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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F12%3A10130643%21RIV13-GA0-11320___
rdf:type
n8:Vysledek skos:Concept
rdfs:seeAlso
http://dx.doi.org/10.1029/2011JA017252
dcterms:description
The present empirical models describing a location and shape of the magnetopause and bow shock are based on a statistical evaluation of magnetopause and bow shock crossings. The crossings are usually identified by a visual inspection of the plots or by automatic methods which are less reliable. We present a new method of determination of the most probable boundary locations. The method is based on continuous plasma and magnetic field measurements in the regions visited by a sounding spacecraft (the solar wind, magnetosheath, and magnetosphere) and on the determination of ratios of these parameters to simultaneously monitored upstream parameters. The regions identified by this method are then used for development of simple models of the magnetopause and bow shock locations parameterized by the upstream pressure. The performance of the models is tested with corresponding boundary crossings based mainly on the THEMIS observations. Both developed models are in a good agreement with the results obtained from identification of crossings. The present empirical models describing a location and shape of the magnetopause and bow shock are based on a statistical evaluation of magnetopause and bow shock crossings. The crossings are usually identified by a visual inspection of the plots or by automatic methods which are less reliable. We present a new method of determination of the most probable boundary locations. The method is based on continuous plasma and magnetic field measurements in the regions visited by a sounding spacecraft (the solar wind, magnetosheath, and magnetosphere) and on the determination of ratios of these parameters to simultaneously monitored upstream parameters. The regions identified by this method are then used for development of simple models of the magnetopause and bow shock locations parameterized by the upstream pressure. The performance of the models is tested with corresponding boundary crossings based mainly on the THEMIS observations. Both developed models are in a good agreement with the results obtained from identification of crossings.
dcterms:title
A new approach to magnetopause and bow shock modeling based on automated region identification A new approach to magnetopause and bow shock modeling based on automated region identification
skos:prefLabel
A new approach to magnetopause and bow shock modeling based on automated region identification A new approach to magnetopause and bow shock modeling based on automated region identification
skos:notation
RIV/00216208:11320/12:10130643!RIV13-GA0-11320___
n8:predkladatel
n9:orjk%3A11320
n3:aktivita
n4:Z n4:S n4:P
n3:aktivity
P(GA205/09/0112), P(GA205/09/0170), S, Z(MSM0021620860)
n3:cisloPeriodika
A05
n3:dodaniDat
n11:2013
n3:domaciTvurceVysledku
n16:7237871 n16:5876265 n16:1504126
n3:druhVysledku
n15:J
n3:duvernostUdaju
n21:S
n3:entitaPredkladatele
n6:predkladatel
n3:idSjednocenehoVysledku
120345
n3:idVysledku
RIV/00216208:11320/12:10130643
n3:jazykVysledku
n14:eng
n3:klicovaSlova
size; interball; dependence; location; shape; magnetic-field; solar-wind control; high-latitude magnetopause
n3:klicoveSlovo
n5:high-latitude%20magnetopause n5:size n5:dependence n5:magnetic-field n5:interball n5:solar-wind%20control n5:shape n5:location
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[6DB5E70138AF]
n3:nazevZdroje
Journal of Geophysical Research
n3:obor
n7:BL
n3:pocetDomacichTvurcuVysledku
3
n3:pocetTvurcuVysledku
3
n3:projekt
n20:GA205%2F09%2F0112 n20:GA205%2F09%2F0170
n3:rokUplatneniVysledku
n11:2012
n3:svazekPeriodika
117
n3:tvurceVysledku
Jelínek, Karel Šafránková, Jana Němeček, Zdeněk
n3:wos
000303672100003
n3:zamer
n19:MSM0021620860
s:issn
0148-0227
s:numberOfPages
8
n10:doi
10.1029/2011JA017252
n18:organizacniJednotka
11320