1998年5月2日和6日GLE期间宇宙射线的俯仰角各向异性和微分刚度谱

A. Lukovnikova, V. Sdobnov
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引用次数: 0

摘要

利用世界中子监测网(39个站点)的数据和全球光谱测量方法,研究了1998年5月2日和6日地面增强期间宇宙射线的俯仰角各向异性和差分刚度谱。我们获得了这些事件中太阳宇宙射线的微分刚性谱,并确定了质子加速到的最大刚度。5月2日地面增强过程中加速质子的最大刚度为~2.4;5月6日,~1.8 GV。所揭示的双向俯仰角各向异性表明,在这些事件中地球处于IMF环结构。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Pitch-angle anisotropy and differential rigidity spectra of cosmic rays during GLE on May 2 and 6, 1998
Using data from the worldwide network of neutron monitors (39 stations) and the method of global spectrographic survey, we have studied pitch-angle anisotropy and differential rigidity spectra of cosmic rays during the ground level enhancements on May 2 and 6, 1998. We obtained differential rigidity spectra of solar cosmic rays in these events and determined the maximum rigidities to which protons accelerated. The maximum rigidities of accelerated protons during the ground level enhancements on May 2 was ~2.4; on May 6, ~1.8 GV. The revealed bidirectional pitch-angle anisotropy indicates that Earth was in the IMF loop structure during these events.
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