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

W. H. Ip

doi:10.1029/JA089iA10p08843

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

W. H. Ip

天文研究所

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

18 引文斯高帕斯（Scopus）

摘要

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.

原文	???core.languages.en_GB???
頁（從 - 到）	8843-8849
頁數	7
期刊	Journal of Geophysical Research E: Planets
卷	89
發行號	A10
DOIs	https://doi.org/10.1029/JA089iA10p08843
出版狀態	已出版 - 1984

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10.1029/JA089iA10p08843

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

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