Science. 1991 Apr 19;252(5004):410-5. doi: 10.1126/science.252.5004.410.
Before direct exploration by spacecraft, Jupiter was the only planet other than Earth that was known to have a magnetic field, as revealed by its nonthermal radio emissions. The term "magnetosphere" did not exist because there was no clear concept of such an entity. The space age provided the opportunity to explore Earth's neighborhood in space and to send instruments to seven of the other eight planets. It was found that interplanetary space is pervaded by a supersonic "solar wind" plasma and that six planets, including Earth, have magnetic fields of sufficient strength to deflect this solar wind and form a comet-shaped cavity called a magnetosphere. Comparative study of these magnetospheres aims to elucidate both the general principles and characteristics that they share in common, and the specific environmental factors that cause the important, and sometimes dramatic, differences in behavior between any two of them. A general understanding of planetary magnetospheres holds the promise of wide applicability in astrophysics, which, for the indefinite future, must rely solely on remote sensing for experimental data.
在航天器直接探测之前,木星是除地球之外唯一已知具有磁场的行星,其非热射电辐射揭示了这一点。由于没有关于这种实体的明确概念,因此“磁层”一词并不存在。太空时代提供了探索地球近地空间并向其他八颗行星中的七颗发送仪器的机会。人们发现,行星际空间充满了超音速的“太阳风”等离子体,其中包括地球在内的六颗行星具有足够强的磁场,可以偏转这种太阳风并形成一个彗星形的空腔,称为磁层。对这些磁层的比较研究旨在阐明它们共同具有的一般原理和特征,以及导致它们之间任何两个之间的行为存在重要且有时是戏剧性差异的具体环境因素。对行星磁层的普遍理解有望在天体物理学中得到广泛应用,而天体物理学在可预见的未来,必须仅依靠遥感来获取实验数据。