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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F12%3A10130873%21RIV13-GA0-11320___
rdf:type
skos:Concept n16:Vysledek
rdfs:seeAlso
http://dx.doi.org/10.1029/2012GL052636
dcterms:description
We present a case study of a large deformation of the magnetopause on November 26, 2008. The investigation is based on observations of five THEMIS spacecraft located at the dawn flank in the magnetosphere and magnetosheath, on Cluster measurements at the dusk magnetosheath, and is supported by ACE solar wind monitoring. The main revelation of our study is that the interaction of the IMF discontinuity with the bow shock creates either one very elongated hot flow anomaly (HFA) or a pair of them that is (are) simultaneously observed at both flanks. Whereas the dusk HFA is weak and does not cause observable deformation of the magnetopause, the pressure variations connected with the dawn HFA lead to a magnetopause displacement by approximate to 5 R-E outward from its nominal position. This is followed by a rapid inward motion of the magnetopause approximate to 4 R-E inward with respect to the model location. The surface deformation is so large that the outermost THEMIS spacecraft was in the magnetosphere, whereas the spacecraft located 9 R-E inbound entered into the magnetosheath at the same time. The whole event lasted about 5 minutes. Citation: Safrankova, J., O. Goncharov, Z. Nemecek, L. Prech, and D. G. Sibeck (2012), Asymmetric magnetosphere deformation driven by hot flow anomaly(ies), Geophys. Res. Lett., 39, L15107, doi:10.1029/2012GL052636. We present a case study of a large deformation of the magnetopause on November 26, 2008. The investigation is based on observations of five THEMIS spacecraft located at the dawn flank in the magnetosphere and magnetosheath, on Cluster measurements at the dusk magnetosheath, and is supported by ACE solar wind monitoring. The main revelation of our study is that the interaction of the IMF discontinuity with the bow shock creates either one very elongated hot flow anomaly (HFA) or a pair of them that is (are) simultaneously observed at both flanks. Whereas the dusk HFA is weak and does not cause observable deformation of the magnetopause, the pressure variations connected with the dawn HFA lead to a magnetopause displacement by approximate to 5 R-E outward from its nominal position. This is followed by a rapid inward motion of the magnetopause approximate to 4 R-E inward with respect to the model location. The surface deformation is so large that the outermost THEMIS spacecraft was in the magnetosphere, whereas the spacecraft located 9 R-E inbound entered into the magnetosheath at the same time. The whole event lasted about 5 minutes. Citation: Safrankova, J., O. Goncharov, Z. Nemecek, L. Prech, and D. G. Sibeck (2012), Asymmetric magnetosphere deformation driven by hot flow anomaly(ies), Geophys. Res. Lett., 39, L15107, doi:10.1029/2012GL052636.
dcterms:title
Asymmetric magnetosphere deformation driven by hot flow anomaly(ies) Asymmetric magnetosphere deformation driven by hot flow anomaly(ies)
skos:prefLabel
Asymmetric magnetosphere deformation driven by hot flow anomaly(ies) Asymmetric magnetosphere deformation driven by hot flow anomaly(ies)
skos:notation
RIV/00216208:11320/12:10130873!RIV13-GA0-11320___
n16:predkladatel
n21:orjk%3A11320
n3:aktivita
n4:Z n4:S n4:P
n3:aktivity
P(GA205/09/0112), P(ME09056), S, Z(MSM0021620860)
n3:cisloPeriodika
15
n3:dodaniDat
n9:2013
n3:domaciTvurceVysledku
n11:3178129 n11:5876265 Goncharov, Oleksandr n11:1504126
n3:druhVysledku
n17:J
n3:duvernostUdaju
n19:S
n3:entitaPredkladatele
n8:predkladatel
n3:idSjednocenehoVysledku
123955
n3:idVysledku
RIV/00216208:11320/12:10130873
n3:jazykVysledku
n10:eng
n3:klicovaSlova
magnetosheath; anomalies; tangential discontinuity; earths bow shock
n3:klicoveSlovo
n7:earths%20bow%20shock n7:magnetosheath n7:tangential%20discontinuity n7:anomalies
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[C00B5622C05A]
n3:nazevZdroje
Geophysical Research Letteres
n3:obor
n13:BL
n3:pocetDomacichTvurcuVysledku
4
n3:pocetTvurcuVysledku
5
n3:projekt
n14:ME09056 n14:GA205%2F09%2F0112
n3:rokUplatneniVysledku
n9:2012
n3:svazekPeriodika
39
n3:tvurceVysledku
Sibeck, D. G. Goncharov, Oleksandr Šafránková, Jana Přech, Lubomír Němeček, Zdeněk
n3:wos
000307742200006
n3:zamer
n15:MSM0021620860
s:issn
0094-8276
s:numberOfPages
6
n22:doi
10.1029/2012GL052636
n18:organizacniJednotka
11320