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Analysis of Spectroscopic Observations of Jupiter and the Variability of the Structure of the Visible Clouds

Published online by Cambridge University Press:  14 August 2015

G. E. Hunt  and
J. T. Bergstralh
G. E. Hunt
Affiliation:
Meteorological Office, Bracknell, Berkshire, England
J. T. Bergstralh
Affiliation:
Jet Propulsion Laboratory, Pasadena, Calif., U.S.A.

Abstract

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Realistic inhomogeneous models of Jupiter's lower atmosphere are used to interpret recent observations of the (3–0) and (4–0) H2 quadrupole lines at different portions of the visible disc of the planet. The time variations of these observations are analysed in terms of changes in the cloud structure.

Type
Part III Outer Planets and Their Satellites
Information
Symposium - International Astronomical Union , Volume 65: Exploration of the Planetary System , 1974 , pp. 385 - 387
Copyright
Copyright © Reidel 1974 

References

Bergstralh, J. T.: 1973, Icarus 19, 390.Google Scholar
Divine, N.: 1971, ‘The Planet Jupiter’ SP, 8069.Google Scholar
Hunt, G. E.: 1973a, Icarus 18, 637.Google Scholar
Hunt, G. E.: 1973b, Monthly Notices Roy. Astron. Soc. 161, 347.Google Scholar
Hunt, G. E. and Margolis, J. S.: 1973, J. Quant. Spectrosc. Radiat. Transfer 13, 417.Google Scholar