Anisotropy in the Arrival Directions of Ultrahigh-Energy Cosmic Rays

被引：0

作者：

Villasenor, Luis ^{[1
]}

机构：

[1] Benemerita Univ Autonoma Puebla, Puebla, Mexico

来源：

VI SCHOOL ON COSMIC RAYS AND ASTROPHYSICS | 2017年 / 866卷

关键词：

D O I：

10.1088/1742-6596/866/1/012014

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this article we illustrate, in an interactive way, the analysis and visualization of anisotropy properties in the arrival directions of ultrahigh-energy cosmic rays detected by the Telescope Array and the Pierre Auger experiments by using data released by both collaborations. We describe the use of several programs that we have written in Python and Julia languages for this purpose. We also discuss the potential sources and analyse the effect of correcting the arrival directions to take into account the deflections of the cosmic rays by the magnetic field of our galaxy for one specific model of the galactic magnetic field under several assumptions about the composition of the primary cosmic rays.

引用

页数：15

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