CONFIGURATION OF THE JOVIAN MAGNETOSPHERE

被引：175

作者：

Hill, T. W. ^{[1
]}

Dessler, A. J. ^{[1
]}

Michel, F. C. ^{[1
]}

机构：

[1] Rice Univ, Dept Space Phys & Astron, Houston, TX 77001 USA

来源：

GEOPHYSICAL RESEARCH LETTERS | 1974年 / 1卷 / 01期

基金：

美国国家航空航天局;

关键词：

D O I：

10.1029/GL001i001p00003

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

We present a model in which the Jovian magnetosphere is severely inflated by the centrifugal stress of partially-corotating plasma streaming out along field lines from the ionosphere. The model is consistent with observations reported from the Pioneer 10 encounter, including the disc-like field configuration, the diurnal modulation of trapped-particle fluxes, and the inferred departure from rigid corotation in the outer magnetosphere. The field configuration is closed on the dayside, but on the night side the plasma can force the magnetic field open to form a planetary wind flowing in the antisolar direction.

引用

页数：4

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