Superposed epoch study of ICME sub-structures near Earth and their effects on Galactic cosmic rays
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F16%3A00547971" target="_blank" >RIV/68378271:_____/16:00547971 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/201628571" target="_blank" >https://doi.org/10.1051/0004-6361/201628571</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201628571" target="_blank" >10.1051/0004-6361/201628571</a>
Alternative languages
Result language
angličtina
Original language name
Superposed epoch study of ICME sub-structures near Earth and their effects on Galactic cosmic rays
Original language description
Interplanetary coronal mass ejections (ICMEs) are the interplanetary manifestations of solar eruptions. The overtaken solar wind forms a sheath of compressed plasma at the front of ICMEs. Magnetic clouds (MCs) are a subset of ICMEs with specific properties (e. g. the presence of a flux rope). When ICMEs pass near Earth, ground observations indicate that the flux of Galactic cosmic rays (GCRs) decreases. The main aims of this paper are to find common plasma and magnetic properties of different ICME sub-structures and which ICME properties affect the flux of GCRs near Earth.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10303 - Particles and field physics
Result continuities
Project
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Continuities
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Others
Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy & Astrophysics
ISSN
0004-6361
e-ISSN
1432-0746
Volume of the periodical
592
Issue of the periodical within the volume
August
Country of publishing house
FR - FRANCE
Number of pages
13
Pages from-to
A118
UT code for WoS article
000384722600134
EID of the result in the Scopus database
2-s2.0-84981717802