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Extreme Spectral Power Distribution of Light Source and its Impact to Vision and Cameras Sensitivity

机译:光源的极端光谱配电及其对视觉和相机敏感性的影响

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Thanks to the advancement of technologies, we may be having more flexibility to determine the spectral power distribution (SPD) of light sources. Suppose any SPD is possible, we derive "extreme SPD of light source" aiming at a specific purpose such as the lowest energy, the largest color gamut, the lowest impact to fine arts, etc. We found that these SPDs always consist of multiple spikes when very high CR1 is not required while the SPD of the black body radiation is continuous in wavelength. In order to investigate the effect of such light sources to human visual system and camera system, we employ two types of such light sources, namely Maximum White Luminous Efficacy of Radiation (MWLER), which gives the best energy efficiency, and Maximum Gamut Area (MGA), which gives the largest color gamut size. Both MWLER and MGA are composed of multiple spikes in wavelength. We generate such SPDs with respect to 6 types of existing light sources with same CCT and CRI (if applicable), and evaluate how sensitive these are with 10 sets of color matching functions (CMFs) given by Stiles and Burch as human visual system and 4 sets of digital camera sensitivities by computer simulation. We presume a color matrix of color conversion for CMFs and camera is adjusted minimizing errors with a Macbeth Color Checker under black body radiation with the white point constraint. With this assumption, we evaluate colorimetric error under the two extreme SPDs in addition to black body radiation and existing light sources. We find that cameras give large error (more than 20 in AE*_(ab)) for these spiky light sources which may not be accepted by users even when they are in a tolerable error range for the human visual system. It is concluded that such spiky light source could be used without problem for a variation of CMFs, but it would be problematic for color reproduction of cameras.
机译:由于技术的进步,我们可具有更大的灵活性来确定的光源的光谱功率分布(SPD)。假设任何SPD是可能的,我们得出“光源的极端SPD”针对某一特定的目的,如能量最低,最大的色域,美术最低的影响,等等。我们发现,这些浪涌保护器总是由多个尖峰当不需要非常高的CR1而黑体辐射的SPD是在波长连续的。为了研究这种光源对人类视觉系统和摄像系统的影响,我们采用两种这样的光源,辐射(MWLER),提供了最好的能效即最大白色发光效率和最大色域面积( MGA),这给最大的色域大小。既MWLER和MGA是由在波长多个尖峰。我们生成这样的SPD相对于6种现有用相同CCT和CRI(如果适用)的光源,以及评估如何敏感这些都是由窗框和伯奇给定为人类视觉系统和4 10套色匹配函数(CMFS)台通过计算机仿真数码相机灵敏度。我们推测色彩转换的色彩矩阵CMFS和相机调整下黑体辐射和白色点约束减少了麦克贝思色卡错误。在这个假设下,我们评估除了黑体辐射与现有光源的两个极端的SPD下色度误差。我们发现,摄像机产生较大的误差(20以上的AE * _(AB))对可能不是用户,即使他们是在一个可容忍的误差范围为人类视觉系统接受这些尖刻的光源。可以得出结论,这种高低不平的光源可以没有问题地用于CMFS的变型,但它是用于照相机的色彩再现的问题。

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