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Theoretical Studies of an Atmosphere Around Saturn's Rings

Published online by Cambridge University Press:  14 August 2015

M. Dennefeld
M. Dennefeld*
Affiliation:
Service d'Aéronomie, Verrières-le-Buisson, France

Abstract

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The subject of this paper is an attempt to predict what can be seen in the vicinity of Saturn through a UV photometer on board the Mariner-Jupiter-Saturn mission. We will restrict ourselves to the study of atomic hydrogen and OH and to H2O which can be the parent molecule and will consider only the particles ejected from the rings and from Titan.

Type
Part III Outer Planets and Their Satellites
Information
Symposium - International Astronomical Union , Volume 65: Exploration of the Planetary System , 1974 , pp. 471 - 481
Copyright
Copyright © Reidel 1974 

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