The interaction of the galactic cosmic rays with the high-speed solar wind streams

Based on statistical and comparative analysis of neutron monitor data from 1995 to 2013 years the influence of recurrent and sporadic high-speed streams of solar wind on the intensity of the galactic cosmic rays near Earth orbit was studied. Both types of high-speed solar wind streams modulate the g...

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Main Author: A. I. Klyuyeva
Format: Article
Language:English
Published: National Aviation University 2014-12-01
Series:Вісник Астрономічної школи
Subjects:
Online Access:http://astro.nau.edu.ua/issues/2014_V.10_Iss.2/Klyuyeva.html
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spelling doaj-f736e154bdf3437698996dcdb74a5acd2020-11-24T21:40:40ZengNational Aviation UniversityВісник Астрономічної школи1607-28552411-66022014-12-0110213614010.18372/2411-6602.10.21362411-6602.10.2136The interaction of the galactic cosmic rays with the high-speed solar wind streamsA. I. Klyuyeva0Main Astronomical Observatory NAS of UkraineBased on statistical and comparative analysis of neutron monitor data from 1995 to 2013 years the influence of recurrent and sporadic high-speed streams of solar wind on the intensity of the galactic cosmic rays near Earth orbit was studied. Both types of high-speed solar wind streams modulate the galactic cosmic rays flux and cause Forbush decreases of different nature. The main parameters of Forbush decreases such as typical shape, magnitude, duration of decrease, delay, size of modulation area etc was studied.http://astro.nau.edu.ua/issues/2014_V.10_Iss.2/Klyuyeva.htmlForbush-effectForbush-decreasesporadic and recurrent high-speed streamssolar windcoronal holes
collection DOAJ
language English
format Article
sources DOAJ
author A. I. Klyuyeva
spellingShingle A. I. Klyuyeva
The interaction of the galactic cosmic rays with the high-speed solar wind streams
Вісник Астрономічної школи
Forbush-effect
Forbush-decrease
sporadic and recurrent high-speed streams
solar wind
coronal holes
author_facet A. I. Klyuyeva
author_sort A. I. Klyuyeva
title The interaction of the galactic cosmic rays with the high-speed solar wind streams
title_short The interaction of the galactic cosmic rays with the high-speed solar wind streams
title_full The interaction of the galactic cosmic rays with the high-speed solar wind streams
title_fullStr The interaction of the galactic cosmic rays with the high-speed solar wind streams
title_full_unstemmed The interaction of the galactic cosmic rays with the high-speed solar wind streams
title_sort interaction of the galactic cosmic rays with the high-speed solar wind streams
publisher National Aviation University
series Вісник Астрономічної школи
issn 1607-2855
2411-6602
publishDate 2014-12-01
description Based on statistical and comparative analysis of neutron monitor data from 1995 to 2013 years the influence of recurrent and sporadic high-speed streams of solar wind on the intensity of the galactic cosmic rays near Earth orbit was studied. Both types of high-speed solar wind streams modulate the galactic cosmic rays flux and cause Forbush decreases of different nature. The main parameters of Forbush decreases such as typical shape, magnitude, duration of decrease, delay, size of modulation area etc was studied.
topic Forbush-effect
Forbush-decrease
sporadic and recurrent high-speed streams
solar wind
coronal holes
url http://astro.nau.edu.ua/issues/2014_V.10_Iss.2/Klyuyeva.html
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