Radiative transfer and remote sensing
Radiative transfer and remote sensing
复制标题
辐射传输和遥感
DOI：
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发表时间：
1982
期刊：
影响因子：
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通讯作者：
B. Conrath
中科院分区：
文献类型：
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作者：
B. Conrath
讨论了行星红外光谱定量解释的基本理论工具——辐射传输。推断了它在将遥感数据与大气特性（成分、热结构、动力学等）联系起来方面所起的作用。简要概述了与行星光谱解释有关的遥感问题。这个演示是教程而不是详尽的。
Radiative transfer, the basic theoretical tool for the quantitative interpretation of planetary infrared spectra, is discussed. The function it plays in linking the remotely sensed data to the properties of the atmosphere (composition, thermal structure, dynamics, etc.), is inferred. A brief overview of the remote sensing problem as it pertains to the interpretation of planetary spectra is presented. The presentation is tutorial rather than exhaustive.