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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F11%3A10108220%21RIV12-GA0-11320___
rdf:type
skos:Concept n13:Vysledek
rdfs:seeAlso
http://dx.doi.org/10.1016/j.pss.2011.03.016
dcterms:description
Interplanetary coronal mass ejections (ICMEs) and their subset, magnetic clouds (MCs), are important manifestations of solar activity which have substantial impact on the geomagnetic field. We re-analyze events already identified in Wind and Voyager 2 data and estimate changes of their geometry along the path from the Sun. The analysis is based on the thickness of the sheath between a shock and a particular ICME or MC which is proportional to the apparent curvature radius of ICMEs/MCs. We have found that this apparent radius of curvature increases with the Mach number and this effect is attributed to the larger deformation of the fast ICME/MC. Further, the relative sheath thickness that is proportional to the flux rope oblateness decreases with the magnetic field intensity inside the ICME/MC and increases with the heliospheric distance. Interplanetary coronal mass ejections (ICMEs) and their subset, magnetic clouds (MCs), are important manifestations of solar activity which have substantial impact on the geomagnetic field. We re-analyze events already identified in Wind and Voyager 2 data and estimate changes of their geometry along the path from the Sun. The analysis is based on the thickness of the sheath between a shock and a particular ICME or MC which is proportional to the apparent curvature radius of ICMEs/MCs. We have found that this apparent radius of curvature increases with the Mach number and this effect is attributed to the larger deformation of the fast ICME/MC. Further, the relative sheath thickness that is proportional to the flux rope oblateness decreases with the magnetic field intensity inside the ICME/MC and increases with the heliospheric distance.
dcterms:title
Deformation of ICMEs/MCs along their path Deformation of ICMEs/MCs along their path
skos:prefLabel
Deformation of ICMEs/MCs along their path Deformation of ICMEs/MCs along their path
skos:notation
RIV/00216208:11320/11:10108220!RIV12-GA0-11320___
n13:predkladatel
n22:orjk%3A11320
n3:aktivita
n14:S n14:P n14:Z
n3:aktivity
P(GA205/09/0170), P(ME09056), S, Z(MSM0021620860)
n3:cisloPeriodika
9
n3:dodaniDat
n9:2012
n3:domaciTvurceVysledku
n5:1504126 n5:1526294 n5:5876265
n3:druhVysledku
n16:J
n3:duvernostUdaju
n21:S
n3:entitaPredkladatele
n15:predkladatel
n3:idSjednocenehoVysledku
193141
n3:idVysledku
RIV/00216208:11320/11:10108220
n3:jazykVysledku
n10:eng
n3:klicovaSlova
Interplanetary coronal mass ejections; Deformation
n3:klicoveSlovo
n18:Deformation n18:Interplanetary%20coronal%20mass%20ejections
n3:kodStatuVydavatele
NL - Nizozemsko
n3:kontrolniKodProRIV
[75EB0A8F65B1]
n3:nazevZdroje
Planetary and Space Science
n3:obor
n20:BL
n3:pocetDomacichTvurcuVysledku
3
n3:pocetTvurcuVysledku
4
n3:projekt
n12:ME09056 n12:GA205%2F09%2F0170
n3:rokUplatneniVysledku
n9:2011
n3:svazekPeriodika
59
n3:tvurceVysledku
Němeček, Zdeněk Richardson, J. D. Lynnyk, Andrii Šafránková, Jana
n3:wos
000292722100004
n3:zamer
n19:MSM0021620860
s:issn
0032-0633
s:numberOfPages
8
n4:doi
10.1016/j.pss.2011.03.016
n17:organizacniJednotka
11320