Saturn’s atmospheric response to the large influx of ring material inferred from Cassini INMS measurements
During the Grand Finale stage of the Cassini mission, organic-rich ring material was discovered to be flowing into Saturn’s equatorial upper atmosphere at a surprisingly large rate. Through a series of photochemical models, we have examined the consequences of this ring material on the chemistry of...
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Published in | Icarus (New York, N.Y. 1962) Vol. 391; p. 115328 |
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Main Authors | , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier Inc
01.02.2023
Elsevier |
Subjects | |
Online Access | Get full text |
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