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Statements

Subject Item
n2:RIV%2F68378289%3A_____%2F09%3A00338070%21RIV10-AV0-68378289
rdf:type
n12:Vysledek skos:Concept
dcterms:description
In the present statistical study, we discuss a probability of simultaneous observations of the same sign of the magnetic field BZ component in the solar wind and magnetosheath. The analysis is based on 5 min data from four spacecraft (Interball-1, IMP 8, Cluster, and THEMIS) operating in different phases of the solar cycle in themagnetosheath. Their measurements are compared with Wind interplanetary magnetic field (IMF) observations, and other available upstream monitors (ACE, THEMIS B, and OMNI database) are tested for some sets. We can conclude that the probability of observations of the same BZ sign in the solar wind and in the magnetosheath is surprisingly very low from a general point of view. The probability changes through the solar cycle, being larger at the solar minimum. Regardless of the solar cycle phase, this probability is close to 0.5 (random coincidence) for IMF |BZ|<1 nT, and it is a rising function of the BZ value. In the present statistical study, we discuss a probability of simultaneous observations of the same sign of the magnetic field BZ component in the solar wind and magnetosheath. The analysis is based on 5 min data from four spacecraft (Interball-1, IMP 8, Cluster, and THEMIS) operating in different phases of the solar cycle in themagnetosheath. Their measurements are compared with Wind interplanetary magnetic field (IMF) observations, and other available upstream monitors (ACE, THEMIS B, and OMNI database) are tested for some sets. We can conclude that the probability of observations of the same BZ sign in the solar wind and in the magnetosheath is surprisingly very low from a general point of view. The probability changes through the solar cycle, being larger at the solar minimum. Regardless of the solar cycle phase, this probability is close to 0.5 (random coincidence) for IMF |BZ|<1 nT, and it is a rising function of the BZ value.
dcterms:title
Reliability of prediction of the magnetosheath Bz component from interplanetary magnetic field observations Reliability of prediction of the magnetosheath Bz component from interplanetary magnetic field observations
skos:prefLabel
Reliability of prediction of the magnetosheath Bz component from interplanetary magnetic field observations Reliability of prediction of the magnetosheath Bz component from interplanetary magnetic field observations
skos:notation
RIV/68378289:_____/09:00338070!RIV10-AV0-68378289
n3:aktivita
n4:S n4:P n4:Z
n3:aktivity
P(GA205/09/0112), P(GA205/09/0170), S, Z(AV0Z30420517), Z(MSM0021620860)
n3:cisloPeriodika
-
n3:dodaniDat
n14:2010
n3:domaciTvurceVysledku
Hayosh, Mykhaylo
n3:druhVysledku
n17:J
n3:duvernostUdaju
n6:S
n3:entitaPredkladatele
n5:predkladatel
n3:idSjednocenehoVysledku
338849
n3:idVysledku
RIV/68378289:_____/09:00338070
n3:jazykVysledku
n15:eng
n3:klicovaSlova
IMF; magnetosheath
n3:klicoveSlovo
n9:magnetosheath n9:IMF
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[A7C441041B03]
n3:nazevZdroje
Journal of Geophysical Research
n3:obor
n16:BL
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
5
n3:projekt
n11:GA205%2F09%2F0112 n11:GA205%2F09%2F0170
n3:rokUplatneniVysledku
n14:2009
n3:svazekPeriodika
114
n3:tvurceVysledku
Hayosh, Mykhaylo Přech, L. Gutynska, O. Němeček, Z. Šafránková, J.
n3:wos
000272946900003
n3:zamer
n13:AV0Z30420517 n13:MSM0021620860
s:issn
0148-0227
s:numberOfPages
7