Investigation of primary cosmic rays at energies above 1014 eV

被引：1

作者：

Varga A. ^{[2
]}

Gudkova E.N. ^{[1
]}

Nesterova N.M. ^{[1
]}

Erdesh G. ^{[2
]}

机构：

[1] Lebedev Physics Institute, Russian Academy of Sciences

[2] Central Research Institute for Physics (KFKI), Hungarian Academy of Sciences

来源：

Bulletin of the Russian Academy of Sciences: Physics | 2011年 / 75卷 / 3期

关键词：

Lebedev Physics Institute; Supernova Remnant; Joint Experiment; White Diamond; Cloudless Night;

D O I：

10.3103/S1062873811030452

中图分类号：

学科分类号：

摘要：

A search for sources of primary cosmic rays at energies of 10 14-1015 eV was performed using the special independent KLARA+Khronotron unit at the Tien Shan Mountain Cosmic Ray Station in a joint experiment of the Lebedev Physics Institute (LPI) and the Central Research Institute for Physics (KFKI). A full data bank of standard events, consisting of 30 million extensive air showers (EASes), was analyzed. Analysis results are presented as maps of the directions of EAS arrival in equatorial coordinates in which the standard deviation of the number of events exceeds a certain value. These could be directions from which neutral primary cosmic particles (e.g.; gamma ray photons) arrive from sources of primary cosmic rays. A match is found between separate directions with results, obtained on other stations, and the location of pulsars. © 2011 Allerton Press, Inc.

引用

页码：339 / 341

页数：2

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