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...
Main Author: | |
---|---|
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 |
id |
doaj-f736e154bdf3437698996dcdb74a5acd |
---|---|
record_format |
Article |
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 |
work_keys_str_mv |
AT aiklyuyeva theinteractionofthegalacticcosmicrayswiththehighspeedsolarwindstreams AT aiklyuyeva interactionofthegalacticcosmicrayswiththehighspeedsolarwindstreams |
_version_ |
1725925260220432384 |