机构地区: 北京大学
出 处: 《河北工学院学报》 1994年第4期77-81,共5页
摘 要: 介绍了脉冲星的磁偶极辐射模型,以及这个模型在理论与观测的比较上所存在的一些困难.还介绍了一种修正的脉冲星辐射模型,这个模型通过假定板冠区的低频偶极辐射。 We introduce the magnetic dipole radiation model of pulsar,and the difficulties of this theoretical model comparing with the observation.We also introduce a modified radiation model of pulsar,which assumes that the radiation is originated from the low freqency dipole radiation on the polar cap,and it solves the magnetic evolutiion problem.