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Detecting 3D Vegetation Structure with the Galileo Space Probe: Can a Distant Probe Detect Vegetation Structure on Earth?

机译:用伽利略太空探测器探测3D植被结构:遥测探测器能否探测到地球上的植被结构?

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摘要

Sagan et al. (1993) used the Galileo space probe data and first principles to find evidence of life on Earth. Here we ask whether Sagan et al. (1993) could also have detected whether life on Earth had three-dimensional structure, based on the Galileo space probe data. We reanalyse the data from this probe to see if structured vegetation could have been detected in regions with abundant photosynthetic pigments through the anisotropy of reflected shortwave radiation. We compare changing brightness of the Amazon forest (a region where Sagan et al. (1993) noted a red edge in the reflectance spectrum, indicative of photosynthesis) as the planet rotates to a common model of reflectance anisotropy and found measured increase of surface reflectance of 0.019 ± 0.003 versus a 0.007 predicted from only anisotropic effects. We hypothesize the difference was due to minor cloud contamination. However, the Galileo dataset had only a small change in phase angle (sun-satellite position) which reduced the observed anisotropy signal and we demonstrate that theoretically if the probe had a variable phase angle between 0–20°, there would have been a much larger predicted change in surface reflectance of 0.1 and under such a scenario three-dimensional vegetation structure on Earth could possibly have been detected. These results suggest that anisotropic effects may be useful to help determine whether exoplanets have three-dimensional vegetation structure in the future, but that further comparisons between empirical and theoretical results are first necessary.
机译:Sagan等。 (1993)使用伽利略太空探测器的数据和第一原理找到了地球上生命的证据。在这里,我们问是否Sagan等。 (1993)还可以根据伽利略太空探测器的数据检测地球上的生命是否具有三维结构。我们重新分析该探测器的数据,以查看是否可以通过反射短波辐射的各向异性在具有丰富光合色素的区域中检测到结构化植被。当行星旋转到反射率各向异性的通用模型时,我们比较了亚马逊森林(Sagan等人(1993年)在反射光谱中显示红色边缘的区域,该区域反映了光合作用)的变化的亮度,并发现测得的表面反射率增加0.019±0.003相对于仅各向异性效应所预测的0.007。我们假设差异是由于轻微的云污染所致。但是,伽利略数据集的相角(太阳卫星位置)只有很小的变化,这减小了观测到的各向异性信号,并且我们证明了理论上,如果探头的相角在0–20°之间变化,将会有很大的变化。预测的表面反射率的较大变化为0.1,在这种情况下,可能已经检测到地球上的三维植被结构。这些结果表明,各向异性效应可能有助于确定未来系外行星是否具有三维植被结构,但首先需要对经验和理论结果进行进一步比较。

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