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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F13%3A10191871%21RIV14-GA0-11320___
rdf:type
n16:Vysledek skos:Concept
rdfs:seeAlso
http://dx.doi.org/10.1063/1.4811079
dcterms:description
A spacecraft configuration with two monitors near L1 and a fleet of the spacecraft orbiting in front of the bow shock brings a great opportunity to test the propagation techniques for the solar wind and the assumption on a negligible solar wind parameter evolution. We use multi-point observations of the THEMIS-ARTEMIS mission and compare them with data from the Wind solar wind monitor in order to estimate different factors influencing solar wind speed evolution. We have found a significant deceleration (up to 6%) of the solar wind close to the bow shock and the effect extends up to 30 RE from the Earth. It is controlled by the level of magnetic field fluctuations and by the flux of reflected and accelerated particles. We can conclude that the reflected particles not only excite waves of large amplitudes but also modify mean values of the solar wind speed measured in an unperturbed solar wind. A spacecraft configuration with two monitors near L1 and a fleet of the spacecraft orbiting in front of the bow shock brings a great opportunity to test the propagation techniques for the solar wind and the assumption on a negligible solar wind parameter evolution. We use multi-point observations of the THEMIS-ARTEMIS mission and compare them with data from the Wind solar wind monitor in order to estimate different factors influencing solar wind speed evolution. We have found a significant deceleration (up to 6%) of the solar wind close to the bow shock and the effect extends up to 30 RE from the Earth. It is controlled by the level of magnetic field fluctuations and by the flux of reflected and accelerated particles. We can conclude that the reflected particles not only excite waves of large amplitudes but also modify mean values of the solar wind speed measured in an unperturbed solar wind.
dcterms:title
Solar Wind Modification Upstream of the Bow Shock Solar Wind Modification Upstream of the Bow Shock
skos:prefLabel
Solar Wind Modification Upstream of the Bow Shock Solar Wind Modification Upstream of the Bow Shock
skos:notation
RIV/00216208:11320/13:10191871!RIV14-GA0-11320___
n16:predkladatel
n25:orjk%3A11320
n3:aktivita
n4:S n4:P n4:Z n4:I
n3:aktivity
I, P(GA205/09/0170), P(GAP209/12/1774), S, Z(MSM0021620860)
n3:dodaniDat
n19:2014
n3:domaciTvurceVysledku
n7:9732675 n7:7237871 n7:5876265 n7:3178129 n7:1504126
n3:druhVysledku
n21:D
n3:duvernostUdaju
n11:S
n3:entitaPredkladatele
n14:predkladatel
n3:idSjednocenehoVysledku
106226
n3:idVysledku
RIV/00216208:11320/13:10191871
n3:jazykVysledku
n24:eng
n3:klicovaSlova
Foreshock; Reflected particles; Interplanetary magnetic field; Solar wind velocity
n3:klicoveSlovo
n17:Reflected%20particles n17:Interplanetary%20magnetic%20field n17:Foreshock n17:Solar%20wind%20velocity
n3:kontrolniKodProRIV
[FFCD624B3AB6]
n3:mistoKonaniAkce
HI
n3:mistoVydani
MELVILLE
n3:nazevZdroje
AIP Conference Proceedings
n3:obor
n18:BL
n3:pocetDomacichTvurcuVysledku
5
n3:pocetTvurcuVysledku
5
n3:projekt
n20:GAP209%2F12%2F1774 n20:GA205%2F09%2F0170
n3:rokUplatneniVysledku
n19:2013
n3:tvurceVysledku
Němeček, Zdeněk Jelínek, Karel Šafránková, Jana Urbář, Jaroslav Přech, Lubomír
n3:typAkce
n8:WRD
n3:wos
000320997100104
n3:zahajeniAkce
2012-05-17+02:00
n3:zamer
n13:MSM0021620860
s:issn
0094-243X
s:numberOfPages
4
n23:doi
10.1063/1.4811079
n9:hasPublisher
AMER INST PHYSICS
n15:isbn
978-0-7354-1163-0
n22:organizacniJednotka
11320