论文标题

城市灯光景观

Spectrometry of the Urban Lightscape

论文作者

Small, Christopher

论文摘要

NASA的通往地球宇航员摄影的门户包含30000多张从国际空间站拍摄的2500张城市灯光景观(Urban Night Lights)的照片。超过100多个多光谱的数码单反相机的照片具有足够的空间分辨率,清晰度和暴露,可用于城市光景的宽带光谱表征。分析来自Modtran辐射转移模型的模拟大气传播率表明,透射率光谱的光谱斜率对选择模型Atmopshere的选择相对不敏感,并且大气路径长度和气溶胶光学上流的变化主要影响光谱的偏置,而不是斜率。这表明,可以校正由颜色温度校准的RGB通道的相对差异,以纠正大气散射和吸收以允许定量比较。 18个插图的RGB照片的镶嵌物为光谱空间提供了四个明确定义的光谱末端,对应于白色,黄色和红色光源,并由深色背景末端成员调节亮度。这四个光谱末端成员构成了线性光谱混合模型的基础,该模型可以倒置以提供每个像素瞬时视野中存在的每个端成的面积分数。所得的光谱特征空间显示了两个不同的混合趋势,这些趋势从黑暗的末端到近乎平坦的光谱(白黄色)和温暖光谱(橙色)源。照明像素的分布强烈偏向较低的温度街道照明的亮度背景,较亮的灯通常与点源和主要通道相对应。尽管暴露和内部混合趋势有所不同,但18个单独的城市光谱特征空间的比对表现出一致的拓扑。

NASA's Gateway to Astronaut Photography of Earth Contains over 30000 photos of 2500 cataloged urban lightscapes (urban night lights) taken from the International Space Station. Over 100 of these multispectral DSLR photos are of sufficient spatial resolution, sharpness and exposure to be used for broadband spectral characterization of urban lightscapes. Analysis of simulated atmospheric transmissivity from the MODTRAN radiative transfer model shows that spectral slopes of transmissivity spectra are relatively insensitive to choice of model atmopshere, with variations in atmospheric path length and aerosol optical depth primarily affecting the bias of the spectrum rather than the slope. This suggests that color tempterature-calibrated RGB channels can be corrected for relative differences in atmospheric scattering and absorption to allow for quantitative intercomparison. A mosaic of 18 intercalibrated RGB photos renders a spectral feature space with four clearly defined spectral endmembers corresponding to white, yellow and red light sources, with brightness modulated by a dark background endmember. These four spectral endmembers form the basis of a linear spectral mixture model which can be inverted to provide estimates of the areal fraction of each endmember present within every pixel instantaneous field of view. The resulting spectral feature space shows two distinct mixing trends extending from the dark endmember to near flat spectrum (white-yellow) and warm spectrum (orange) sources. The distribution of illuminated pixels is strongly skewed toward a lower luminance background of warm spectrum street lighting, with brighter lights generally corresponding to point sources and major thoroughfares. Intercomparison of 18 individual urban lightscape spectral feature spaces show consistent topology, despite variations in exposure and interior mixing trends.

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