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Radiative transfer and remote sensingRadiative 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.
Document ID
19820017169
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Conrath, B. J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 10, 2013
Publication Date
April 1, 1982
Publication Information
Publication: Vibrational-Rotational Spectry. for Planetary Atmospheres, Vol. 1
Subject Category
Lunar And Planetary Exploration
Accession Number
82N25045
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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