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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F11%3A10109842%21RIV12-GA0-11320___
rdf:type
n5:Vysledek skos:Concept
rdfs:seeAlso
http://www.mff.cuni.cz/veda/konference/wds/proc/pdf11/WDS11_203_f2_Goncharov.pdf
dcterms:description
Propagation of interplanetary discontinuities through the interplanetary space, their modification in the foreshock and interaction with the bow shock and magnetopause are key problem of the Space Weather Program because they are often connected with strong geomagnetic disturbances. We are presenting a comprehensive analysis of the propagation of two moderate IP shocks in the solar wind and through the magnetosphere. In both cases, the shock is observed by four spacecraft in the solar wind and by ten spacecraft in the different magnetospheric regions, which allows us to follow the evolution of the original shock and its transformation to geomagnetic disturbances and finally to trace these disturbances into the magnetotail. We found the influence of the foreshock and Bow shock on the propagation of the IP shock to the magnetotail. Propagation of interplanetary discontinuities through the interplanetary space, their modification in the foreshock and interaction with the bow shock and magnetopause are key problem of the Space Weather Program because they are often connected with strong geomagnetic disturbances. We are presenting a comprehensive analysis of the propagation of two moderate IP shocks in the solar wind and through the magnetosphere. In both cases, the shock is observed by four spacecraft in the solar wind and by ten spacecraft in the different magnetospheric regions, which allows us to follow the evolution of the original shock and its transformation to geomagnetic disturbances and finally to trace these disturbances into the magnetotail. We found the influence of the foreshock and Bow shock on the propagation of the IP shock to the magnetotail.
dcterms:title
Interplanetary Shock Propagation Through the Magnetosphere to the Magnetotail Interplanetary Shock Propagation Through the Magnetosphere to the Magnetotail
skos:prefLabel
Interplanetary Shock Propagation Through the Magnetosphere to the Magnetotail Interplanetary Shock Propagation Through the Magnetosphere to the Magnetotail
skos:notation
RIV/00216208:11320/11:10109842!RIV12-GA0-11320___
n5:predkladatel
n15:orjk%3A11320
n3:aktivita
n13:Z n13:S n13:P
n3:aktivity
P(GA205/09/0170), S, Z(MSM0021620860)
n3:dodaniDat
n11:2012
n3:domaciTvurceVysledku
n4:1504126 Goncharov, Oleksandr Grygorov, Kostiantyn n4:5876265 n4:3178129
n3:druhVysledku
n23:D
n3:duvernostUdaju
n7:S
n3:entitaPredkladatele
n16:predkladatel
n3:idSjednocenehoVysledku
205478
n3:idVysledku
RIV/00216208:11320/11:10109842
n3:jazykVysledku
n20:eng
n3:klicovaSlova
Magnetotail; Magnetosphere; Interplanetary shock
n3:klicoveSlovo
n14:Magnetosphere n14:Interplanetary%20shock n14:Magnetotail
n3:kontrolniKodProRIV
[790AE8061326]
n3:mistoKonaniAkce
Praha
n3:mistoVydani
Praha
n3:nazevZdroje
WDS'11 Proceedings of Contributed Papers: Part II – Physics of Plasmas and Ionized Media
n3:obor
n9:BL
n3:pocetDomacichTvurcuVysledku
5
n3:pocetTvurcuVysledku
5
n3:projekt
n24:GA205%2F09%2F0170
n3:rokUplatneniVysledku
n11:2011
n3:tvurceVysledku
Goncharov, Oleksandr Šafránková, Jana Grygorov, Kostiantyn Němeček, Zdeněk Přech, Lubomír
n3:typAkce
n17:EUR
n3:zahajeniAkce
2011-05-31+02:00
n3:zamer
n22:MSM0021620860
s:numberOfPages
8
n8:hasPublisher
Matfyzpress
n21:isbn
978-80-7378-185-9
n18:organizacniJednotka
11320