摘要
本文从Lorentz协变方程和推迟势出发,讨论了在脉冲星表面磁层强磁场条件下电子的运动和辐射.并根据天体物理的有关实测数据参数,给出了曲率辐射表达式的具体形式及临界频率与峰频的数值.
This paper ,taking lorentz covariant equation and retarded potential as starting point, is to discuss the motion and radiation of electron under circumstance of strong magnetic field in magnetic lager of pulsar surface . According to the measured data and parameters of Astrophysics, the concrete form of curvature radiation expression ,the numerical value of critical and peak frequencies are presented here.
出处
《新疆师范大学学报(自然科学版)》
1996年第1期17-21,共5页
Journal of Xinjiang Normal University(Natural Sciences Edition)
关键词
脉冲星
表面磁层
曲率辐射
极冠模型
Pulsar Surface magnetic layer Curvature radition Polar gap model.