Essential properties of the Difference Method for the Search of the Anisotropy of the Primary Cosmic Radiation

The methodical properties of the original difference method for the search of the anisotropy at the knee region of the primary cosmic radiation energy spectrum are analyzed. The main feature of the suggested method is a study of the difference in the EAS characteristics in different directions but n...

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Published inarXiv.org
Main Authors Pavlyuchenko, V P, Martirosov, R M, Nikolskaya, N M, Erlykin, A D
Format Paper
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 30.09.2015
Subjects
Anisotropy
Anomalies
Celestial sphere
Coordinates
Cosmic rays
Energy spectra
Galaxies
Knee
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Abstract The methodical properties of the original difference method for the search of the anisotropy at the knee region of the primary cosmic radiation energy spectrum are analyzed. The main feature of the suggested method is a study of the difference in the EAS characteristics in different directions but not their intensity. It is shown that the method is stable to the random experimental errors and allows to separate the anomalies related to the laboratory coordinate system from the anomalies in the celestial coordinates. The method uses multiple scattering of the charge particles in the Galaxy magnetic fields to study the whole celestial sphere including the regions outside of the line of sight of the installation.
AbstractList The methodical properties of the original difference method for the search of the anisotropy at the knee region of the primary cosmic radiation energy spectrum are analyzed. The main feature of the suggested method is a study of the difference in the EAS characteristics in different directions but not their intensity. It is shown that the method is stable to the random experimental errors and allows to separate the anomalies related to the laboratory coordinate system from the anomalies in the celestial coordinates. The method uses multiple scattering of the charge particles in the Galaxy magnetic fields to study the whole celestial sphere including the regions outside of the line of sight of the installation.
Author Martirosov, R M
Erlykin, A D
Nikolskaya, N M
Pavlyuchenko, V P
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SubjectTerms Anisotropy
Anomalies
Celestial sphere
Coordinates
Cosmic rays
Energy spectra
Galaxies
Knee
Title Essential properties of the Difference Method for the Search of the Anisotropy of the Primary Cosmic Radiation
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