| タイトル | Is Jupiter's magnetosphere like a pulsar's or earth's? |
| 本文（外部サイト） | http://hdl.handle.net/2060/19750002817 |
| 著者（英） | Coroniti, F. V.; Kennel, C. F. |
| 著者所属（英） | California Univ. |
| 発行日 | 1974-09-01 |
| 言語 | eng |
| 内容記述 | The application of pulsar physics to determine the magnetic structure in the planet Jupiter outer magnetosphere is discussed. A variety of theoretical models are developed to illuminate broad areas of consistency and conflict between theory and experiment. Two possible models of Jupiter's magnetosphere, a pulsar-like radial outflow model and an earth-like convection model, are examined. A compilation of the simple order of magnitude estimates derivable from the various models is provided. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 75N10889
PUBL-1353
NASA-CR-140600
PPG-188 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/192261 |
