This HTML5 document contains 57 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
dctermshttp://purl.org/dc/terms/
n20http://localhost/temp/predkladatel/
n11http://linked.opendata.cz/resource/domain/vavai/projekt/
n5http://linked.opendata.cz/resource/domain/vavai/riv/tvurce/
n10http://linked.opendata.cz/resource/domain/vavai/subjekt/
n9http://linked.opendata.cz/ontology/domain/vavai/
n21http://linked.opendata.cz/resource/domain/vavai/zamer/
shttp://schema.org/
skoshttp://www.w3.org/2004/02/skos/core#
rdfshttp://www.w3.org/2000/01/rdf-schema#
n3http://linked.opendata.cz/ontology/domain/vavai/riv/
n14http://bibframe.org/vocab/
n22http://linked.opendata.cz/resource/domain/vavai/vysledek/RIV%2F00216208%3A11320%2F12%3A10130673%21RIV13-GA0-11320___/
n2http://linked.opendata.cz/resource/domain/vavai/vysledek/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n12http://linked.opendata.cz/ontology/domain/vavai/riv/klicoveSlovo/
n4http://linked.opendata.cz/ontology/domain/vavai/riv/duvernostUdaju/
xsdhhttp://www.w3.org/2001/XMLSchema#
n18http://linked.opendata.cz/ontology/domain/vavai/riv/jazykVysledku/
n15http://linked.opendata.cz/ontology/domain/vavai/riv/aktivita/
n13http://linked.opendata.cz/ontology/domain/vavai/riv/druhVysledku/
n8http://linked.opendata.cz/ontology/domain/vavai/riv/obor/
n7http://reference.data.gov.uk/id/gregorian-year/

Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F12%3A10130673%21RIV13-GA0-11320___
rdf:type
n9:Vysledek skos:Concept
rdfs:seeAlso
http://dx.doi.org/10.1029/2011JA017429
dcterms:description
This paper analyzes the distribution of different pressure components (dynamic, thermal, magnetic) in the magnetosheath along the Sun-Earth line for northward and radial interplanetary magnetic field (IMF) orientations with motivation to explain an unusual location and shape of the magnetopause often observed during the intervals of the radial IMF. The analysis employs isotropic and anisotropic MHD models, and their results are compared with the statistical processing of THEMIS observations. We have found that (1) the temperature anisotropy in the magnetosheath controls the pressure distribution near the magnetopause, and (2) the total pressure exerted on the subsolar magnetopause depends on the IMF orientation being significantly lower than the solar wind dynamic pressure for the radial IMF. The results of both MHD simulations and statistical investigations are quantitatively consistent with already published observations of the average magnetopause location as a function of the IMF orientation. This paper analyzes the distribution of different pressure components (dynamic, thermal, magnetic) in the magnetosheath along the Sun-Earth line for northward and radial interplanetary magnetic field (IMF) orientations with motivation to explain an unusual location and shape of the magnetopause often observed during the intervals of the radial IMF. The analysis employs isotropic and anisotropic MHD models, and their results are compared with the statistical processing of THEMIS observations. We have found that (1) the temperature anisotropy in the magnetosheath controls the pressure distribution near the magnetopause, and (2) the total pressure exerted on the subsolar magnetopause depends on the IMF orientation being significantly lower than the solar wind dynamic pressure for the radial IMF. The results of both MHD simulations and statistical investigations are quantitatively consistent with already published observations of the average magnetopause location as a function of the IMF orientation.
dcterms:title
Why does the subsolar magnetopause move sunward for radial interplanetary magnetic field? Why does the subsolar magnetopause move sunward for radial interplanetary magnetic field?
skos:prefLabel
Why does the subsolar magnetopause move sunward for radial interplanetary magnetic field? Why does the subsolar magnetopause move sunward for radial interplanetary magnetic field?
skos:notation
RIV/00216208:11320/12:10130673!RIV13-GA0-11320___
n9:predkladatel
n10:orjk%3A11320
n3:aktivita
n15:S n15:P n15:Z
n3:aktivity
P(GA205/09/0112), P(ME09106), S, Z(MSM0021620860)
n3:cisloPeriodika
A05
n3:dodaniDat
n7:2013
n3:domaciTvurceVysledku
n5:5876265 n5:1504126 n5:7237871
n3:druhVysledku
n13:J
n3:duvernostUdaju
n4:S
n3:entitaPredkladatele
n22:predkladatel
n3:idSjednocenehoVysledku
180968
n3:idVysledku
RIV/00216208:11320/12:10130673
n3:jazykVysledku
n18:eng
n3:klicovaSlova
flow; one-fluid; cluster data; mhd simulations; ulf fluctuations; magnetosheath region; dayside magnetosphere; solar-wind; proton temperature anisotropy; earths bow shock
n3:klicoveSlovo
n12:one-fluid n12:ulf%20fluctuations n12:mhd%20simulations n12:cluster%20data n12:magnetosheath%20region n12:earths%20bow%20shock n12:solar-wind n12:dayside%20magnetosphere n12:proton%20temperature%20anisotropy n12:flow
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[4B0BD474CA36]
n3:nazevZdroje
Journal of Geophysical Research
n3:obor
n8:BL
n3:pocetDomacichTvurcuVysledku
3
n3:pocetTvurcuVysledku
4
n3:projekt
n11:ME09106 n11:GA205%2F09%2F0112
n3:rokUplatneniVysledku
n7:2012
n3:svazekPeriodika
117
n3:tvurceVysledku
Šafránková, Jana Samsonov, A. A. Jelínek, Karel Němeček, Zdeněk
n3:wos
000304014300001
n3:zamer
n21:MSM0021620860
s:issn
0148-0227
s:numberOfPages
13
n14:doi
10.1029/2011JA017429
n20:organizacniJednotka
11320