Toward an Empirical Theory of Pulsar Emission. VI. The Geometry of the Conal Emission Region
Toward an Empirical Theory of Pulsar Emission. VI. The Geometry of the Conal Emission Region
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DOI：
10.1086/172361
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发表时间：
1993-03
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影响因子：
--
通讯作者：
J. Rankin
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文献类型：
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作者：
J. Rankin
本文提出了一个经验分析的几何形状的锥形发射区的总人口约150个卫星，其中有足够的身体的观测现在存在。它继续了在以前的论文中开始的分析，该论文探索了核心发射区的几何形状，并提供了一种估计具有核心组件的恒星的旋转轴和磁轴之间的角度α的方法。因此，根据其形态学分类，将各种植物分为几组，首先处理那些具有核心成分的物种。特别考虑到五组分（M）类和与之密切相关的其他完全锥形的种类，锥形三联体（cT）和锥形四联体（cQ）
This paper presents an empirical analysis of the geometry of the conal emission region for a total population of some 150 pulsars for which an adequate body of observations now exists. It continues the analysis begun in a previous paper that explored the geometry of the core emission region and provided a means of estimating the angle α between the rotation and magnetic axes of pulsars with core components. The various pulsars are thus divided into groups according to their morphological classification, and those species that have core components are treated first. Special consideration is given to the five-component (M) class and to those other, entirely conal species which are closely related to it, the conal triple (cT) and the conal quadruple (cQ)