| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10705227 | Planetary and Space Science | 2012 | 17 Pages |
Abstract
⺠Theoretical study of how solar wind affects Jupiter's magnetosphere-ionosphere system. ⺠Power dissipated in atmosphere is anti-correlated with solar wind pressure. ⺠Power dissipated in magnetosphere is a maximum for solar wind pressure â¼0.02-0.06 nPa. ⺠Auroral emission and brightness increase with magnetospheric size. ⺠Value of radial current at infinity influences magnetodisc structure.
Related Topics
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Authors
J.N. Yates, N. Achilleos, P. Guio,