论文标题
脉冲星磁层深处的同步发射
Synchrotron emission from the depths of pulsar magnetospheres
论文作者
论文摘要
在本文中，我们研究了正常脉冲星的高能发射产生。为此，我们考虑沿封闭磁场线滑动的外部磁层中加速的颗粒。已经表明，在适当的运动过程中，初始的小螺距角增加了，并且在与中子恒星的一定距离下同步加速器发射变得显着。我们发现，一个从150美元到$ 500 $恒星Radii覆盖的地区的排放模式的特征是在间隔$（0.1-10）$ MEV中的能量。
In this paper we study the generation of high energy emission from normal pulsars. For this purpose we consider the particles accelerated in the outer magnetosphere sliding along the closed magnetic field lines. It has been shown that in due course of motion the initial small pitch angle increases and at a certain distance from the neutron star the synchrotron emission becomes significant. We found that a region covered from $150$ to $500$ stellar radii the emission pattern is characterised by energies in the interval $(0.1-10)$ MeV.
