Comparison of the results of the solar protons release times in solar proton events obtained by various methods

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Abstract

The comparison was made between the values of the solar release times of unrelativistic protons determined on scailing similarity time profiles of solar proton events and results of papers in which the solar release times of relativistic protons in GLE is determined on first observations with utilizing the method of velocity dispersion and on the first observations on neutron monitors with account of the dependence of the length of Sun–Earth magnetic line on solar wind velocity.

About the authors

Yu. P Ochelkov

Institute of Applied Geophysics

Email: yur_och@mail.ru
Moscow, Russia

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