in near bands, and that will lead to low match ratio. In order to reduce the impact of band displacement, the extended encoding method is proposed and used in this paper. Its idea is that if the code of a certain band is“1”then the bands prior to and behind it will be assigned the same code “1”, and then matching and analysis will be done.The similarity measure to code vector is matching by bit. The matching ratio is got by the ratio of matched bands to total band count. In this study, two match schemes are used. One is matching the code of all bands and the other is only matching those feature bands.Based on above analysis, four schemes are used and compared. These are: ( 1) direct encoding to all bands and matching by all bands, and ( 2 ) direct encoding to all bands and matching only by feature bands, and ( 3) extended encoding and matching by all bands, and ( 4 ) extended encoding and matching only by feature bands.From above analysis and comparison to spectral absorption and reflection feature encoding and matching, it can be found that although absorption and reflection band can describe the spectral properties of ground object, effective matching operation should be used in order to overcome the impacts of noise, band displacement and other factors. In practical applications, absorption and reflection can be used to extract thematic information and retrieve a certain type of object effectively.Based on spectral absorption and reflection features, the spectral absorption index ( SA I) or spectral reflection index ( SR I) can be computed by wavelength, albedo of feature band and its left and right shoulders, and those indexes can describe spectral feature more precisely on some occasions.4 Spectra l computation and transformation featuresBoth correlativity and mutual compensation exist in differentbands of hyper spectral RS information, so many new features can be got by certain computation and combination to some bands and used to classification, information extraction and other tasks.4. 1 Normalized difference of vegetation index (NDVI)NDVI plays very important roles in hyper spectral application. It can describe some fine information about vegetation such as Leaf Area Index (LA I) , ratio of vegetation and soil, component of vegetation and so on. In some classifiers ( for example, ANN classifier) NDVI usually is used as an independent feature in classification.4. 2Derivative spectrumDerivative spectrum is also called as spectral derivative technique. One rank and two rank derivative spectrum can be computed by Equation.Each rank derivative spectrum can be computed using algorithms similar to above. After derivative computation is end, we can find that each type of ground object may have some features distinguished from other entities in a certain rank derivative spectrum and that can be used to identify information. Sometimes derivative spectrum image can be used as the input of classifier directly. Although spectral derivative can provide new features in addition to original information, some new images will be formed after derivative operation and that will increase data volume dramatically. Form rank derivative spectrum, N - 2M bands will be formed, so how to process relationship between data volume and efficiency becomes a new question.5Conclusions and discussionsIn this paper, oriented to the demands of hyper spectral RS information processing to spectral features, the framework of spectral features is proposed and some major feature extraction algorithms and their applications are discussed, and some improvement, experiments and analysis are finished. From the studies in this paper, the following conclusions can be drawn:1 ) Based on the extraction principle and algorithm, spectral features in hyper spectral RS information can be categorized intothree levels: spectral curve features, spectral transformation and computation features and spectral similarity measure features. This framework is useful for further analysis and applications.2) As the common style of pixel spectral vector, some features can be extracted and used. The algorithm and computation of binary encoding is simple and easy but it will lead to loss of some detail information. Quaternary encoding can describe curve features with high rescission and be used to matching, retrieval and other work. The reflection and absorption features based on spectral curve have wide applications in retrieval, thematic information extraction and other tasks, but effective matching strategy must be adopted in order to control errors. In this paper two new app roaches including extended encoding and matching and combined matching of reflectance and absorption features are proposed and it p roved that they can get better results than traditional methods in feature measure.3) As the main computation and transformation features, NDV I and derivative spectrum can provide new features participating in classification, extraction and other processing and extract those useful patterns and information hidden behind original data, so they are very useful in hyper spectral RS information processing.4) For those spectra similarity measure indexes, Spectral Angle and SID are more effective than traditional indexes because they can measure the similarity more precisely, so they are usually used to classification, clustering and retrieval.Some topics about the feature extraction and application of spectral feature are discussed in this paper. Our further studies will be focused on classification, object identification and thematic information extraction in hyper spectral RS information and the specific application modes of different spectral features in order to promote the development of hyper spectral RS application.高光谱遥感信息中的特征提取与应用研究面向高光谱遥感信息处理和应用的需求,在高光谱遥感图像的光谱特征可分为三个尺度:点规模,块规模和数量规模。
吸收光谱简介 Absorption Spectrum An Introduction 英语作文论文
吸收光谱简介Absorption Spectrum AnIntroductionWhat is Absorption Spectrum?The absorption spectrum of a material can be defined as the fraction of the incident radiation which is absorbed by that material over a wide range of frequencies. The molecular and atomic composition of a material is used to determine the absorption spectrum. Fundamental radiation is generally observed at those frequencies which get mixed with the energy difference that takes place between two mechanical states of the molecules.The absorption takes place because of the transition between these two states and it is known as the absorption line. The spectrum is composed of several absorption lines. The frequencies where such absorption lines develop along with their relative intensities generally depend on the molecular structure and electronic structure of the sample. The frequencies also depend on molecular interactions. In the sample, the crystal structure is found in solids and on different environmental factors like pressure, temperature, electromagnetic fields, etc.What is Absorption Spectrum?Assingment Experts will explain Absorption Sepctrum in deatils. The absorption spectrum of a material can be defined as the fraction of theincident radiation which is absorbed by that material over a wide range of frequencies. The molecular and atomic composition of a material is used to determine the absorption spectrum. Fundamental radiation is generally observed at those frequencies which get mixed with the energy difference that takes place between two mechanical states of the molecules.The absorption takes place because of the transition between these two states and it is known as the absorption line. The spectrum is composed of several absorption lines. The frequencies where such absorption lines develop along with their relative intensities generally depend on the molecular structure and electronic structure of the sample. The frequencies also depend on molecular interactions. In the sample, the crystal structureis found in solids and on different environmental factors like pressure, temperature, electromagnetic fields, etc.The absorption lines also possess a definite shape and width which are fundamentally determined by the density of states for spectral density of the system. Absorption lines are generally classified by the feature of quantum mechanical change taking place in an atom or molecule. Rotational states sometimes get changed and give result in the development of rotational lines which are found in the region of the microwave spectrum. On the other hand, vibrational lines in correspondence to vibrational state changes in the molecule are found in the area of infrared region. The electronic lines are composed of several changes taking place in the electronic state of a molecule or atom whichare found in the ultraviolet and visible region.It can be noticed that there are various dark lines in the sun’s spectrum. These lines are developed by the atmosphere of the Sun which absorbs light at different wavelengths resulting in different light intensity at the wavelength to appear dark. The molecules and atoms present in a gas absorb certain light wavelengths. The pattern of the lines is very unique with respect to each element which provides us information about the elements which help in making the sun’s atmosphere. The absorption spectra can be observed from spatial regions in the presence of a cooler gas line between in a hotter source and the earth.The absorption spectra can also be observed from the planets with atmospheres, stars, and galaxies. In analyzing the light of the Sun, aspectrometer is used. The spectrometer is a device which separates light by colour and energy. In separating light by colour and energy, the image of the spectrum of the sun gets created. This is quite similar to the absorption spectrum. The dark lines are the areas where the light gets absorbed by different elements present in the Sun’s outer layers. The lowest energy is represented by red light and the highest energy is represented by blue light.The black gaps or lines in the spectrum of the sun are termed as absorption lines. The gas present in the sun’s outer layers develops the absorption lines by absorbing the light. There are different elements such as Helium, hydrogen, carbon, and other smaller quantities of heavy elements in the sun. When the sunlight shines, the elements the energy gets absorbed by the atoms. The atoms can only absorb the lightrelevant to the energy the atoms need. The gaps in the spectrum of the Sun get developed and help in informing the formation of the sun. The emission spectrum is quite different from the absorption spectrum.In developing an absorption spectrum, the light needs to shine through a gas but in creating and emission spectrum a gas needs to be heated up. The atoms present in the gas get absorbed the energy only for a short tenure. The atoms get energetic and jiggled up by heating the gas because of the concentration of a high level of energy. The energy is emitted or re-released as light eventually. Absorption spectrum takes place when the light passes through a dilute and cold gas and characteristic frequencies get absorbed by the atoms present in the gas. The re-emitted light cannot be emitted in a similardirection which is followed by absorbed Photon because of which dark lines in the spectrum are created in the absence of light. The absorption spectrum is the dark lines. The absorption spectrum is defined as an Electromagnetic Spectrum in which the radiation intensity at some specific wavelengths gets decreased. An absorbing substance gets manifested as bands or dark lines. Medically, the absorption spectrum is also defined as an Electromagnetic Spectrum in which radiation intensity at specific ranges of wavelength is manifested as dark lines.X-ray absorptions are highly associated with the excitation taking place in the inner shell electrons in an atom. These changes generally get combined to develop a new absorption line which is typically found in the combined energy develop mainly during the changes. The changes are mainly radiation-vibrationstransitions. The energy which is typically found in the quantum mechanical change fundamentally determines the absorption line frequency. The frequency can get shifted because of several interactions. The magnetic and electric fields can give result in a shift.The interactions with some of the neighbouring molecules can also cause shifts. Absorption lines of any gas-phase molecule can get shifted typically when the molecule is present in either solid or liquid phase and involves in interacting with neighbouring molecules strongly. The shape and width of the absorption lines are generally determined by the observation instrument. The physical environment radiation and material absorbing of that material also determine the shape and width of absorption lines. Now our experts from Instant AssingnmentHelp will tell you about the relationship between Absorption Spectrum andThe relation between Transmission and absorption spectraTransmission and absorption spectra are interconnected. Transmission and absorption spectra are found to represent similar information. Transmission spectrum can be calculated from the absorption spectrum only. Absorption spectrum can also be calculated from transmission spectra. Mathematical transformation is used in calculating either the absorption spectrum or transmission spectrum. It has been observed that a transmission spectrum has maximum intensities where thewavelengths of the absorption spectrum are quite weak because of the transmission of more light through the sample takes place. Similarly, an absorption spectrum is found to have maximum intensities at its wavelengths where the absorption rate is quite stronger.The absorption spectrum is also related to any emission spectrum. Now, it is important to understand the concept of the emission spectrum. The process by which a substance can release energy is known as emission process. The energy which is released from a substance through any emission process can be found in electromagnetic radiation from. Emission can take at any frequency of absorption which makes the absorption lines to gets determined from the emission spectrum. But it is to be remembered that the emissionspectrum will always have different intensity pattern where it becomes distinguished from that of the absorption spectrum. Hence, it can be said that the absorption spectrum and emission spectrum can never be equivalent. The emission spectrum can be used to calculate the absorption spectrum with the application of effective theoretical models and other relevant information from where quantum mechanical states of a substance can be understood.Relationship between Absorption spectrum and reflection and scattering spectraThe absorption spectrum is also related to reflection and scattering spectra. The scattering and reflection spectra of any material getinfluenced by the absorption spectrum and index of refraction of that material. Extinction coefficient quantifies the absorption spectrum and index coefficients along with extinction coefficients which are related through Kramers-Kroening relation quantitatively. Therefore, it can be said that reflection or scattering spectrum standardize absorption spectrum can give rise to absorption spectrum.Reflection or scattering spectrum assumptions or models need to be simplified so that it can lead to effect an approximation of the derivation of absorption spectra. In the domain of chemical analysis, we can find the use of absorption spectroscopy because of the quantitative nature and specificity of the absorption spectrum. The specificity enables the compounds to get distinguished from each other in a mixture whichmakes absorption spectroscopy to be highly useful in different applications. For example, the presence of any pollutant in the air can be identified by the use of infrared gas analyzers.These analyses are also used to distinguish the air pollutant from oxygen, water, nitrogen, and other constituents. The specificity is also helpful in allowing several unknown samples to get rightly identified. It can be done by comparing the measured spectrum with the findings of reference spectra. It has been found that qualitative information of any sample can also be determined even if the information is not present in a library. For example, infrared spectra have several characteristics absorption bands which help in indicating the presence of carbon-oxygen bond or Carbon hydrogen bonds.Absorption spectrum can also be related to the quantity of material present with the use of Beer-Lambert law. This relationship is established quantitatively. In determining the typical compound concentration, it needs knowledge of the absorption coefficient of the compound. The absorption coefficient can be known from several reference sources and can be measured by accessing calibre standard spectrum with an available target concentrationabsorption spectrumAbsorption spectroscopy and its applicationAbsorption spectroscopy is one of the methods with the help of which a substance can get characterized by the support of wavelengths at which the spectrum of colour gets absorbedduring the passage of light through a substance solution. It is one of the fundamentally used methods used in assessing the chromospheres concentrations in the solutions. Absorption spectroscopy can also be explained as a non-destructive technique which is widely used by biochemists and biologists to assess the characteristic parameters and cellular components of functional molecules.This quantification is highly important in the domain of systems biology. In developing metabolic pathway quantitative depiction, various variables and parameters are needed which are to be assessed experimentally. Ultraviolet-visible absorption spectroscopy is used in producing experimental data which help in modelling techniques of system biology. These techniques use kinetic parameters andconcentrations of enzymes of signalling on metabolic pathways, fluxes, and intercellular metabolic concentrations. Absorption spectroscopy also describes the usage of the technique in quantifying bio-molecules and investigating bio-molecular interactions.Absorption spectroscopy is a significant technique which is used in chemistry to study simple inorganic species. It refers to spectroscopic techniques which are used in measuring radiation absorption as a function of wavelength or frequency when the interaction between absorption radiation and sample takes place. Photons are absorbed by the samples from the field of radiation. The absorption intensity varies as a frequency function and this absorption intensity is the absorption spectrum. Absorption spectroscopy is fundamentallyperformed across an absorption spectrum or electromagnetic spectrum.In the domain of analytical chemistry, absorption spectroscopy is used to assess the presence of any specific substance in a sample. In several cases, absorption spectroscopy is also used to quantify the quantity of a substance. In the domain of analytical applications, ultraviolet-visible and infrared spectroscopy is commonly observed. In the study of atomic physics, remote sensing, molecular physics, and astronomical spectroscopy, the use of absorption spectroscopy are widely observed.There are various experimental approaches which are used to measure the absorption spectrum. The most commonly used arrangement is to guide the regeneratedradiation beam at the sample in detecting the radiation intensity passing through it. The transmitted energy can be applied in calculating the absorption. The sample arrangement source and detection technique are also very used quite significantly depending on the objective of the experiment and that of the frequency range.Advantages of absorption spectroscopyThere can be several advantages of absorption spectroscopy because it can be used as an analytical method where measurements can be accomplished without any contact between the sample and the instrument. Radiation which travels between an instrument and a sample contains some important spectral information and measurement which is done remotely. Remote spectral sensing is quite significant indifferent situations. For example, hazardous and toxic environments can be measured without risking any instrument or operator.The material of the sample needs not to be brought into direct contact with any instrument which can prevent cross-contamination at a possible rate. Remote spectral measurements have certain challenges as compared to that of the laboratory measurements. To reduce such challenges, differential optical absorption spectroscopy has become quite popular because it mainly emphasizes on the features of differential absorption and erasers broadband absorption like the extinction of aerosol extinction because of Rayleigh scattering. This technique is used in airborne, ground-based, and satellite-based measuring actions. There are certain ground-based techniques whichprofile the possibilities of retrieving stratospheric and tropospheric trace gas profiles.The absorption lines also possess a definite shape and width which are fundamentally determined by the density of states for spectral density of the system. Absorption lines are generally classified by the feature of quantum mechanical change taking place in an atom or molecule. Rotational states sometimes get changed and give result in the development of rotational lines which are found in the region of the microwave spectrum. On the other hand, vibrational lines in correspondence to vibrational state changes in the molecule are found in the area of infrared region. The electronic lines are composed of several changes taking place in the electronic state of a molecule or atom which are found in the ultraviolet and visible region.Itcan be noticed that there are various dark lines in the sun’s spectrum. These lines are developed by the atmosphere of the Sun which absorbs light at different wavelengths resulting in different light intensity at the wavelength to appear dark. The molecules and atoms present in a gas absorb certain light wavelengths. The pattern of the lines is very unique with respect to each element which provides us information about the elements which help in making the sun’s atmosphere. The absorption spectra can be observed from spatial regions in the presence of a cooler gas line between in a hotter source and the earth.The absorption spectra can also be observed from the planets with atmospheres, stars, and galaxies. In analyzing the light of the Sun, a spectrometer is used. The spectrometer is adevice which separates light by colour and energy. In separating light by colour and energy, the image of the spectrum of the sun gets created. This is quite similar to the absorption spectrum. The dark lines are the areas where the light gets absorbed by different elements present in the Sun’s outer layers. The lowest energy is represented by red light and the highest energy is represented by blue light.The black gaps or lines in the spectrum of the sun are termed as absorption lines. The gas present in the sun’s outer layers develops the absorption lines by absorbing the light. There are different elements such as Helium, hydrogen, carbon, and other smaller quantities of heavy elements in the sun. When the sunlight shines, the elements the energy gets absorbed by the atoms. The atoms can only absorb the light relevant to the energy the atoms need. The gapsin the spectrum of the Sun get developed and help in informing the formation of the sun. The emission spectrum is quite different from the absorption spectrum.In developing an absorption spectrum, the light needs to shine through a gas but in creating and emission spectrum a gas needs to be heated up. The atoms present in the gas get absorbed the energy only for a short tenure. The atoms get energetic and jiggled up by heating the gas because of the concentration of a high level of energy. The energy is emitted or re-released as light eventually. Absorption spectrum takes place when the light passes through a dilute and cold gas and characteristic frequencies get absorbed by the atoms present in the gas. The re-emitted light cannot be emitted in a similar direction which is followed by absorbed Photonbecause of which dark lines in the spectrum are created in the absence of light. The absorption spectrum is the dark lines. The absorption spectrum is defined as an Electromagnetic Spectrum in which the radiation intensity at some specific wavelengths gets decreased. An absorbing substance gets manifested as bands or dark lines. Medically, the absorption spectrum is also defined as an Electromagnetic Spectrum in which radiation intensity at specific ranges of wavelength is manifested as dark lines.X-ray absorptions are highly associated with the excitation taking place in the inner shell electrons in an atom. These changes generally get combined to develop a new absorption line which is typically found in the combined energy develop mainly during the changes. The changes are mainly radiation-vibrations transitions. The energy which is typically foundin the quantum mechanical change fundamentally determines the absorption line frequency. The frequency can get shifted because of several interactions. The magnetic and electric fields can give result in a shift.The interactions with some of the neighbouring molecules can also cause shifts. Absorption lines of any gas-phase molecule can get shifted typically when the molecule is present in either solid or liquid phase and involves in interacting with neighbouring molecules strongly. The shape and width of the absorption lines are generally determined by the observation instrument. The physical environment radiation and material absorbing of that material also determine the shape and width of absorption lines. Now our experts from Instant AssingnmentHelp will tell you about the relationship between Absorption Spectrum andThe relation between Transmission and absorption spectraTransmission and absorption spectra are interconnected. Transmission and absorption spectra are found to represent similar information. Transmission spectrum can be calculated from the absorption spectrum only. Absorption spectrum can also be calculated from transmission spectra. Mathematical transformation is used in calculating either the absorption spectrum or transmission spectrum. It has been observed that a transmission spectrum has maximum intensities where thewavelengths of the absorption spectrum are quite weak because of the transmission of more light through the sample takes place. Similarly, an absorption spectrum is found to have maximum intensities at its wavelengths where the absorption rate is quite stronger.The absorption spectrum is also related to any emission spectrum. Now, it is important to understand the concept of the emission spectrum. The process by which a substance can release energy is known as emission process. The energy which is released from a substance through any emission process can be found in electromagnetic radiation from. Emission can take at any frequency of absorption which makes the absorption lines to gets determined from the emission spectrum. But it is to be remembered that the emissionspectrum will always have different intensity pattern where it becomes distinguished from that of the absorption spectrum. Hence, it can be said that the absorption spectrum and emission spectrum can never be equivalent. The emission spectrum can be used to calculate the absorption spectrum with the application of effective theoretical models and other relevant information from where quantum mechanical states of a substance can be understood.Relationship between Absorption spectrum and reflection and scattering spectraThe absorption spectrum is also related to reflection and scattering spectra. The scattering and reflection spectra of any material getinfluenced by the absorption spectrum and index of refraction of that material. Extinction coefficient quantifies the absorption spectrum and index coefficients along with extinction coefficients which are related through Kramers-Kroening relation quantitatively. Therefore, it can be said that reflection or scattering spectrum standardize absorption spectrum can give rise to absorption spectrum.Reflection or scattering spectrum assumptions or models need to be simplified so that it can lead to effect an approximation of the derivation of absorption spectra. In the domain of chemical analysis, we can find the use of absorption spectroscopy because of the quantitative nature and specificity of the absorption spectrum. The specificity enables the compounds to get distinguished from each other in a mixture whichmakes absorption spectroscopy to be highly useful in different applications. For example, the presence of any pollutant in the air can be identified by the use of infrared gas analyzers.These analyses are also used to distinguish the air pollutant from oxygen, water, nitrogen, and other constituents. The specificity is also helpful in allowing several unknown samples to get rightly identified. It can be done by comparing the measured spectrum with the findings of reference spectra. It has been found that qualitative information of any sample can also be determined even if the information is not present in a library. For example, infrared spectra have several characteristics absorption bands which help in indicating the presence of carbon-oxygen bond or Carbon hydrogen bonds.Absorption spectrum can also be related to the quantity of material present with the use of Beer-Lambert law. This relationship is established quantitatively. In determining the typical compound concentration, it needs knowledge of the absorption coefficient of the compound. The absorption coefficient can be known from several reference sources and can be measured by accessing calibre standard spectrum with an available target concentrationabsorption spectrumAbsorption spectroscopy and its applicationAbsorption spectroscopy is one of the methods with the help of which a substance can get characterized by the support of wavelengths at which the spectrum of colour gets absorbed during the passage of light through a substancesolution. It is one of the fundamentally used methods used in assessing the chromospheres concentrations in the solutions. Absorption spectroscopy can also be explained as a non-destructive technique which is widely used by biochemists and biologists to assess the characteristic parameters and cellular components of functional molecules.This quantification is highly important in the domain of systems biology. In developing metabolic pathway quantitative depiction, various variables and parameters are needed which are to be assessed experimentally. Ultraviolet-visible absorption spectroscopy is used in producing experimental data which help in modelling techniques of system biology. These techniques use kinetic parameters and concentrations of enzymes of signalling onmetabolic pathways, fluxes, and intercellular metabolic concentrations. Absorption spectroscopy also describes the usage of the technique in quantifying bio-molecules and investigating bio-molecular interactions.Absorption spectroscopy is a significant technique which is used in chemistry to study simple inorganic species. It refers to spectroscopic techniques which are used in measuring radiation absorption as a function of wavelength or frequency when the interaction between absorption radiation and sample takes place. Photons are absorbed by the samples from the field of radiation. The absorption intensity varies as a frequency function and this absorption intensity is the absorption spectrum. Absorption spectroscopy is fundamentallyperformed across an absorption spectrum or electromagnetic spectrum.In the domain of analytical chemistry, absorption spectroscopy is used to assess the presence of any specific substance in a sample. In several cases, absorption spectroscopy is also used to quantify the quantity of a substance. In the domain of analytical applications, ultraviolet-visible and infrared spectroscopy is commonly observed. In the study of atomic physics, remote sensing, molecular physics, and astronomical spectroscopy, the use of absorption spectroscopy are widely observed.There are various experimental approaches which are used to measure the absorption spectrum. The most commonly used arrangement is to guide the regeneratedradiation beam at the sample in detecting the radiation intensity passing through it. The transmitted energy can be applied in calculating the absorption. The sample arrangement source and detection technique are also very used quite significantly depending on the objective of the experiment and that of the frequency range.Advantages of absorption spectroscopyThere can be several advantages of absorption spectroscopy because it can be used as an analytical method where measurements can be accomplished without any contact between the sample and the instrument. Radiation which travels between an instrument and a sample contains some important spectral information and measurement which is done remotely. Remote spectral sensing is quite significant indifferent situations. For example, hazardous and toxic environments can be measured without risking any instrument or operator.The material of the sample needs not to be brought into direct contact with any instrument which can prevent cross-contamination at a possible rate. Remote spectral measurements have certain challenges as compared to that of the laboratory measurements. To reduce such challenges, differential optical absorption spectroscopy has become quite popular because it mainly emphasizes on the features of differential absorption and erasers broadband absorption like the extinction of aerosol extinction because of Rayleigh scattering. This technique is used in airborne, ground-based, and satellite-based measuring actions. There are certain ground-based techniques which。
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Driving factors for surface and web inspection in QA of manufacturing: • Detection of smaller defect sizes (< 10 microns) • Better reliability of inspection process (‘zero defect’) • Reduced cost by more efficient component use (faster scan for increased throughput) Impact on machine vision components: • increasing resolution of line scan cameras (4k, 8k, 12k, 16k, …) • smaller pixel sizes of line scan sensors (7 microns, 5 microns, 3.5 microns) • high performance optics for macro imaging
吸色程度不同英语表达
吸色程度不同英语表达Title: The Variability of Color Absorption: A Technical Exploration.In the realm of color science and technology, the concept of color absorption plays a pivotal role. This process, which involves the interaction of light with matter, determines how we perceive the hues and shades of the visible spectrum. However, a fascinating aspect of color absorption is its variability—the degree to which different materials, surfaces, and environments absorb and reflect light. This article delves into the factors that influence the degree of color absorption and its significance across various applications.### Factors Influencing Color Absorption.1. Material Properties: The physical and chemical properties of a material significantly impact its ability to absorb light. Certain materials, such as dark-coloredfabrics or pigmented plastics, are highly absorbent, while others, like mirrors or certain types of glass, reflect most of the incident light.2. Surface Texture: The roughness or smoothness of a surface also affects color absorption. Rough surfaces scatter light more, reducing the intensity of absorbed colors, while smooth surfaces allow for more uniform absorption.3. Environmental Conditions: External factors like lighting conditions, temperature, and humidity can alter the absorption properties of materials. For instance, changes in lighting intensity or color temperature can shift the perceived hue of a surface.4. Spectral Composition of Light: The specific wavelengths of light incident on a surface determine the colors absorbed. Natural light, for instance, contains a broad spectrum of wavelengths, while artificial light sources may emit a narrower range.### Applications of Color Absorption.1. Printing and Dyeing: In the printing and dyeing industries, understanding color absorption is crucial for achieving consistent color reproduction. Different fabrics absorb dyes differently, necessitating precise adjustmentsin dye concentration and application techniques.2. Photography and Filmmaking: Photographers and filmmakers rely on color absorption principles to capture and manipulate images. The choice of film or digital sensor, as well as post-processing techniques, can significantly affect the final color rendition.3. Paint and Coatings: The paint and coatings industry benefits from a detailed understanding of color absorption. This knowledge helps in developing paints that adhere well, dry uniformly, and maintain color consistency over time.4. Display Technology: In displays such as LCDs and OLEDs, color absorption plays a key role in defining the color gamut and accuracy. The materials used in thesedisplays must have precise absorption characteristics to reproduce a wide range of colors accurately.### Conclusion.The degree of color absorption is a complex phenomenon influenced by various factors, including material properties, surface texture, environmental conditions, and the spectral composition of light. Understanding and controlling these factors is essential for achieving consistent and accurate color reproduction across various applications. As technology continues to evolve, so does our understanding of color absorption, opening up new possibilities for manipulating and experiencing color in unique and captivating ways.。
外国论文
Time and space resolved spectroscopic characterization of a laser carbonplasma plume in argon background.H.M. Ruiz1, F. Guzmán1, V. Munizaga1, M. Favre1, H. Bhuyan1, H. Chuaqui1, E. Wyndham1 1D epartamento de Física, Pontificia Universidad Católica de Chile, Vicuña Mackenna 4860, Santiago, Chile We present time and space resolved spectroscopic observations of a laser produced carbon plasma,in an argon background. An Nd:YAG laser pulse, 370 mJ, 3.5 ns, at 1.06 µm, with a fluence of 1.7J/cm2, is used to produce a plasma from a solid graphite target, in a 0.5 to 250 mTorr argonbackground. The spectral emission in the visible is recorded with 15 ns time resolution. The carbonplasma emission is found to evolve from that characteristic of single ionized carbon, to a morecomplex one, where C2 and C3 molecular bands dominate. The actual time and space features ofthe molecular carbon species evolution are clearly dependent on the argon background pressure.These results are discussed in the context of morphological properties of carbon film deposition,growth from the laser carbon plasma, under different argon background pressure conditions.1. IntroductionThin film deposition using laser produced plasmas has become a well established technique [1]. In particular, carbon and diamond like (DLC) thin film deposition using graphite targets has been investigated, using different parameter regimes [2-4]. Further interest in DLC has been stimulated by biomedical applications [5]. In this context we have investigated carbon film deposition using a graphite target laser plasma in an argon background. Preliminary analysis of the resulting films indicates a correlation between films properties, as inferred from AFM and other standard materials science diagnostics, with the pressure of the argon background. In order to establish a relationship between the carbon plasma and the resulting films properties, we have studied the time and space evolution of the laser produced carbon plasma. Here, we present time and space resolved spectroscopic observations of the laser plasma, as a function of the background argon pressure. These observations allow us to identify carbon film growing conditions where the dominant species in the carbon plasma content are either single atom carbon ions or C2 and C3 molecules.2. Experimental set-upThe experiments were performed in a vacuum chamber at a base pressure of 0.5 mTorr. An Nd:YAG laser pulse, 370 mJ, 3.5 ns, at 1.06 µm, operating at 10 Hz was applied to a rotating graphite target, at approximately 45º to the normal. The focal spot was 0.214 cm2, thus resulting in a fluence of 1.7 J/cm2. Time resolved spectral observations of the carbon plasma plume were performed, at different values of argon admission, in the range from 25 to 250 mTorr. The visible spectra were obtained with a Spectra Pro 275 (1200 g/mm and 140 g/mm) spectrometer, with a gated avalanche array with an aperture of 15 ns. Light emission from the carbon plasma plume was collected with a f-f fiber optic arrangement, focusing at 5, 10, 15 and 20 mm, from the target surface. A negative biased Faraday cup is available to measure the energy spectra of the carbon ions, at different background pressures.2. Experimental resultsFigure 1 shows a time integrated spectrum obtained at 20 mm from the target surface, with 50 mTorr argon background. The spectrum shows emission lines associated with single ionized carbon, and molecular bands, corresponding to vibrational states of the A3Πg→X3Πu transition, swan band, of the neutral C2 molecule. The emission band around 405 nm has been assigned previously to transitions A1Πu→X1Πg, swing band, of the neutral C3 molecule [6,7]. A residual second harmonic laser emission line can also be identified.Figure 2 shows the characteristic temporal evolution of the carbon plasma emission, at 5 mm from the target, with an argon pressure of 25 mTorr.A low spectral resolution was used to record the whole visible emission in a single shot. The spectra are shown with the same arbitrary units intensity scale. At early time, 24 to 56 ns, the spectrum is dominated by emission lines of single ionized carbon. This is even more evident at times closer to the application of the laser pulse, when no molecular emission is observed. At latertimes,emission bands associated with the C 2 molecule, corresponding to the vibrational states identified above, are seen to growth steadily. At 135 ns an emission band from the C 3 molecule becomes noticeable, and increases at later times. A similar characteristic behaviour is observed over theparameter range investigated,Figure 1: time integrated spectrum, at 20 mm form the target, with 50 mTorr argon background. Laser@0.53 µmFigure 2: time evolution of the spectral emission, at 5 mm from the target, with 25 mTorr argon background.Figure 3 shows the characteristic temporal evolution of the carbon plasma emission, at 20 mm from the target, with an argon pressure of 250 mTorr, which corresponds to the extreme conditions in both, pressure and distance from the target that we investigated. In this condition, no significant plasma emission is detected at early times. Carbon ions emission is also not seen.In order to investigate the time and space evolution of the molecular content in the laser plasma plume we used the peak intensity of the C 2 molecular band centred at 467.5 nm as a characteristic feature. This is showed in figure 4, for different distances from the target surface, at 25,100 and 250 mTorr argon background pressure. The arbitrary units intensity scale is the same in all graphs. The figure indicates a clear effect of the argon pressure on the spatial and temporal features of the molecular emission. At a given distance from the target surface, the intensity of the C 2 emission is seen to increase with pressure. On the other hand, the characteristic time duration of the C 2 emission at a given position is not very sensitive to the argon pressure. A double peak structure is clearly observed at 100 mTorr, for distances greater than 5 mm from the target, as pointed out by the arrows in figure 3-b. This feature is also observed at longer distances at 250 mTorr. At an argon base pressure of 0.5 mTorr, no C 2 emission was detected at distancesgreater than 5 mm from the target surface.Figure 3: time evolution of the spectral emission, at 20mm from the target, with 250 mTorr argon background.Figure 3: time evolution of the peak intensity of the C 2 band, centred at 467.5 nm, as a function of the distance from the target surface, for different argon background pressures. a) 25 mTorr, b) 100 mTor, and c) 250 mTorr.Figure 5:intensity of the C2molecule emission, as a function of argon pressure, measured at 20 mm from the target surface.Figure 5 shows the intensity of the C2 emission, as defined above, at 20 mm from the target, as a function of pressure, in a wide pressure range. As seen in the figure, C2emission decays at half the peak value at around 1 Torr of argon background pressure.3. DiscussionPrevious investigations have already reported on the expansion of a laser ablated carbon plasma in an ambient background gas. Experiments using a Nd:YAG laser at high fluence, 2·103 J/cm2, in air at 1-1000 mTorr, identified a double peak structure in the temporal evolution of C+emission at 426.7 nm [8]. Higher ionization states were also identified. In another experiment, with a Nd:YAG, at fluences in the 12.7 to 29.3 J/cm2range, in helium at 100 mTorr, emission from the C2molecule was identified. The time evolution of the C2emission was also found to exhibit a double peak structure [9]. C3molecular emission was identified in experiments using also a Nd:YAG laser, at a fluence of 1.1 J/cm2, in helium and argon, at 200 Torr [6]. In the same experiments, but operating at a high fluence of 280 J/cm2, C3 emission was not detected.The expansion of a laser ablated plasma plume in a gas background presents a different dynamics to that in vacuum. The spherically symmetric model does not describe adequately the plume expansion dynamics. A better agreement with the experimental data is achieved with a model that describes the plume as a thin ellipsoidal shell with total mass corresponding to the amount of accumulated background material resulting from snowploughing of the background gas. This model has been validated at a background pressure of 8 mTorr argon [10]. Ion probe measurements showed the double peak structure, where the first fast peak is mainly attributed to the non-colliding fraction of the laser ablated material and a second slow peak is ascribed to the shock front created by plume–gas interaction. As the background pressure is further increased, a combination of snowploughing, followed by diffusion, should result in slowing down and cooling of the expanding plasma.In order to estimate the initial conditions of the laser produced carbon plasma, we used the analytical model of self-regulating laser ablation [11]to approximate the electron temperature and electron density at a time coinciding with the termination of the laser pulse. Considering that the dominant ionization stage, as inferred from the spectroscopic observation, is Z= 1, and using the experimental values of the different parameters, characteristic values T e~ 4 eV and N e ~ 2·1021 cm-3. As the laser plasma plume expands, the temperature and density decrease. To further estimate the plasma conditions at early stages of the plasma plume expansion, before carbon molecules begin to show in the spectra, we used the PRIMSPECT code [12] to evaluate plasma parameters at a stage when plasma emission is dominated by single charged carbon ions. This is shown in figure 6, where a synthetic spectrum resulting from a PRIMSPECT calculation for a 2.2 eV, 3.5·1017cm-3carbon plasma, results in the best fit to the spectral emission recorded at 5 mm from the target, with a background pressure of 25 mTorr, 56 ns after the laser pulse. The much lower argon background density, of the order of 1014 to 1015 cm-3, is consistent with the fact that no argon emission is detected in our spectralobservations.Figure 6:comparison between a synthetic spectrum generated with the PRIMSPECT code [12] and a measured spectrum at 5 mm from the target, and 25 mTorr argon pressure.Following the temperature estimations at the early stages of the plasma expansion, fast cooling of the expanding carbon plasma is required to achieve conditions where, as shown by our observations, the spectral emission is dominated by neutral carbon molecules. In fact, for C2 and C3 to be the primary components of an equilibrium carbon vapor, the temperatures should in the range of 0.2 to 0.4 eV [13]. The time and space evolution of the carbon plasma emission indicates that the net effect of the argon background is to produce conditions for fast cooling of the carbon plasma, which leads to ion recombination and the establishment of molecular bonds.In parallel to these spectroscopic observations we have exposed silicon substrates to the expanding carbon plasma plume. We have found that the surface morphology of the resulting carbon films, as determined by AFM, depends on the argon background pressure, for otherwise identical experimental conditions, such as substrate position relative to the target, exposure time or substrate temperature. As the pressure increases, in the range from 0.5 to 50 mTorr, the surface roughness was found to growth.Our time and space resolved observations indicate that in pulsed laser deposition of carbon films, in which the experimental conditions are such that the deposition substrate is located further than 5 mm from the target, the dominant species in the expanding carbon plasma are C2 and C3 molecules. Under these conditions it can be speculated that carbon film growth is due mainly to carbon molecules deposition, with a negligible contribution from carbon ions.4. ConclusionsOur results share several features with those reported earlier, but we also report on some new findings, mainly, on the temporal and spatial scales for the plasma plume to cool down, changing form a carbon ions dominated plasma, to one where C2 and C3dominate. Further analysis of our spectroscopic data, combined with ongoing experiments with different background gases, will result in a better description of the physics processes which determine both, the dynamics and plasma chemistry of laser target plasma expanding in an ambient gas. Further contributions are expected on the understanding of the morphological properties of thin films grown under these experimental conditions. 5. AcknowledgementsThis work has been funded by FONDECYT project 1110380. H. R. Ruiz and F. Guzmán acknowledge doctoral studies scholarships from MECESUP and CONICYT, respectively.6. References[1] R. Eason (Ed.), Pulsed laser deposition of thin films, Wiley, New York (2007).[2] D.L. Pappas, K.L Saenger, J. Bruley, W. Krakov, J.C Cuomo, J. Appl. Phys. 71 (1992) 5675.[3] F. Qian, R.K. Singh, S.K. Dutta, P.P. Pronko, Appl. Phys. Lett. 67 (1995) 3120.[4] P.M. Ossi, C.E. Bottani, A. Miotello, Thin Solid Films 482 (2005) 2.[5] R. Kumar Roy, K.-R. Lee, J. Bio. Mat. Res. B: Appl. Biomaterials 83B (2007) 72.[6] L. Nemes, A.M. Keszler,C.G. Parigger, J.O. Hornkohl, H.A. Michelsen, V. Stakhursky, Appl. Optics 46 (2007) 4032.[7] A. Van Orden, R.J. Saykally, Chem. Rev. 98 (1998) 2313.[8] Abhilasha, P.S.R. Prasad, R.K. Thareja, Phys. Rev. E 48 (1993) 2929.[9] S.S. Harilal, Riju C. Issac, C.V. Bindhu, V.P.N. Nampoori, C.P.G. Vallabhana, J. Appl. Phys.80 (1996) 3561.[10] C.V. Budtz-Jørgensen, M.M. Mond, B. Doggett, J.G. Lunney, J. Phys. D: Appl. Phys.38 (2005) 1892.[11] C. R. Phipps, R. W. Dreyfus, Laser Ionization Mass Analysis: Chemical Analysis, edited by A. Vertes, R. Gijbels, and F. Adams, Wiley, New York, (1993), Vol. 124, p. 369.[12] J.J. MacFarlane, I.E. Golovkin, P. Wang, P.R. Woodruff, N.A. Pereira, High Energy Phys. 3 (2007) 181.[13] A. Van Orden, R.J. Saykally, Chem. Rev.98 (1998)2313.。
北京一版帆船邮票印刷色料科技分析
㊀㊀收稿日期:2021-01-05基金项目:北京市属高校高水平教师队伍建设支持计划长城学者培养计划(CIT&TCD20190318);北京印刷学院博士启动基金(27170120003/014)第29卷㊀第5期Vol.29㊀No.5北京印刷学院学报Journal of Beijing Institute of Graphic Communication2021年5月May 2021北京一版帆船邮票印刷色料科技分析曹婉颖,刘铮峰,解明思,周文华,施继龙(北京印刷学院印刷与包装工程学院,北京102600)摘㊀要:利用超景深三维视频显微镜㊁激光显微共聚焦拉曼光谱仪㊁扫描电镜-能谱仪对三枚民国时期北京一版帆船邮票印刷色料进行科技分析㊂结果表明,三枚邮票均为手工雕刻凹版印制,灰棕色邮票油墨中的色料是红丹和炭黑,桔黄色邮票为铬酸铅,草绿色邮票为铬酸铅和普鲁士蓝;纸张和油墨中的填料可能是高岭土㊁碳酸钙㊁氧化锌㊁二氧化硅等㊂研究表明,多技术联用在邮票印刷品分析中有较好的应用㊂关键词:北京一版帆船邮票;印刷色料;科技分析中图分类号:TS801文献标志码:A文章编号:1004-8626(2021)05-0155-04㊀㊀帆船邮票是中华民国建立后发行的第一套普通邮票,在其设计上废弃了清代以龙为王权象征的图腾形象,选择了与生活密切相关的帆船,帆船邮票分为三个版别,每一版还设计有农民的劳作形象以及象征国家对教育重视的圜桥牌坊,该邮票的印制㊁发行在中国邮票史上意义重大,具有较高的历史价值和研究价值㊂对于邮票等印刷材料的无损分析方法,前人已有较多成果:甘清等利用显微观测㊁拉曼光谱分析和电镜能谱分析对一张清代绿色蟠龙邮票样品的印刷材料进行无损分析[1];Chaplin 等利用拉曼光谱仪对夏威夷传教士邮票的原版㊁赝品㊁复制品进行了科技分析,还鉴定了早期邮票上的颜料来区分毛里求斯的原始邮票和伪造的邮票[2-3];Widjaja 等利用拉曼光谱识别商业邮票中的染料[4];Badovi-nac 等采用拉曼光谱仪和X 射线光谱仪分析了匈牙利邮票上的颜料[5];裔传臻对拉曼光谱在纸张老化㊁碳黑颜料以及其他颜料上的应用和研究现状进行了梳理归纳[6]㊂本文拟采用激光显微共聚焦拉曼光谱仪㊁扫描电镜-能谱仪和超景深三维视频显微镜等对三枚北京一版帆船邮票油墨中的色料进行科技分析,所得结果还可为邮票等纸制品的保护修复以及科技鉴定提供科技支撑㊂1㊀实验部分1.1㊀样品及测试区域图1为三枚北京一版帆船邮票样品,分别命名为:样品1㊁样品2和样品3,面值为半分㊁壹分和贰分,图幅尺寸20mm ˑ22mm,票幅尺寸22.5mm ˑ24mm,齿孔度数为14度㊂三枚邮票上均有黑色邮戳,无背胶,颜色分别呈灰棕色㊁桔黄色和草绿色㊂该邮票由北京财政部印刷局承印,由外籍雇员海趣依照伦敦版帆船邮票图案雕刻制版印制,于1914年正式发行㊂图1㊀样品及测试区域㊀㊀㊀其中,1-a㊁2-a㊁3-a 分别为三张样品显微测试区域,1-b㊁2-b㊁3-b 为拉曼光谱仪测试区域,3-a㊁3-b㊁3-c 为扫描电镜-能谱仪测试区域㊂1.2㊀实验仪器及工作条件KEYENCE VHX -600超景深三维视频显微镜:放大倍率:ˑ1000㊂Horiba Jobin Yvon XploRA 激光显微共聚焦拉曼光谱仪:常温;暗室;物镜倍率ˑ50,激光器785nm,过滤器50%,孔径100,缝隙200,光栅刻线600gr㊃mm -1,光斑尺寸1μm,曝光时间30s,光谱扫描范围100~3000cm -1㊂JEOL JSM -6610LA 扫描电镜-能谱仪:二次电子信号(SEI);加速电压20kV;测试距离10mm;放大倍率:ˑ30㊂2㊀结果与讨论2.1㊀视频显微镜分析利用KEYENCE VHX -600超景深三维视频显微镜对样品表面的油墨进行显微形貌观察,如图2,由图可知,三个样品的油墨墨层厚实有堆积感且中间部分比边缘部分厚㊁颜色深,图案边缘较清晰,有明显的凹凸感,符合手工雕刻凹版印刷工艺的特点㊂此外,样品1油墨中混有红色颗粒物,样品3中混有桔黄色颗粒物,初步认为这两枚邮票油墨中的色料至少含有两种呈色物质㊂图2㊀测试区域1-a ㊁2-a ㊁3-a 显微形貌图㊀2.2㊀拉曼光谱分析对三张样品的1-b㊁2-b㊁3-b 区域进行拉曼检测,结果如图3~图5,测试结果与参考文献(见表1)进行比对㊂图3㊀测试区域1-b 拉曼光谱图㊀表1㊀参考文献颜料拉曼特征峰颜料拉曼特征峰/cm -1红丹[7]1201522252803133894595477111085炭黑[8]108313801592铬酸铅[9]146336358374401838普鲁士蓝[10]53020982160㊀㊀通过比对可以发现:1-b 的拉曼特征峰与红丹颜料(Pb 3O 4)以及炭黑颜料(C)的特征峰基本吻图4㊀测试区域2-b 拉曼光谱图㊀图5㊀测试区域3-b 拉曼光谱图651北京印刷学院学报2021年合,结合显微形貌图可以初步推断样品1是由桔红色颜料红丹与灰黑色颜料炭黑共同呈色的㊂2-b 拉曼特征峰铬酸铅颜料(PbCrO 4)的特征峰基本吻合,推断样品2的印刷色料是黄色颜料铬酸铅㊂3-b 的拉曼特征峰与铬酸铅颜料(PbCrO 4)以及普鲁士蓝颜料(Fe 4[Fe(CN)6]3)的特征峰基本吻合,结合显微形貌图可以初步推断样品3是由黄色颜料铬酸铅与蓝色颜料普鲁士蓝共同呈色的㊂2.3㊀扫描电镜-能谱仪Mapping 分析对三个样品进行Mapping 分析,结果如图6~图8所示㊂图6㊀测试区域1-c 能谱Mapping 图㊀图7㊀测试区域2-c 能谱Mapping 图㊀样品1:纸张中含有C㊁O㊁Al㊁Si 元素,油墨中含有C㊁O㊁Al㊁Si㊁Ca㊁Fe㊁Zn㊁Pb 元素,且可以明显地看出 1/2 形状㊂C㊁O 元素在纸张中的含量明显高于油墨;Al 元素在纸张中和油墨中含量几乎相同;Si 元素在油墨中的含量略高于纸张;Ca㊁Fe㊁Zn㊁Pb 元素在油墨中的含量明显高于纸张㊂图8㊀测试区域3-c 能谱Mapping 图㊀样品2:纸张中含有C㊁O㊁Al㊁Si 元素,油墨中含有C㊁O㊁Al㊁Si㊁Cr㊁Zn㊁Pb 元素,且可以明显地看出 分 字形状㊂C㊁O 元素在纸张中的含量明显高于油墨;Al㊁Si 元素在油墨中的含量略高于纸张中;Cr㊁Zn㊁Pb 元素在油墨中的含量明显高于纸张㊂样品3:纸张中含有C㊁O㊁Al㊁Si 元素,油墨中含有C㊁O㊁Al㊁Si㊁Cr㊁Fe㊁Zn㊁Pb 元素,且可以明显地看出 贰 字形状㊂C㊁O 元素在纸张中的含量明显高于油墨;Al㊁Si 元素在纸张中和油墨中含量几乎相同;Cr㊁Fe㊁Zn㊁Pb 元素在颜料中的含量明显高于纸张㊂2.4㊀讨论通过分析可知:三张样品中C㊁O 元素主要来源于纸张纤维中的纤维素(C 6H 10O 5)n ,除C㊁O 外的其他元素来源于造纸时添加的胶料㊁填料等辅助材料和油墨中的填料㊁连接料及各种助剂等㊂结合拉曼光谱分析初步确定样品1油墨中的色料为桔红色颜料红丹(Pb 3O 4)和灰黑色颜料炭黑(C);样品2油墨中的色料为黄色颜料铬酸铅(PbCrO 4);样品3油墨中的色料为黄色颜料铬酸铅(PbCrO 4)和蓝色颜料普鲁士蓝(Fe 4[Fe(CN)6]3)㊂两种实验数据可以相互印证和补充,其余检测出的元素推断为纸张和油墨辅助成分可能是高岭土(Al 2O 3㊃2SiO 2㊃2H 2O)㊁碳酸钙(CaCO 3)㊁氧化锌(ZnO)㊁二氧化硅(SiO 2)等物质㊂在印刷色彩学中,青㊁品红㊁黄为色料三原色,不同颜色的油墨在印刷时遵循色料减色法原理,混合色的明度会相对降低㊂样品1呈现灰棕色是由于桔红色主要吸收蓝光和部分绿光,反射红光和部分绿光,灰黑色的加入会使整个混合色明度降低且发黑,一定量混合后最终形成样品1的灰棕色㊂同理,黄色颜料铬酸铅主要吸收蓝光,反射红光和绿光,蓝色颜料普鲁士蓝主要吸收红光,反射蓝光和751第5期曹婉颖,刘铮峰,解明思,等:北京一版帆船邮票印刷色料科技分析绿光,二者通过一定比例的混合就会形成样品3中的草绿色㊂3㊀结论本次实验运用了视频显微镜㊁拉曼光谱仪和扫描电镜-能谱仪分别对三枚1914年北京一版帆船邮票的印刷油墨进行了无损分析㊂测试结果表明:三枚邮票均为手工雕刻凹版印制,样品1灰棕色油墨中的色料是红丹和炭黑,样品2桔黄色邮票油墨中的色料为铬酸铅,样品3草绿色邮票油墨中的色料为铬酸铅和普鲁士蓝㊂根据检测出的元素推测出纸张和油墨中的填料可能是高岭土㊁碳酸钙㊁氧化锌㊁二氧化硅等㊂通过实验研究,将上述三种技术联用能较好地对邮票进行无损分析,进而为邮票等纸制品的保护修复以及科技鉴定提供科技的支撑㊂参考文献:[1]㊀甘清,季金鑫,姚娜,等.清代绿色蟠龙邮票印刷材料无损分析[J].光谱学与光谱分析,2016,36(9):2823-2826. [2]㊀Chaplin T D,Clark R J,Beech D parison of genuine(1851-1852AD)and forged or reproduction Hawaiian Mission-ary stamps using Raman microscopy[J].Journal of Raman Spec-troscopy,2002,33(6):424-428.[3]㊀Chaplin T D,Jurado‐López A,Clark R J,et al.Identificationby Raman microscopy of pigments on early postage stamps:dis-tinction between original1847and1858-1862,forged and repro-duction postage stamps of Mauritius[J].Journal of Raman Spec-troscopy,2004,35(7):600-604.[4]㊀Widjaja E,Garland e of Raman microscopy and band-tar-get entropy minimization analysis to identify dyes in a commercial stamp.Implications for authentication and counterfeit detection [J].Analytical chemistry,2008,80(3):729-733. [5]㊀Badovinac I J,Orlic'N,Lofrumento C,et al.Spectral analysis ofpostage stamps and banknotes from the region of Rijeka in Croatia [J].Nuclear Instruments and Methods in Physics Research Sec-tion A:Accelerators,Spectrometers,Detectors and Associated Equipment,2010,619(1-3):487-490.[6]㊀裔传臻.拉曼光谱在纸质文物研究中的应用[J].文物保护与考古科学,2018,30(3):135-141.[7]㊀Castro K,Rodríguez-Laso M D,Fernandez L A,et al.Fouriertransform Raman spectroscopic study of pigments present in deco-rative wallpapers of the middle nineteenth century from the Santa Isabel factory(Vitoria,Basque Country,Spain)[J].Journal of Raman Spectroscopy,2002,33(1):17-25.[8]㊀闫海涛,孙凯,唐静,等.明代周懿王墓壁画颜料的科技分析[J].华夏考古,2019(2):39-44.[9]Burgio L,Clark R J.Library of FT-Raman spectra of pigments,minerals,pigment media and varnishes,and supplement to exist-ing library of Raman spectra of pigments with visible excitation [J].Spectrochimica Acta Part A:Molecular and Biomolecular Spectroscopy,2001,57(7):1491-1521.[10]E Imperio,G Giancane.Spectral characterization of postagestamps printing inks by means of Raman spectroscopy[J].Ana-lyst,2015,140(5):1702.(责任编辑:周宇)Scientific and Technological Analyses of Printing Pigmentof Beijing First Edition Sailboat StampsCAO Wanying,LIU Zhengfeng,XIE Siming,ZHOU Wenhua,SHI Jilong(Beijing Institute of Graphic Communication,Beijing102600,China) Abstract:Scientific and technological analysis of the printing pigments of three Beijing first edition sailboat stamps during the Republic of China period.These methods include ultra-depth of field three-dimensional video microscope,Raman spectrometer and scanning electron microscope-energy diapersive spectrometer.Results show that all three stamps were printed by hand-engraved intaglio. The coloring substance of the greenish-brown stamp is composed of red lead and carbon black.The orange stamp is lead chromate,and the grass green stamp are lead chromate and Prussian blue.Then, based on the detected elements,it is inferred that the auxiliary components of paper and ink may be kaolin,calcium carbonate,barium sulfate,silicon dioxide and so on.According to the theory of color subtractive method in printing chromatics,the coloring principle of greenish-brown and grass green ink is analyzed.This study have shown that multi-technology has a good application in the analysis of stamp prints.Key words:Beijing first edition sailboat stamp;printing pigment;analysis of science and technology 851北京印刷学院学报2021年。
声全息简介LMS
TheoryCategory: Acoustics and sound qualityTopic: Acoustic holographyIntroductionAcoustic holography allows you to accurately localize noise sources. It therefore helps in both the reduction of unwanted vibro-acoustic noise and optimization of noise levels. It :• estimates the acoustic power and the spectral content emitted by the object under examination.• maps sound pressure, velocity and intensity on the measurement plane and on all parallel planes. The mapping of these acoustical quantities outside the measurement plane is donethrough acoustical holography (near field - far field).• estimates the acoustic level of the principal sources, including contribution analysis.This document describes the principles of taking acoustic measurements and the subsequent analysis of acoustic holography data, for both stationary and transient measurements.Basic principlesIn performing acoustic holography, you need to measure cross spectra between a set of reference transducers and the hologram microphones. From these measurements you can derive sound intensity, particle velocity and sound power values.A basic assumption is that you are operating in free field conditions and that the energy flow is coming directly from the source. Measurements need to be taken close to the source.It provides you with an accurate 3D characterization of the sound field and the source with a higher spatial resolution than is possible with conventional intensity measurements.Acoustic holography conceptsThe principle of acoustic holography is to decompose the measured pressure field in plane waves, by using a spatial Fourier transform. With the frequency being fixed, we can calculate how each of these plane waves propagates, and by adding them we can find the pressure field on any plane which is parallel to the measurement plane.Consider an acoustic wave. Measuring the pressure on a plane means cutting the wavefronts by the measurement plane :LMS proprietary information: reproduction or distributionof this document requires permission in writing from LMSAcoustic holography.docThe goal is to determine the whole acoustic wavefront from the known pressure on the measurement plane. Each microphone in the array measures the complex pressure (amplitude and phase). Temporal and spatial frequencyIn considering how to do this we will compare the time and the spatial domain.Time domainWhen considering measurements in the time domain, then the position from the sound source (m) is fixed and we obtain a measure of the pressure variation as a function of time.The transformation from the time to the frequency domain is achieved using the Fourier Transform given belowSpatial domainIf we now consider measurements where time is fixed and pressure varies as a function of distance, we can obtain a measure of energy flow.The spatial frequency of this function or wavenumber (k0) is defined as :If we fix the temporal frequency, this means that the acoustic wavelength is fixed too.The complex pressure as a function of the space is called the pressure image at the specified frequency.Conversion from the spatial domain is also done using a Fourier transform. In Acoustic holography pressure is measured in two dimensions (x and y for example), so a 2-dimensional transformation is performed.where S (k x , k y) is the spatial transform of the measured pressure field to the wavenumber (k x and k y) domain resulting in the 2-D hologram pressure field.A measured pressure (sound) wave with a particular temporal frequency can propagate in a number of directions, so the wavenumber vector (k) will have a number of components. The appearance of these vectors depends on the plane on which you are looking at them. The aim is to find the components of these vectors in the 2 dimensions that define the plane and to do this projections of the vectors in the plane are made.Summation of plane wavesThe spatial Fourier transform implies that a measured pressure field can be considered as a sum of sinusoidal functions.Each of these sinusoidal functions can be understood as the result of cutting the wavefronts of a plane wave by the measurement plane.There is a coincidence between the nodes of the sinusoidal function and the wavefronts. In effect,decomposing the pressure field into a sum of sinusoidal functions means decomposing the real acoustic wave into a sum of plane waves.Whatever the angle of incidence, the spatial periodicity must be greater than the wavelength (l). Propagating and evanescent wavesThere are two kinds of plane waves :To understand why we must take evanescent plane waves into account, let us consider our decomposition of the pressure field into sinusoidal functions. If the spatial periodicity of a sinusoidal function is shorter than the wavelength, it cannot be the result of cutting a propagating plane wave by the measurement plane :Whatever the direction of the propagating plane wave may be, there is no possible coincidence between the nodes of the sinusoidal function and the wavefronts. Therefore, this sinusoidal function must be understood as the intersection between an evanescent wave (which can have a smaller spatial periodicity than propagating waves) and the measurement plane.A mathematical interpretation of the evanescent waves is based on the value of k z which is the component perpendicular to the measurement directions in the wave number domain.k z can be determined from the wave number k0 and the known values of k x and k y from the transformation.k z is real when (the spatial periodicity is greater than the wavelength). This means that the waves lie in the circle defined by the radius w/c in the wave number domain. k z is imaginary outside of this region.When k z is imaginary, the propagation factor becomes a damped exponential function (e-jk z z) meaning that a propagated wave undergoes an amplitude modification while the phase is not changed. (Back) propagating to other planesPressure levels at other planes can be found using Raleigh’s integral Equation with Dirichlet’s Green function :where the Green function G d can be thought of as the transformation function to transform the sound pressure field from one plane to another.We can use wave domain properties (k) to predict the pressure at a different spatial position (z). The practical computation of Raleigh’s equation iswhere z’ is the measurement plane and z is the position of the required plane. The green function is given byand k z can be found from equation 6-3.The final step is to perform an inverse transformation back to the temporal domain.The Wiener filter and the AdHoc windowAs mentioned above, evanescent waves undergo a change in amplitude when propagating. Propagating towards the source implies an amplification of the signal that is a function of k.z, therefore their amplitude is Evanescent waves that lie far away from the unit circle have a large kzamplified significantly when propagating to the source. The contribution of these evanescent waves results in an increase of spatial resolution. Note that the inclusion of evanescent waves is only appropriate when propagating towards the source.Propagating away from the source, the evanescent waves decrease so rapidly in amplitude that their contribution to the spatial resolution becomes negligible. However the further away a wave is located from the circle, the less accurate the amplitude estimate becomes so that at a certain point noise is propagated and at that point the propagated image starts to blur.When propagating towards the source, a Wiener filter can be used to include a certain number of evanescent waves to improve the resolution. Taking a higher number of waves taken into account may result in the amplification becoming unstable. This depends on a parameter of the Wiener filter known as the Signal to Noise Ratio (SNR). When the SNR value is greater than 15dB, then the amplification will become unstable as the number of evanescent waves included increases. Using an low SNR value (5dB for example) means that the evanescent waves are taken into account but they are so attenuated that the improvement in resolution is negligible. The default value of 15dB provides the best compromise in terms of resolution and amplification.When the Wiener filter is used, the pressure image needs to be multiplied by a two-dimensional window. As is the case with a single FFT, the observed pressure must be ‘periodic’ within the observed hologram. If this is not the case, then truncation errors occur as with a single FFT. These truncation errors manifest themselves as ghost sources at the borders of the observed area.Two windows are usedThe rectangular window,which does not modify the pressure image. In case of a rectangular window, only propagating waves are included in the calculations resulting in a resolution equivalent to an intensity measurement.The so-called Ad Hoc windowFor a time signal, the FFT algorithm takes the time signal and duplicates it from minus to plus infinity. If the amplitude of the measured time signal differs between the start and the end of the window, a discontinuity occurs during this multiplication introducing an error in the FFT algorithm. This can be corrected using a Hanning window. Holography used a double FFT so the AdHoc window is used, which is basically a two dimensional Hanning window thus removing discontinuities in the both the x and y directions.The one-dimension Ad Hoc window (W) would be:Derivation of other acoustic quantitiesIf we know how the plane waves propagate, we can calculate the pressure field in any parallel plane, by adding the contributions of all plane waves. This will be correct only if all acoustic sources are on the same side of both planes :Knowing the pressure field on the parallel plane, it is possible to calculate the particle velocity and eventually the intensity on this plane.The particle velocity (V) will be known if the pressure differential can be determined -which is the case with Acoustic holography since the pressure can be measured at r and (r + dr)Once the pressure and the velocity are known then the intensity is just the product of the two.。
惠威DIAMOND 200 S E R I E S说明书
"…quite simply they are one of the best budget speakers around."What Hi-Fi review, October 2014Diamond 220Best Stereo Speakers up to £200HeritageBritain has long been recognised as being the home of loudspeaker technology in terms of innovation and quality. Gilbert Briggs’ first loudspeaker was manufactured in 1932 through a passion for music and an ear for detail – in a sleepy little market town of Yorkshire Wharfedale was born. After winning multiple awards, his work is still much admired and respected throughout the hi-fi world today and our speakers are still driven by the same passion for music. Wharfedale’s Diamond series has a long history of achievement. The first Diamond was born in 1982 in the form of a rear ported hi-fi speaker. A combination of a 19mm dome tweeter, 120mm long throw polypropylene bass/mid driver and a simple yet highly effective crossover in a compact hi-fi speaker took the industry by storm. The speaker produced an impeccable stereo image, quickly becoming a best seller and a permanent fixture in the Wharfedale product range. Since then, every Wharfedale Diamond Series has been a best-seller.From 1982 Wharfedale Diamond has meant one thing – impeccable performance at an affordable price. Today we are pleased to bring you the latest series of loudspeakers from Wharfedale that aspires to this tradition – Diamond 200.Diamond Re-EngineeredThe Diamond 200 boasts the latest in hi-fi technology to produce a thoroughly enjoyable listening experience. Foremost in the design criteria for Diamond 200 is the ongoing research into loudspeaker driver sound quality. The Diamond Series utilises our famous woven Kevlar® cone drawing influence from the flagship Jade Series. Semi-elliptical ‘break-up’ areas on the Kevlar® woofer smooth the response through the audible range and the cone edges are treated with a unique diamond moulding.For Diamond 200 series Wharfedale’s engineers have refined and updated this design and drive unit motor systems have been red efined with more power with greater efficiency. Larger magnets for instance on the Diamond 220 create a greater sensitivity compared with previous loudspeakers.The treble unit uses a sheer fabric dome and advanced ferrite magnet system, surrounded by a carefully crafted wave guide that encourages outstanding midrange performance too.Improved Cabinet ConstructionCabinet materials have taken a leaf out of the extensive research that resulted in the advanced Jade series. Even the appearance is improved with new, lacquered front baffles and cosmetically enhanced veneers.Cabinet walls and internal bracing developed using Wharfedale’s latest ‘Virtual Speaker ’ software, with the help of Delayed Cumulative Spectral Analysis that ruthlessly reveals panel coloration in all its forms. Using this technique Wharfedale engineers updated the cabinet combining layers of particle board and MDF bonded in a unique structure to damp annoying High-Q resonances and block internal sound leakage. The effect is that the ‘noise’ from cabinet walls is buried more than 35dB below the driver output. The same computer modeling also assists in fine tuning the crossover while ensuring the speaker projects both on and off-axis for an enjoyable, room-filling experience.Hundreds of hours of listening tests have resulted in refinements to the crossoversystems to yield greater attack, dynamics and musical enjoyment in conjunctionwith the neutrality and startling realism that is a Wharfedale tradition. Althoughcomputer modeling is a valuable tool in modern loudspeaker production, it isa combination of our engineers experience and passion for music that results insuch an enjoyable loudspeaker.In the final evaluation weeks are spent fine tuning the acoustic performanceusing a wide variety of music in Wharfedale’s five listening rooms, each ofwhich mimics the kind of domestic environments the Diamond Series are likelyto be used in. Only when the acoustic tests are deemed truly satisfying are theloudspeaker designs signed-off for production, ensuring that each speakermodel fulfils its eventual owner’s dreams of musically enjoyable reproductionfrom Britain’s Most Famous Loudspeakers.Tuned For Your Living RoomSPECIFICATIONS:General description2-way bookshelf speaker 2-way bookshelf speaker 2.5-w ay floorstanding speaker Enclosure typebass reflex bass reflex bass reflex Transducer complement2-way 2-way 2.5-way Bass driver100mm Woven Kevlar® Cone 130mm Woven Kevlar® Cone 165mm Woven Kevlar® Cone Midrange dri ver165mm Woven Kevlar® Cone Treble driverAV shieldNo No No Sensitivity(2.83V @ 1m)86dB 86dB 88dB Recommended amplifier po wer15-75W 25-100W 25-150W Peak SPL90dB 95dB 102dB Nominal impedance8Ω Compatible 8Ω Compatible 8Ω Compatible Minimum impedance4.1Ω 4.1Ω 3.7ΩFrequency response (+/-3dB)68Hz - 20kHz 56Hz - 20kHz 40Hz - 20kHz Bass extension (-6dB)58Hz 45Hz 37Hz Crossover frequency2.3kHz 2.2kHz 2.3kHz Cabinet Volume (in litres)3.2L 7L 35L Dimensions (mm)Height (on plinth & spikes)232mm 315mm (938+25)mm Width143mm 174mm 196mm Depth (with terminals)(165+5)mm (227+28)mm (306+28)mm Carton size415x260x330mm 495x320x410mm 420x310x1060mm Net w eight2.6kg/pcs 5.3kg/pcs 17.8kg/pcs Gross w eight6.5kg/ctn 12.6kg/ctn 21.2kg/ctn FinishRosewood /Walnut Pearl/White sandex/Black wood Vinyl Rosewood /Walnut Pearl/White sandex/Black wood Vinyl Rosewood /Walnut Pearl/White sandex/Black wood Vinyl Standard accessoriesspike/spike seatOptional accessories BlackWhiteWalnut Rosewood3-w ay floorstanding speaker3-w ay floorstanding speaker2-w ay centre speakerbass reflex bass reflex bass reflex3-way3-way2-way165mm W o v en Kevlar® Cone x 2200mm W o v en Kevlar® Cone x 2130mm W o v en Kevlar® Cone x 2 130mm W o v en Kevlar® Cone130mm W o v en Kevlar® ConeNo No Y es89dB89dB89dB25-150W25-200W25-150W102dB110dB95dB4Ω6Ω 8Ω Compatible3.0Ω 3.1Ω4Ω40Hz - 20kHz35Hz - 20kHz60Hz - 20kHz35Hz32Hz65Hz470Hz & 2.7kHz350Hz & 2.5kHz 2.3kHzMid internal 10.6L Mid internal 8L11.8LBass internal 37.2L Bass internal 66.3L(998+25)mm(1103+25)mm(174+16)mm204mm250mm470mm(366+28)mm(396+28)mm(236+28)mm480x320x1120mm510x365x1225mm560x3320x280mm21.6kg/pcs29.4kg/pcs8.5kg/pcs25.2kg/ctn34.5kg/ctn10kg/ctnRose w ood /W alnut P earl/White sandex/ Black w ood V inyl Rose w ood /W alnut P earl/White sandex/Black w ood V inylRose w ood /W alnut P earl/White sandex/Black w ood V inylspike/spike seat spike/spike seat rubber feetcentre base©CODE: WH14-BR0001IAG House, 13/14 Glebe Road, Huntingdon, Cambridgeshire, PE29 7DL, UKTel: +44(0)1480 452561 Fax: +44(0)1480 413403 。
颜色与波长的关系(Therela...
颜色与波长的关系(The relationship between color andwavelength)For the convenience of studying the color properties of light, the visible spectrum is surrounded by a circle and divided into nine regions (see Fig.), called the color ring. Digital color ring said corresponding light wavelength, unit (nm), nano color ring two on top of any sector in color, are called complementary. For example, blue (435 ~ 480nm) complementary yellow (580 ~ 595nm). It is found that light colors also have the following characteristics: (L) complementary colors are mixed in a certain proportion to obtain white light. White light, such as blue light and yellow light, is white. Similarly, blue and orange light is obtained by mixing white light; (2) any kind of color ring can be used two kinds of monochromatic light on both sides of the adjacent, even from two kinds of monochromatic light mixed subneighbouring reproduced. Orange light is mixed with yellow light and red light. Typically, red light and green light are mixed into yellow light; (3) if you choose three separate monochromatic lights on the color ring. It can be blended into different shades of everyday life in different proportions. These three kinds of monochromatic light is called primary colors. The primary colors in the optics are red, green and blue. It should be noted that the primary colors of the pigments are red, yellow and blue. However, the choice of colors is quite arbitrary; (4) when the sun light irradiation of an object, a wavelength of light by the object from the object, the display color (reflected light) for the light color. If the sun is shining on the object, if the object absorbs the violet light with a wavelength of 400 ~ 435ntn, the object appears yellow green. It should be noted that some people say that theobject's color is that the object absorbs other colors and reflects the light of this color. It's wrong to say that. For example, yellow green leaves actually absorb only violet light of 400 to 435urn, showing that yellow green is the reflection of other colors, rather than reflecting yellow green light.The laser frequency range of 3.846*10^ to 7.895*10^ (14) Hz (14) Hz. electromagnetic spectrum can be divided into: (1) - radio wavelengths from thousands of meters to 0.3 meters, general TV and radio band is in this wave; (2) microwave wavelength from 0.3 meters to 10^ meters -3, these wave used in radar or other communication system; (3) - infrared wavelengths from 10^-3 * 10^-7 meters to 7.8 meters; (4) visible light. This is a very narrow band of people can be sensitive. The wavelength ranges from 780 to 380nm. Light is the electromagnetic wave produced by the change of the motion of electrons in atoms or molecules. Because it is the very little part of the electromagnetic wave that we can feel directly; (5) ultraviolet rays - wavelengths from 3 x 10^-7 meters to 6 x 10^-10 meters. The causes of these waves are similar to those of light waves, often emitted during discharge. Because its energy is similar to the energy involved in general chemical reactions, the chemical effects of ultraviolet light are strongest; (6) roentgen rays - this part of the electromagnetic spectrum, wavelengths from 2 x 10^-9 meters to 6 x 10^-12 m..Visible light (English visible light) is a human electromagnetic spectrum can be perceived, no accurate visible spectral range; electromagnetic waves generally people's eyes can perceive the wavelength between 400 to 700 nm, but there are some people can perceive the wavelength around theelectromagnetic wave between 380 to 780 nm. The human eye with normal vision is most sensitive to electromagnetic waves with a wavelength of about 555 nanometers, which is in the green region of the optical spectrum (see item: luminosity function).Visible light sourceThe main natural light source of visible light is the sun, and the main artificial light source is incandescent objects (especially incandescent lamps). The visible spectrum emitted by them is continuous. The gas discharge tube also emits visible light, and the spectrum is discrete. Various gas discharge tubes and filters are used as monochromatic light sources.The range of light visible to the human eye is affected by the atmosphere. The atmosphere is opaque to most of the electromagnetic radiation, only visible light bands and other exceptions, such as radio bands. Many other creatures can see light waves that are different from human beings,For example, some insects, including bees, can see the ultraviolet band, which is very helpful for finding nectar.The spectrum does not contain all the colors that the human eye and the brain can recognize, such as brown, pink, and purplish red, because they need to be mixed with a variety of light waves to adjust the red shade.The wavelength of visible light can penetrate the optical window, which can penetrate the earth's atmosphere and attenuation of electromagnetic wave range is not much (bluelight scattering is red is serious, which is why we see the sky is blue). The human eye's response to visible light is a subjective definition (see CIE), but the window of the atmosphere is defined in terms of physical measurements. It's called the visible light window because it just covers the visible spectrum of the human eye. The near infrared (NIR) window is just outside the visible range of the human eye, while the mid wavelength infrared (WMIR) and far infrared (LWIR, FIR) are far away from the visible section of the human eye. As a result, the appearance of various plants under ultraviolet light has more influence on the attraction and reproduction of insects than the color in our eyes.Explanation of visible spectrumThe early 2 explanations of spectra came from Isaac Newton's optics and the color of Johann Wolfgang von Goethe. Newton first used the word "spectrum" in Latin for his optical experiments in 1671 (in Latin for appearance and imaging). Newton observed a beam of sunlight entering the glass prism at an angle, partially reflecting, and partly through the glass and showing a different ribbon. Newton assumes that the sun is made up of small particles of different colors, and that these colors move differently across the material. The red light is faster than the violet light, resulting in the deflection of the red light after the prism passing, which is smaller than that of the violet light, resulting in various spectra.Newton divides the spectrum into 7 colors: red, orange, yellow, green, blue, indigo, purple (the order in children's nursery rhymes), so that you can remember it. He ancient Greekphilosopher thought, selected the 7 colors, and notes, and links the days of the solar system planets, and for a week. As a result, some experts, such as Isaac Asimov (Isaac Asimov), have suggested that indigo should not be considered as a color. It is just a blue and purple shade of different shades. Goethe claims that continuous spectrum is a composite phenomenon. And Newton believes that only the visible spectrum is a separate phenomenon, Goethe observed a much broader part, he found that no interval of the spectrum, such as red yellow and blue border boundary is white, originally in the boundary region there will be light overlapping. So far the popular acceptance of light is composed of photons from (some light has wave characteristics, other time is particle characteristics, see wave particle characteristics, light is all double) speed of light in a vacuum, and the speed of light in the other material, compared with the speed of light in vacuum is low. This ratio is the refractive index of the substance. In some known substances (non dispersive material) light speed has no difference in different frequencies, but other substances in light of different frequencies have different speed: glass belongs to this material, so the glass prism of white light. The rainbow of nature is an ideal example of the spectrum seen by refraction.Green 495 – 570 nmYellow 570 – 590 nmOrange 590 – 620 nmRed 620 – 750 nmThe rainbow spectrum, as we know it, includes all the visible light of a single wavelength, that is, pure monochromatic light. Although there is no distinct boundary between adjacent colors, the range of wavelengths mentioned above is a commonly used approximation.spectroscopyThe science of studying the radiation spectrum of objects is called spectroscopy. One of its important applications is astronomy, because spectroscopy is the basis for analyzing the nature of distant objects. Common astronomical spectroscopy applied to spectral analysis of high refractive index and extremely high resolution. For example, helium is the first element found in the solar spectrum; the chemical elements in the planet can be read by their emission spectrum or absorption spectrum;。
GE Entropy
EntropyWhat is EntropyThe GE Entropy™ Module is indicated for adult and pediatric patients older than 2 years within a hospital for monitoring the state of the brain by data acquisition of electroencephalograph (EEG) and frontal electromyograph (FEMG) signals. The spectral entropies, Response Entropy (RE) and State Entropy (SE), are processed EEG and FEMG variables.In adult patients, Response Entropy (RE) and State Entropy (SE) may be used as an aid in monitoring the effects of certain anesthetic agents, which may help the user to titrate anesthetic drugs according to the individual needs of adult patients. Furthermore in adults, the use of Entropy parameters may be associated with a reduction of anesthetic use and faster emergence from anesthesia.1,2,3 The Entropy measurement is to be used as an adjunct to other physiological parameters.How is Entropy calculatedEntropy is a measure of irregularity in any signal. During general anesthesia, EEG changes from irregular to more regular patterns when anesthesia deepens. Similarly, FEMG quiets down as the deeper parts of the brain are increasingly saturated with anesthetics. The Entropy Module measures these changes by quantifying the irregularity of EEG and FEMG signals.4In adults, the Entropy Range Guideline reflects a general association between the patient’s clinical status and Entropy values. The Guideline is based on an Entropy validation study 5 involving administration of specific anesthetic agents. Titration of anesthetics to Entropy Guideline should be done in context of patient status and treatment plan. Individual patients may show different values.GE HealthcareQuick GuideGetting startedMonitoring the electrical activity of the brain and facial muscles with the Entropy Module is easy, just attach the Entropy sensor on the patient’s forehead according to the instructions provided on the sensor pouch. The module automatically checks that the electrode impedances are within an acceptable range and starts the measurement. The measurement will continue until thesensor is removed.Figure 1: Entropy set-upIn adults, Entropy values have been shown to correlate to the patient’s anesthetic state. High values of Entropy indicate high irregularity of the signal, signifying that the patient is awake. A more regular signal produces low Entropy values which can be associated with low probability of consciousness.Entropy Range GuidelinesRE is a fast reacting parameter, which may be used to detect the activation of facial musclesSE is a more stable parameter, which may be used to assess the hypnotic effect of anesthetic drugs on the brainIndividual patients may show different values. 6** F requent eye movements, coughing and patient movement cause artifacts and may interfere with the measurement. Entropy readings may be inconsistent when monitoringpatients with neurological disorders, traumas or their sequelae. Epileptic seizures and psychoactive medication may cause inconsistent Entropy readings.The Entropy parametersThere are two Entropy parameters: the fast-reacting Response Entropy (RE) and the more steady and robust State Entropy (SE). State Entropy consists of the entropy of the EEG signal calculated up to 32 Hz. Response Entropy includes additional high frequencies up to 47 Hz. Consequently the fast frontalisEMG (FEMG) signals enable a fast response time for RE.Table 1: Frequency and display ranges for Entropy parameters.Response Entropy (display range 0-100)Response Entropy is sensitive to the activation of facial muscles, (i.e., FEMG). Its response time is very fast; less than 2 seconds. FEMG is especially active during the awake state but may also activate during surgery. Facial muscles may also give an early indication of emergence, and this can be seen as a quick rise in RE.State Entropy (display range 0 - 91)The State Entropy value is always less than or equal to Response Entropy. During general anesthesia the hypnotic effect of certain anesthetic drugs on the brain may be estimated by State Entropy value. SE is less affected by sudden reactions to the facial muscles because it is mostly based on the EEG signal.Neuromuscular blocking agents (NMBA), administered insurgically appropriate doses are not known to affect the EEG, butare known to have an effect on the EMG.Figure 2: Entropy shown in the waveform fieldWhy use Entropy monitoringUse Entropy to titrate anesthetic drugs according to the individual needs of the patientEntropy measures the activity of the brain, which is the target organ for anesthetic medication, and has been shown to reflect the different phases of anesthesia. Furthermore, the use of Entropy has been found to reduce the use of certain hypnotic drugs. Therefore, Entropy may help you tailor the administration of anesthetic drugs for each patient individually.Use Entropy to control recovery and to improve your perioperative processWith Entropy monitoring, it is possible to ensure faster emergence and recovery in the operating room. It is a tool for optimizing the perioperative process and ensuring efficient patient flow.Integrated informationWhen Entropy monitoring is integrated into a monitoring system, the measured values are displayed, trended, and automatically documented together with all of the other monitored parameters.Adequacy of AnesthesiaUnconsciousness, amnesia, antinociception and at least some degree o f i mmobility c ombined w ith a utonomic s tability a re v arious targets, when tailoring anesthesia for each patient. Therefore, it takes more than one measurement to reliably assess theadequacy of anesthesia. With Entropy used together with other monitored parameters, such as the hemodynamic measurements and NMT, you can get a complete picture of the patient status combined on one screen. All these values are stored in the monitor memory for trending and information management purposes.At GE Healthcare, our vision is to provide you with the complete range of clinical parameters to help you give personalized anesthesia for each patient.Subcortical ComponentsCorticalComponentsAntinociceptionImmobilityAutonomicStabilityUnconsciousnessAmnesiaClinical use of Entropy1.A fter the sensor is attached, the monitor will start the measurement by checking the sensor integrity and impedance level acceptability.2. D uring awake state and induction there is adifference between the two Entropies indicating muscle activity on the face.3. D ecrease in the Entropy measurement may enable the physician to observe the moment when patient loses responsiveness.4. B oth Entropies stabilize during the operation. Sudden peaks in RE during surgery are primarily caused by activation of FEMG.5. B urst Suppression Ratio (BSR) can be selected on the screen to indicate the amount of silent periods in the raw EEG.6. A t the end of the case, rise in both Entropies is seen.Additional resourcesFor white papers, guides and other instructive materials aboutour clinical measurements, technologies and applications, pleasevisit /References1. Vakkuri et al. Spectral entropy monitoring is associated withreduced propofol use and faster emergence in propofol -nitrous oxide - alfentanil anesthesia. Anesthesiology103,274-9 (2005).2. Aimé, I., et al. Does monitoring bispectral index or spectralentropy reduce sevoflurane use? Anesthesia and Analgesia,103(6), 1469–1477 (2006).3. El Hor, T., et al. Impact of entropy monitoring on volatileanesthetic uptake. Anesthesiology, 118(4), 868–873 (2013).4. Viertiö-Oja et al. Description of the Entropy algorithm asapplied in the Datex-Ohmeda S/5 Entropy Module. ActaAnaesthesiologica Scandinavica48, Issue 2: 154-161 (2004).5. Vakkuri et al. Time-frequency balanced spectral entropy as ameasure of anesthetic drug effect in central nervous systemduring sevoflurane, propofol, and thiopental anesthesia. ActaAnaesthesiologica Scandinavica48, Issue 2: 145-153 (2004).6. Klockars et al. Spectral entropy as a measure of hypnosis inchildren. Anesthesiology104, 708-17 (2006).Imagination at workProduct may not be available in all countries and regions. Full product technical specification is available upon request. Contact a GE Healthcare Representative for more information. Please visit /promotional-locations.Data subject to change.© 2010 - 2016 General Electric Company.GE, the GE Monogram, Imagination at work and Entropy are trademarks of General Electric Company. All other third-party trademarks are the property of their respective owners.Reproduction in any form is forbidden without prior written permission from GE. Nothing in this material should be used to diagnose or treat any disease or condition. Readers must consult a healthcare professional.JB44337XX 11/16。
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Spectral Reproduction from Scene to Hardcopy II: Image ProcessingMitchell Rosen, Francisco Imai, Xiao-Yun (Willie) Jiang, Noboru Ohta Munsell Color Science Laboratory, RITABSTRACTTraditional image processing techniques used for 3- and 4- band images are not suited to the many-band character of spectral images. A sparse multi-dimensional lookup table with inter-node interpolation is a typical image processing technique used for applying either a known model or an empirically derived mapping to an image. Such an approach for spectral images becomes problematic because input dimensionality of lookup tables is proportional to the number of source image bands and the size of lookup tables is exponentially related to the number of input dimensions. While an RGB or CMY source image would require a 3-dimensional lookup table, a 31-band spectral image would need a 31-dimensional lookup table. A 31dimensional lookup table would be absurdly large. A novel approach to spectral image processing is explored. This approach combines a low-cost spectral analysis followed by application of one from a set of low-dimensional lookup tables. The method is computationally feasible and does not make excessive demands on disk space or run-time memory.1. BACKGROUNDAlthough many research centers around the world are looking at various aspects of the spectral imaging workflow,1-5 there are very few publications concerned with spectral hardcopy output. There are notable exceptions to this observation including several papers from the Munsell Color Science Laboratory.6-8 Spectral hardcopy remains an elusive holdout for several reasons: 1) it is not necessarily obvious how one would utilize typical spectrally broad printing inks for spectral output and, even if one could use these inks, natural intuition leads to the assumption that a plethora of inks would be needed to make a reasonable spectral match to an arbitrary input spectrum; 2) very few spectral models exist for hardcopy devices describing the relationship between requested output digit and the delivered spectrum; and, 3) even in the case where a model is given, if it is assumed that the model is computationally complex, then the problem remains as to how to apply the inverse of the model to a large spectral image within a reasonable time. These first two concerns have already been addressed in previous publications. It has been shown that for certain images, four process inks plus two or three readily available inks can be used to produce highly spectrally accurate output6. Even for cases where best obtainable spectral accuracy is still low, reduction of metamerism is a worthy goal for many applications. Spectral models do exist for certain printing technologies9 and have been utilized in the above referenced studies6,7. Application of the inverse of a model to a complex and large spectral image is where the effort for this study was applied. In any color reproduction system, there are generally three major components. There is the image capture or synthesis stage, then the image processing stage and finally an image output stage, sometimes referred to as image display or image rendering. Traditionally, color capture devices have been engineered to take into account the spectral integration which is an important aspect of human color perception. Thus, typical color capture devices have three channels each having spectrally wide sensitivity, much like the human. For image output, a computer monitor is similar to the typical image capture device in that it relies on three spectrally wide channels. Typical printers have four channels where a black is added to a set of three spectrally wide subtractive primaries. The black is primarily used to increase the color gamut for dark colors. A standard image processing regime is designed to manipulate the three incoming channels in anticipation of how the output stage renders colors. For accurate color reproduction, the image processing stage must be aware of the characteristics of both the image capture device and the image rendering device. Figure 1a describes a general color reproduction system. The International Color Consortium (ICC) defines the industry standard method for informing color processing about the stimulus and response character of the two ends of the color reproduction chain. The input device ICC profile describes the relationship between input digit and colorimetry under the D50 illuminant. Colorimetry, based on the human color matching functions, is a three-dimensional space. For most color capture devices the mapping between its three channels and the three dimensions of colorimetry is overall one-to-one. Where the actual mapping is many-to-one or one-to-many, this is due to differences between the instrumental metamerism of the input device and the metameric characteristics of the “standard observer.” The ICC profile for the output device describes the relationship between D50 colorimetry and output digit. For most printing devices, there is much redundancy between colorimetry and output digits. This is due to the presence of the fourth colorant. Makers of ICC profiles must deal with these mapping issues and provide color processing with singlemappings in each instance. In a typical ICC compliant image processing stage of a color reproduction system, a pair of profiles will be used, one referring to the image capture device and the other referring to the image rendering device, as shown in Figure 1b. Optimizations will take place to ensure that the image processing proceeds in as efficient a manner as possible since it is typical that each pixel in a captured image would undergo some level of manipulation. The fact that each ICC profile is tied to the common space of colorimetry makes the concatenation of a series of transforms described in the profiles a fairly straight forward and computationally efficient matter. Figure 1c shows a typical ICC image processing block diagram which includes concatenation. After applying these efficiencies to the transformation parameters, it is likely that at its most complex, the image processing stage would consist of applying in parallel to each input channel a one-dimensional lookup followed by a three-dimensional lookup and possibly a final one-dimensional lookup applied to each output channel. Computationally and with respect to memory requirements the image processing chain described here is very feasible and highly efficient.Input Device CharacterizedInput Image Captured by Input Deviceinput imageinput profileinput imageinput profile input imageinput profileTransform from device digit to Colorimetrycolorimetric imageImage Processedoutput profileCreate New Transform Representing Concatenation of Input and Output Transformsdigit->digit transformTransform from Device Digit to Device Digitmodified imageoutput profileTransform from Colorimetry to device digitoutput profilemodified imageOutput Device CharacterizedOutput Image Rendered by Output Devicemodified imageFigure 1a: General color reproduction block diagram.Figure 1b: Logical ICC image processing block diagram.Figure 1c: Typical ICC image processing with efficiencies. Transform box may include 1-D and 3-D lookups and matricies.When the input and output devices in a color reproduction system possess a sufficient number of channels, spectral characterizations rather than colorimetric ones are possible. The image processing stage for such a system would necessarily be more complex than the ICC approach described above. In this scenario, a request could be to match input and output reflectance (or transmittance) or to match input and output radiance under user selected illuminants. These spectral matching capabilities would require far more computational power than that needed for the ICC colorimetric approach. In order to discuss efficient approaches to this problem, it is first necessary to outline the type of demands to which such a system might be subject.2. SPECTRAL COLOR MANAGEMENTThe discussion of how spectral color management strategies might proceed has only recently begun within the community.1012 Once the spectra of an incoming image is known, either in terms of reflectance or radiance, those data could be harnessed to generate a number of useful outcomes. A reproduction which matches the reflectance spectra of an original object would be highly desirable. Theoretically, such a reproduction would preserve color matches over the range of all illuminants and for all observers. Reflectance-based rendering would be less sensitive to small characterization and calibration errors and to rendering noise. Radiance matching could take current viewing conditions into consideration when reconstructing an object’s appearance as it would be under other viewing conditions. Again, sensitivity to noise and error would be reduced. It should be noted, however, that certain appearance attributes such as surface characteristics, surround conditions, selfradiating versus reflective copy, viewing distance, etc. are no more accounted for within a simple spectral color management system then they would be within a traditional ICC system, but such concerns are outside the purview of this paper. The reflectance and radiance matching tasks referred to above are only the most obvious spectral-based extensions of a colorreproduction infrastructure. New capabilities not previously appreciated will also present themselves. Some examples include: an increased ability to analyze original scenes improving the recognition and reproduction of certain memory colors such as skin tones, grass, sky, etc.; higher levels of within-gamut reproduction quality through the use of multi-channel input devices for which instrumental metamerism, previously unavoidable and the scourge of today’s color reproduction world, would be rare; the introduction of fluorescence as a positive force in color reproduction, unmasked through the acquisition of multiple spectral images taken under different light sources; and, improvement in making spot-color and specialty ink choices. The spectral color reproduction system will have the same basic stages as discussed before and shown in Figure 1a: input, image processing and output. Characterization of input and output devices will need to be carried out, but this time with respect to spectra. It would be very convenient if Figure 1b which describes the ICC logical image processing work flow could be replaced by a similar diagram which simply replaces the word ‘colorimetry’ with ‘spectra’ and the word ‘colorimetric’ with ‘spectral.’ Unfortunately, it does not turn out to be so simple. By increasing the generality of the system, it now needs to obtain added functionality. Within a spectral color management system the following requirements would be necessary: Input profiles could describe any of the following transforms: a) Input digits to reflectance b) Input digits to radiance c) Input digits to colorimetry (not spectral, but good for backwards compatibility) Color processing would need to be able to make the following conversions: d) reflectance to radiance by multiplying by illuminant e) radiance to reflectance by dividing by illuminant f) reflectance to colorimetry by multiplying by illuminant, multiplying by color matching functions and then integrating g) radiance to colorimetry by multiplying by color matching functions and then integrating Output profile could describe any of the following transforms: h) reflectance to output digits i) radiance to output digits j) colorimetry to output digits These basic operations can be applied in series to carry out complex tasks. For example, consider the problem of choosing the right wallpaper for one’s tungsten lit living room. It is well known that the cool white fluorescents in the store can be misleading. Any thinking customer could take out a multispectral camera, capture a picture of the wallpaper in the store and take a second shot of the store’s lights. At home the two images would be downloaded to the computer. Using the camera’s spectral profile, each image would be converted to radiance (functionality ‘b’, above). Using the radiance image of the store light source, the wallpaper radiance image could then be transformed to reflectance (functionality ‘e’, above – this is not true reflectance. This pseudo-reflectance will be discussed below). A subsequent picture of the living room light allows for calculation of what the wallpaper would have looked like at home (functionality ‘d’, above). Finally, to view the color image on the home monitor, the radiance image needs to be converted to XYZ (functionality ‘g’, above) and then the ICC monitor profile would be used to transform to monitor RGB (functionality ‘j’, above). Figure 2 illustrates a cartoon of the user action in this example. Figure 3 shows the series of actions taken by the spectral color management system.Figure 2: Spectral color management would provide a way to impose a new light source on the image of a captured object.Input Device Characterized with respect to RadianceWallpaper Captured by Multi-Channel Input DeviceStore Light Source Captured by Multi-Channel Input Devicestore light input imageLiving Room Light Source Captured by Multi-Channel Input Deviceinput profilewallpaper in store input imageliving room light input imageApply Input Profile Transform to Radiancewallpaper in store radiance image store light radiance imageDivide by Light Sourcewallpaper pseudo-reflectance imageliving room light radiance imageMultiply by Light Sourcewallpaper in living room radiance imageMultiply by Color Matching Functions and Integrate Monitor Characterized with respect to Colorimetry (ICC)wallpaper in living room XYZ imageoutput profileApply Output Profile Transform to Monitor Digitswallpaper in living room RGB monitor imageFigure 3: Block diagram illustrating the logical color management system actions which would accompany the wallpaper example described above. The wallpaper radiance image has the store light source divided away and then is converted to a new radiance image with the living room light source multiplied into it. The new image is displayed colorimetricly on a monitor.Dividing the radiance image by the store light source would not return, strictly, a reflectance image. The resultant image would still contain the effect of uneven illumination and gloss. Also, it would be impossible without refering to a known reflector in the scene to assign an absolute reflectance level to anywhere in the image. All values would be relative. After the division, a first pixel with twice the value of a second pixel in the same band would certainly have reflected twice the photons toward the camera as the second pixel did. It would be impossible, though, to determine if this was because the surface imaged by the first pixel had twice the reflectance of the surface associated with the second pixel or whether the first surface was illuminated with twice the light as the second surface, or some combination of differences in illumination level andreflectance. Specular highlights would be impossible to distinguish from highly reflective areas of the scene. If specular highlights were interpreted as lambertian reflectors, then the overall absolute reflectances in the scene would be underpredicted. This pseudo-reflectance should not be dismissed as being without value, though. By using such an image, as was done in the previous example, a resultant image can simulate the appearance of replacing the original store light bulbs with the living room light bulbs along with the same levels of uneven illumination. For a second example, the reflectance reproduction of a painting is described. This example contains a far less complicated set of transformations than the previous, wallpaper, example. Here, a multi-channel scanner would be chosen to capture the input image. The input profile relates scanner digits to reflectance. For an output device, a multi-ink printer would be the desired rendering engine. An output profile relates reflectance to printer digits. The reflectance image is manipulated by the output transformation which yields printer digits. The digits are printed and the reflectance match is consummated. Figure 4 is a cartoon representing this example and Figure 5 shows the color management steps.Figure 4: Spectral color management would provide a way to match the reflectance of a captured object.Scanner Characterized with respect to ReflectancePainting Captured by Multi-Channel Scannerinput profilepainting input imageApply Input Profile Transform to Reflectance Printer Characterized with respect to Reflectancepainting reflectance imageoutput profileApply Output Profile Transform to Printer Digitspainting multi-ink printer imageFigure 5: Block diagram illustrating the logical color management system actions which would accompany the painting reproduction example described above. The painting reflectance image is converted to printer digits and then printed.3. THE PROBLEM: SPECTRA TO DIGIT TRANSFORMSThe painting reflectance reproduction outlined in Figure 5 seems like a comparatively simple task when compared to the wallpaper matching example, found in Figure 3. Although it has far fewer transformations than the previous example, it is deceptive in its apparent simplicity. The major question being explored by this paper concerns how an efficient transform from spectra to output digit might be designed. In Figure 5, the box labeled “Apply Output Profile Transform to Printer Digits” is central to this question. It is there that a transform which accepts spectra must determine which digits are to be fed to the output device. A spectral sampling frequency might be every 10nm from 400nm to 700nm. This would mean that every pixel for an image with such a sampling would have 31 values associated with it, in essence a 31-dimensional image. To make the problem easier, one might sample the spectra every 20nm yielding a 16-dimensional image or every 40nm for an 8- or 9-dimensional image. Further downsampling is possible, but the loss of spectral detail will eventually return the image to the wide-band domain with no advantage over current RGB devices. Traditional color management tools available to carry out transforms in highly efficient manners include matrix multiplies, one-dimensional lookups and multi-dimensional lookups. Applying one-dimensional lookups to the individual bands of a multi-channel image would not be a costly enterprise. Even performing a matrix multiply would not be particularly expensive for modern computers. It is the application of a multi-dimensional lookup table to an 8-, 16- or 31-dimensional image which would be overwhelming due to the memory requirements of such a huge table. Due to the non-linear characteristics of printer physics, it is inevitable that a transformation between spectra and printer digits will eventually require a computationally expensive step. Within the realm of color management when such transforms need to be applied in an efficient manner, multi-dimensional lookups are the transforms of choice.4. METHODThe method described here can easily be customized to particular needs where tradeoffs can be biased among desired precision, processing time requirements, available computational power and memory constraints. A statement of the aim of the method is as follows: reduce the dimensionality of the input to no more than the dimensionality of the output. In other words, if there are input spectra described by N sample points per pixel and the image is being processed for output to an Mink per pixel printer, the task begins as an N to M problem but reduces to an M to M problem. The savings can be tremendous. If transforming from a 31 sample point per pixel input to a 6-ink printer, the problem reduces from a 31- to 6dimensional transform to no greater than a 6- to 6-dimensional transform. In our own case, the model we have been exercising for a 6-ink printer9 assumes no more than 4 inks printed for any particular pixel. For such a case, the problem is further reduced to a 4- to 4-dimensional transform. Reduction of input dimensionality from N to M is handled by carefully choosing a set of M spectral curves to be used for analyzing the source spectra. While processing a source pixel, weightings are derived for the M chosen curves such that the weighted sum best represents the original N point spectrum. It is these weightings which are used as lookup values for the final M to M lookup as shown in Figure 6.00a*00450500550600650700+1 0.9 0.8 0.7 0.6 0.5 0.4 0.3 0.2 0.10 400450500550600650700≈b*400450500550600650700+ c* d*0 450 500 550 600 650 700 450 500 550 600 650 700CMYKout= LUT(a,b,c,d)+(a)(b)(c)(d)Figure 6: Reduction of dimensionality, starting with a 31- to 4-dimensional problem and reducing it to a 4- to 4dimensional problem. (a) 31 input bands. (b) Each pixel represents 31 samples of a reflectance spectrum. (c) Derive weightings for a set of fixed spectra such that the sum of the weighted spectra is an approximation of the original spectrum. (d) Weights are used as input to a 4- to 4-dimensional lookup table.In a standard colorimetry-based image processing approach, the printer characterization starts with either the construction of a physical model of the printer or, more commonly, a brute force gamut-wide sampling takes place. This printer model can be used to report the colorimetry expected from rendering a set of printer digits. If a physical model were derived and it was mathematically invertible, then the inverse relationship would be easily found. For a sampling-based model or for mathematically non-invertible models, search methods are employed to efficiently guess which digits might yield a particular colorimetric value. Typically off-line, a three-dimensional lookup table indexed by regularly spaced colorimetric values will be built. Search methods are used to populate the lookup table with printer digits. Figure 7 demonstrates the building of such a lookup table.Produce Regular Grid of Colorimetric Valuescolorimetric valuesDerive Printer Colorimetric Model (digit -> colorimetry)digit -> colorimetry printer modelInvert Printer Colorimetric Model (colorimetry -> digit)printer digitsStore Inverted Model3D LUTFigure 7: Process for creating a printer characterization for a colorimetric-based color management system.The spectral approach has a flow similar to the colorimetric characterization process. It is illustrated in Figure 8. A printer model is needed which reports reflectance given a printer digit. This might be a physically derived model or one based upon the measurement of a plethora of printed samples. As in the colorimetric approach, the inversion process would useProduce Regular Grid of M gain factorsChoose M Spectral Curves as Grid Curvesgain factorsgrid curvesMultiply Each Grid Curve by Associated Gain Factor and Sumreflectance spectraDerive Printer Spectral Model (digit -> reflectance)digit -> reflectance printer modelInvert Printer Spectral Model (reflectance -> digit)printer digitsStore Inverted ModelMD LUTFigure 8: Process for creating a printer characterization for a spectral-based color management system.optimization techniques to exercise the printer model until a grid request was satisfied. It is the production of the grids which deviates significantly from the colorimetric approach. If, alternatively, there were no deviations and the colorimetric model had been faithfully followed, a regular grid of spectral domain values would need to be processed. As already pointed out, this could be an 8-, 16- or 31-dimensional grid. Obviously such lookup tables would be absurdly large. Our approach, instead, is to choose a set of M spectral curves which will be referred to as “grid curves.” A regular M-dimensional grid of gain factors is constructed where each dimension is associated with a single grid curve. For each node in the grid, the gain factors are applied to the respective grid curves and the M gained spectra are summed. The summed spectra produce a unique spectrum and this spectrum becomes associated with the gain factors which lookup to that node. This unique spectrum is then inverted and the derived digits are stored at the node. Thus, if a spectrum were completely decomposed into the M grid curves, the gain factors for that spectrum could be looked up in the table and the appropriate printer digits would be found such that when those digits were fed to the printer, the reflectance spectrum would be rendered. This is shown in Figure 9.grid curvesDecompose Reflectance Image With Respect to Grid Curvesgain factorsreflectance imageMD LUTLookup Gain Factors in MD LUT (gain factors -> digit)printer digitsFigure 9: Image processing with spectral lookup method. Each reflectance image pixel is decomposed into gain factors associated with the grid curves. The lookup table constructed in Figure 8 expects these values as input and reports printer digits.5. CONCLUSIONSA method for reducing the dimensionality demands of spectral color management has been introduced. Without such approaches, spectral color management would remain a very slow process or would make memory demands far exceeding today’s capabilities. The method is fairly simple. It involves creating a low-dimensional lookup table or set of lookup tables which can be accessed with values derived through the analysis of image spectral curves. These analyses involve decomposing the spectral curves into a standard set of curves known as “grid curves.” Future discussions will include describing how to choose grid curves, decomposition approaches, and alternative spectral spaces within which such decomposition has greater physical meaning and thus lookup error is reduced.6. ACKNOWLEDGEMENTSThe authors would like to express their gratitude to Fuji Xerox Corporation for its support of this work. We would also like to acknowledge the many members of the Munsell Color Science community who are working on research which either directly feeds this study or which conjures new questions helping to guide our approach. We recognize Mark Fairchild for encouraging the realization of a spectral image visualization tool, now grown into Spectralizer.12 The process around designing and building that tool has helped to cement many of the issues discussed in this paper.7. REFERENCES1. 2. 3. 4. Good examples of such papers may be found in Proc. of the International Symposium on Multispectral Imaging and Color Reproduction for Digital Archives (1999) and papers from sessions 1, 2 and 3 in Proc. of SPIE 3963 (2000). S. Tominaga, , “Spectral Imaging by a Multi-Channel Camera”, Proc. of SPIE 3648, pg. 38 (1999). P. D. Burns and R. S. Berns, “Analysis of multispectral image capture”, Proc. 4th IS&T/SID Color Imaging Conference, 19 (1996). F. H. Imai and R. S. Berns, “High-resolution Multi-Spectral Image Archives: A Hybrid Approach”, Proc. of The Sixth Color Imaging Conference: Color Science, Systems, and Applications, 224 (1998).5.G. M. Johnson and M. D. Fairchild, “Full-Spectral Color Calculations in Realistic Image Synthesis,” IEEE Computer Graphics and Applications, 19, 4 (1999). 6. D. Tzeng,” Spectral-Based Color Separation Algorithm Development for Multiple-Ink Color Reproduction”, Ph.D. dissertation, Rochester Institute of Technology (1999). 7. M. Rosen, X. Jiang, “Lippmann2000: A spectral image database under construction”, Proc. of the International Symposium on Multispectral Imaging and Color Reproduction for Digital Archives (1999). 8. F.H. Imai, M. Rosen, R. Berns, D. Tzeng, “Spectral Reproduction from Scene to Hardcopy II: Image Input and Output”, Submitted to EI 2001. 9. K Iino and R. Berns, “Building Color Management Modules Using Linear Optimization II. Prepress System for Offset Printing”, Journal of Imaging Science and Technology, 42, 2 (1998). 10. P. Hung, “Color Reproduction Using Spectral Characterization”, International Symposium on Multispectral Imaging and Color Reproduction for Digital Archives, pp. 98-105 (1999). 11. B. Hill, “Color capture, color management and the problem of metamerism: does multispectral imaging offer the solution?”, Color Imaging: Device-Independent Color, Color Hardcopy, and Graphic Arts V, R. Eschbach, G. G. Marcu, Editors, Proc. of SPIE 3963 Bellingham, WA, pp.2-14 (2000). 12. M. Rosen, M. Fairchild, G. Johnson, D. Wyble, “Color Management within a Spectral Image Visualization Tool”, submitted to CIC 2000.。