RING ATMOSPHERE OF SATURN: MONTE CARLO SIMULATION OF RING SOURCE MODELS.

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Abstract

The spatial distribution of hydrogen atoms emitted from the rings of Saturn with a range of emission speeds are simulated by a Monte Carlo technique. This method makes it possible to examine the spatial profiles of the ring atmosphere under a variety of physical conditions.

Original languageEnglish
Pages (from-to)8843-8849
Number of pages7
JournalJournal of Geophysical Research E: Planets
Volume89
Issue numberA10
DOIs
StatePublished - 1984

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