Abstract

Detection of cosmic ray fluxes makes it possible to study dynamics of the interplanetary magnetic field and gain information about processes that occur both on the solar surface and in the entire Solar system. The main variations in the cosmic ray intensity are 27-day variations and Forbush effects. These variations are caused by complex spatial solar-plasma formations resulting from various processes on the solar surface and propagating in space with widely varying velocities. The data recorded by the PAMELA magnetic spectrometer on board the Resurs-DK1 satellite in 2006–2016 are used.

中文翻译：

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宇宙射线通量的短期变化的起源

摘要

探测宇宙射线通量可以研究行星际磁场的动力学，并获得有关在太阳表面和整个太阳系中发生的过程的信息。宇宙射线强度的主要变化是27天变化和Forbush效应。这些变化是由复杂的空间太阳等离子形成所引起的，这些复杂的空间是由太阳表面上的各种过程导致的，并且在空间中以不同的速度传播。使用了Resurs-DK1卫星上的PAMELA磁谱仪在2006–2016年记录的数据。