Topology of Saturn's main magnetic field

Topology of Saturn's main magnetic field
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土星主磁场的拓扑结构

DOI:
10.1038/292721a0
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发表时间:
1981
期刊:
影响因子:
64.8
通讯作者:
N. Ness
N. Ness
中科院分区:
综合性期刊1区
文献类型:
--
作者:
M. Acuna;J. Connerney;N. Ness

文献摘要

被引文献

相似文献

旅行者一号在土星的磁场观测证实了行星磁场的主要偶极拓扑,并表明需要更通用的模型,其中包含行星外部和行星磁层内部的非势场源。
The Voyager 1 magnetic field observations at Saturn confirm the principally dipolar topology of the planetary magnetic field and suggest the need for more general models which incorporate non-potential field sources external to the planet and within the planetary magnetosphere.