Precursory signals of Forbush decreases with and without shock wave

D. Lingri, H. Mavromichalaki, A. Belov, E. Eroshenko
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引用次数: 0

Abstract

Many previous studies have shown that before the beginning of a Forbush Decrease (FD) of the cosmic ray intensity, a precursor signal can be observed. All these surveys were focused on FDs that are associated with a sudden storm com- mencement (SSC). In this work we demonstrate that precursors could also be observed in events without a SSC that is determined by an abrupt increase of the interplanetary magnetic field. The type of precursory signals and their diversity among the events are the main purpose of this study. We try to figure out similarities and differences on the signals and the associated events from both categories in the last fifty years, from 1969 to 2019, using the same selection criteria of the under investigation FDs. Simultaneously the orientation of the upcoming solar disturbances in comparison to the way they configure the increase of the interplanetary magnetic field and create these signals are discussed.
在有激波和没有激波的情况下,Forbush的前兆信号减小
许多先前的研究表明,在宇宙射线强度的福布什衰减(FD)开始之前,可以观察到一个前兆信号。所有这些调查都集中在与突然风暴形成(SSC)有关的FDs上。在这项工作中,我们证明在没有SSC的事件中也可以观察到前体,这是由行星际磁场的突然增加决定的。前兆信号的类型及其在事件中的多样性是本研究的主要目的。我们试图用相同的被调查fd的选择标准,找出1969年至2019年近50年来这两个类别的信号和相关事件的异同。同时讨论了即将到来的太阳扰动的方向,以及它们如何配置行星际磁场的增加和产生这些信号。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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