摘要
From a re-examination of the trajectories of small charged grains in the vicinity of the Saturnian rings, it is shown that the orbital motion of positively charged grains with a charge-to-mass ratio on the order of 10 -6 e amu-1 could allow the injection of water material into the equatorial atmosphere. Thus, a mechanism of ionospheric depletion in the equatorial region is provided, as indicated by the Cassini radio occultation measurements.
原文 | ???core.languages.en_GB??? |
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文章編號 | 34 |
期刊 | Astrophysical Journal |
卷 | 786 |
發行號 | 1 |
DOIs | |
出版狀態 | 已出版 - 1 5月 2014 |