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Abstract <p>Times of the release of solar unrelativistic protons, determined from the scale invariance of temporal profiles of solar proton events, are compared to results from studies in which the times of release for solar relativistic protons in GLE events are determined through velocity dispersion and the initial observation on neutron monitors, allowing for the dependence of the length of Sun‒Earth magnetic lines on the velocity of the solar wind.</p>

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Comparing Data on the Times of Solar Proton Release in Solar Proton Events, Obtained in Different Ways

  • 期刊论文

  • 发表日期：

    2025年6月1日

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  • Yu. P. Ochelkov

摘要

Abstract

Times of the release of solar unrelativistic protons, determined from the scale invariance of temporal profiles of solar proton events, are compared to results from studies in which the times of release for solar relativistic protons in GLE events are determined through velocity dispersion and the initial observation on neutron monitors, allowing for the dependence of the length of Sun‒Earth magnetic lines on the velocity of the solar wind.