Searching for Sources of Solar Cosmic Rays in Weak Events

被引：0

作者：

Bazilevskaya G.A. ^{[1
]}

Daibog E.I. ^{[2
]}

Logachev Y.I. ^{[2
]}

机构：

[1] Lebedev Physical Institute, Russian Academy of Sciences, Moscow

[2] Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow

来源：

Bulletin of the Russian Academy of Sciences: Physics | 2023年 / 87卷 / 07期

关键词：

27;

D O I：

10.3103/S1062873823702787

中图分类号：

学科分类号：

摘要：

Abstract: Some of the weak solar proton events in which protons with energies E ≥ 10 MeV are registered by observers on the Earth are particles accelerated by shock waves in interplanetary space. They can be associated with flares and coronal mass ejections tens of hours before an observed increase in proton fluxes that inject particles into the process of subsequent acceleration in interplanetary space. © 2023, Allerton Press, Inc.

引用

页码：935 / 937

页数：2

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