The spin - down rate has been measured for almost every radio pulsar, and theory indicates that it depends on the strength of the star 's magnetic field.
这种自转变慢的速率，几乎每一颗无线电波霎都量得到，而理论指出，此速率和星体的磁场强度有关。
In this paper, the magnetospheric structure of pulsar is discussed for the forced magnetic field.
本文讨论有力场的脉冲星磁层结构。用极角展开的方法。
In this paper, the magnetospheric structure of pulsar is discussed for the forced magnetic field.
本文讨论有力场的脉冲星磁层结构。用极角展开的方法。
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