| タイトル | The magnetic field of Jupiter |
| 著者（英） | Acuna, M. H.; Ness, N. F. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 1976-01-01 |
| 言語 | eng |
| 内容記述 | The paper is concerned mainly with the intrinsic planetary field which dominates the inner magnetosphere up to a distance of 10 to 12 Jovian radii where other phenomena, such as ring currents and diamagnetic effects of trapped charged particles, become significant. The main magnetic field of Jupiter as determined by in-situ observations by Pioner 10 and 11 is found to be relatively more complex than a simple offset tilted dipole. Deviations from a simple dipole geometry lead to distortions of the charged particle L shells and warping of the magnetic equator. Enhanced absorption effects associated with Io and Amalthea are predicted. The results are consistent with the conclusions derived from extensive radio observations at decimetric and decametric wavelengths for the planetary field. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 77A21929 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/439233 |
