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2004/11/02 | 大气遥感[Atmosphere Remote Sensing]
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发表于 16:28
Given a warm surface and a cool atmosphere, radiation detectors receive thermal radiation from the surface at transparent wavelengths and from various atmospheric heights at opaque wavelengths. This allows temperature profiles to be constructed for planetary atmospheres.
Absorption and reflection features which allow the identification of atmospheric composition are electronic transitions (UV), molecular vibrations (IR and near IR), and molecular rotation (IR, far IR).
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