太阳周期的主要阶段在银河系宇宙射线强度

M. Krainev
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引用次数: 2

摘要

[1]在银河系宇宙射线强度的调制中,太阳周期的分离被考虑为四个主要阶段(最小、上升、最大和下降)。我们论证了这种分类的优点,选择了已知的一种分类作为其出发点,并讨论了太阳周期主要阶段在日球层的特殊性和宇宙射线特征。提出了对寻求分类的物理意义的初步假设。简要讨论了极局部星际介质在日球层形成太阳周期中的作用。索引项:7536太阳物理学,天体物理学和天文学:太阳活动周期;2104行星际物理学:宇宙射线;2134行星际物理:行星际磁场;关键词:银河宇宙射线;非常局部的星际介质;宇宙射线调制的相位。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Main phases of the solar cycle in the galactic cosmic ray intensity
[1] The separation of the solar cycle in the modulation of the galactic cosmic ray intensity into the four main phases (the minimum, ascending, maximum, and descending) is considered. We substantiate advantages of such classification, choose as its initial point one of the known classifications, and discuss the special features of the main phases of the solar cycle in the heliospheric and cosmic ray characteristics. The initial assumption on the physical meaning of the sought for classification is proposed. The role of the very local interstellar medium in forming the solar cycle in the heliosphere is briefly discussed. INDEX TERMS: 7536 Solar Physics, Astrophysics, and Astronomy: Solar activity cycle; 2104 Interplanetary Physics: Cosmic rays; 2134 Interplanetary Physics: Interplanetary magnetic fields; KEYWORDS: Galactic cosmic ray; Very local interstellar medium; Phases of cosmic ray modulation.
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