Physics of pulsar magnetospheres
Physics of pulsar magnetospheres
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DOI：
10.1070/pu1986v029n10abeh003528
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发表时间：
1986-10
期刊：
影响因子：
2.7
通讯作者：
V. S. Beskin;A. Gurevich;Y. Istomin
中科院分区：
文献类型：
--
作者：
V. S. Beskin;A. Gurevich;Y. Istomin
构建了脉冲星磁层的自洽模型。该模型基于描述磁层整体特性的方程的连续解以及对已发展的理论和观测数据的基本预测的比较。
A self-consistent model of the magnetosphere of a pulsar is constructed. This model is based on a successive solution of the equations describing global properties of the magnetosphere and on a comparison of the basic predictions of the developed theory and observational data.