The Forbush-decreases in cosmic ray fluxes and solar-proton events in July and September 2017

IF 0.2 Q4 PHYSICS, MULTIDISCIPLINARY Recent Contributions to Physics Pub Date : 2021-06-01 DOI:10.26577/rcph.2021.v77.i2.02
Ye. A. Tulekov, А.К. Morzabaev, V. Makhmutov
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引用次数: 1

Abstract

The study of the nature of variations in cosmic ray fluxes, including diurnal, 27-day, annual, etc., and the question of the relationship of solar-geophysical factors on the state of the atmosphere attracts special attention of scientists. Coronal mass ejections are the result of solar winds generated on the Sun during a series of flares. At the same time, solar winds provoke variations in the intensity of cosmic rays, which include, in particular, Forbush-decreases. The article presents brief characteristics of the CARPET detector of the scientific cosmophysical complex of the L.N.Gumilyov ENU and experimental data obtained at this facility during the observation of Forbush-deacreases in July and September 2017. The results of the analysis of variations in cosmic ray fluxes are presented and their relationship with the conditions in the interplanetary medium and the Earth’s magnetosphere caused by processes on the Sun is described. It was found that the decrease in cosmic ray fluxes in July and September 2017 was due to high solar activity (a series of solar flares). A comparative analysis of the time changes recorded by the CARPET detector modules of the L.N.Gumilyov ENU scientific complex with the data of the world network of neutron monitors («Apatity», «Almaty» and «Jungfraujoch IGY») is also presented. Data on the electromagnetic environment of interplanetary space during the period of heliospheric and magnetospheric disturbances were also used for the analysis. The analysis showed that the measurement data of the CARPET detector is in good agreement with the data of the above-mentioned neutron monitors of the world network, which allows us to study the physical nature of cosmic ray variations for different time intervals.
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2017年7月和9月,Forbush宇宙射线通量和太阳质子事件减少
研究宇宙射线通量的变化性质,包括日、27日、年等,以及太阳-地球物理因子与大气状态的关系问题,引起了科学家们的特别关注。日冕物质抛射是太阳在一系列耀斑期间产生的太阳风的结果。与此同时,太阳风引起宇宙射线强度的变化,其中特别包括福布什衰减。本文简要介绍了L.N.Gumilyov ENU科学宇宙物理复合物的CARPET探测器的特点,以及该设备在2017年7月和9月观测forbush - deacls期间获得的实验数据。介绍了宇宙射线通量变化的分析结果,并叙述了宇宙射线通量变化与行星际介质和太阳活动引起的地球磁层条件的关系。研究发现,2017年7月和9月宇宙射线通量的减少是由于太阳活动频繁(一系列太阳耀斑)。本文还介绍了古米廖夫科学基地的CARPET探测器模块记录的时间变化与世界中子监测网(“Apatity”、“Almaty”和“Jungfraujoch IGY”)的数据的对比分析。利用日球层和磁层扰动期间行星际空间的电磁环境数据进行分析。分析表明,CARPET探测器的测量数据与上述世界网络中子监测仪的数据吻合较好,这使我们能够研究宇宙射线在不同时间间隔变化的物理性质。
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