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射电脉冲星的磁层与辐射机制理论
引用本文:张冰,乔国俊.射电脉冲星的磁层与辐射机制理论[J].天文学进展,1996,14(4):332-352.
作者姓名:张冰  乔国俊
作者单位:北京大学地球物理系,北京大学地球物理系 北京 100871,北京 100871
摘    要:在本文中简介强磁场中一些特殊理过程的特性,在此基础上综述了射电脉冲星的磁层与辐射机理理论。关于磁层,主要由GJ模型了发,从斜转子磁层、加速区机制及回路问题三方面总结前人对磁层问题的认识。

关 键 词:射电脉冲星  磁层  辐射机制理论  脉冲星

Theories of Magnetosphere and Radiation Mechanism of Radio Pulsar
Zhang Bing,Qiao Guojun.Theories of Magnetosphere and Radiation Mechanism of Radio Pulsar[J].Progress In Astronomy,1996,14(4):332-352.
Authors:Zhang Bing  Qiao Guojun
Institution:Zhang Bing,Qiao Guojun Department of Geophysics,Peking University Beijng 100871 Received 1995 October 7, revised 1996 September 3
Abstract:In this paper, properties of some special processes in strong magnetic fields are brieflyintroduced, and the theories on magnetosphere and radiation mechanism of radio pulsar arereviewed. As to the magnetospheric models, we start with the GJ model, and then deal withthe three important problems: the oblique rotator, the site and the mechanism of particleacceleration, and the current closure problem. As to the radiation mechanism, we focus on the"coherent problem", and point out the advantages of the Inverse Compton Scattering model.Some comments on the models are presented in the end.
Keywords:star  neutron--pulsars  general--radiation mechanism  non--thermal-magnetic fields
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