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 in a region covered from 150 to 500 stellar radii the emission pattern is characterised by energies in the interval ( 0.1 − 10 ) $(0.1-10)$ MeV.

中文翻译：

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脉冲星磁层深处的同步辐射

在本文中，我们研究了普通脉冲星高能发射的产生。为此，我们考虑在外磁层中加速的粒子沿闭合磁场线滑动。已经表明，在适当的运动过程中，初始小俯仰角增加，并且在距中子星一定距离处，同步加速器发射变得显着。我们发现，在一个覆盖 150 到 500 个恒星半径的区域中，发射模式的特征在于区间 (0.1 - 10) $(0.1-10)$ MeV 中的能量。