摘要
If the solar radiation pressure effect is taken into consideration, the structure of the atomic hydrogen cloud emitted from Titan would be significantly modified. Instead of a circular torus characterized by azimuthal symmetry and with density peak near the orbit of Titan, the atomic hydrogen cloud will take on a pear-shaped structure with the long-lived H atoms distributed through the whole Saturnian system.
原文 | ???core.languages.en_GB??? |
---|---|
頁(從 - 到) | 335-339 |
頁數 | 5 |
期刊 | Advances in Space Research |
卷 | 13 |
發行號 | 10 |
DOIs | |
出版狀態 | 已出版 - 10月 1993 |