THE NATURE OF PULSAR SUBPULSE DRIFT

被引:32
作者
KAZBEGI, AZ
MACHABELI, GZ
MELIKIDZE, GI
机构
来源
AUSTRALIAN JOURNAL OF PHYSICS | 1991年 / 44卷 / 05期
关键词
D O I
10.1071/PH910573
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
A possible mechanism for the explanation of pulsar subpulse drift is suggested. In the region of the open magnetic field lines the existence of an electron-positron plasma penetrated by a primary particle beam is assumed. There is a possibility of excitation of large-scale drift waves propagating transversely to the magnetic field lines. These waves can affect the fulfilment of the radio-wave generation conditions. If the pulsar angular velocity is near to the frequency of the drift waves one should observe regular drift phenomena.
引用
收藏
页码:573 / 584
页数:12
相关论文
共 25 条