SPATIALLY RESOLVED HIGH RESOLUTION SPECTROSCOPY OF $H_{2}$ AND $NH_{3}$ IN THE ATMOSPHERE OF JUPITER

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1976-RN-12.jpg (61.76 KB)

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1976

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Ohio State University

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Abstract

Observational determination of the variation of the equivalent widths of molecular features in the atmosphere of Jupiter as observations are taken from the center of the disc to the limb are given. These observed variations are related to models for the vertical structure of the Jovian atmosphere.

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This research was supported by ERDA.
Author Institution: Princeton University Observatory

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http://hdl.handle.net/1811/9732

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Abstracts of OSU International Symposium on Molecular Spectroscopy 1970-1979