Physics of the Jovian magnetosphere. 10. Magnetospheric models.
Physics of the Jovian magnetosphere. 10. Magnetospheric models.
复制标题
木星磁层物理学。
DOI：
10.1017/cbo9780511564574.012
复制
发表时间：
1983
影响因子：
2.6
通讯作者：
C. Goertz
中科院分区：
文献类型：
--
作者：
T. Hill;A. Dessler;C. Goertz
在已被探索的行星磁层中，木星的磁层是迄今为止最大的。它是一个主要由旋转效应控制的磁层。因此，它提供了独特的见解，难以进入脉冲星磁层的研究。目前的调查是有关的理论概念，被认为是与现有的意见。人们发现，位于伽利略卫星最里面的木卫一是木星磁层等离子体的主要来源。我们考虑了沿着的太阳风源、电离层源、其它卫星源以及木卫一等离子体环的温度和含量随时间的变化。木星的旋转作为磁层现象的主要能源进行了讨论沿着方面的木卫一-木星相互作用。注意力也被给予粒子加速，和自旋周期性。
Of the planetary magnetospheres which have been explored, Jupiter's is by far the largest. It is a magnetosphere largely dominated by rotational effects. As such, it offers unique insight to the study of inaccessible pulsar magnetospheres. The present investigation is concerned with theoretical concepts which are believed to be consistent with available observations. It has been found that Io, the innermost of the Galilean satellites, is the principal source of plasma for the Jovian magnetosphere. The Io source is considered along with the solar-wind source, the ionospheric source, other satellite sources, and variations of the temperature and the content of the Io plasma torus with time. The rotation of Jupiter as the dominant source of energy for magnetospheric phenomena is discussed along with aspects of the Io-Jupiter interaction. Attention is also given to particle acceleration, and spin periodicity.