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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F13%3A10191776%21RIV14-GA0-11320___
rdf:type
skos:Concept n16:Vysledek
rdfs:seeAlso
http://dx.doi.org/10.1002/grl.50814
dcterms:description
A formation of low-Mach-number quasi-perpendicular shocks is expected to be well understood. From theoretical considerations as well as from observations, it follows that the shock ramp thickness would scale with the ion inertial length. We present analysis of 12 subcritical or marginally critical interplanetary shocks that reveals that (1) the ion transition scale determined from direct measurements of plasma moments (speed, temperature, and density) are of the same order as the ramp thickness determined from the magnetic field and (2) the ion transition scale is directly proportional to the ion thermal gyroradius, R-th; it was found to be approximate to 3.2R(th) in a broad range of solar wind and shock parameters. These results stress a role of the ion kinetics in the shock formation. A formation of low-Mach-number quasi-perpendicular shocks is expected to be well understood. From theoretical considerations as well as from observations, it follows that the shock ramp thickness would scale with the ion inertial length. We present analysis of 12 subcritical or marginally critical interplanetary shocks that reveals that (1) the ion transition scale determined from direct measurements of plasma moments (speed, temperature, and density) are of the same order as the ramp thickness determined from the magnetic field and (2) the ion transition scale is directly proportional to the ion thermal gyroradius, R-th; it was found to be approximate to 3.2R(th) in a broad range of solar wind and shock parameters. These results stress a role of the ion kinetics in the shock formation.
dcterms:title
Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks
skos:prefLabel
Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks
skos:notation
RIV/00216208:11320/13:10191776!RIV14-GA0-11320___
n16:predkladatel
n17:orjk%3A11320
n4:aktivita
n14:I n14:S n14:P n14:Z
n4:aktivity
I, P(GA205/09/0112), P(GAP209/12/1774), S, Z(MSM0021620860)
n4:cisloPeriodika
16
n4:dodaniDat
n15:2014
n4:domaciTvurceVysledku
n5:3178129 n5:1504126 n5:2926016 n5:5876265
n4:druhVysledku
n13:J
n4:duvernostUdaju
n6:S
n4:entitaPredkladatele
n21:predkladatel
n4:idSjednocenehoVysledku
81194
n4:idVysledku
RIV/00216208:11320/13:10191776
n4:jazykVysledku
n18:eng
n4:klicovaSlova
ion scale; interplanetary shock; solar wind
n4:klicoveSlovo
n11:ion%20scale n11:interplanetary%20shock n11:solar%20wind
n4:kodStatuVydavatele
US - Spojené státy americké
n4:kontrolniKodProRIV
[BCF6F9D6BE7C]
n4:nazevZdroje
Geophysical Research Letters
n4:obor
n9:BL
n4:pocetDomacichTvurcuVysledku
4
n4:pocetTvurcuVysledku
5
n4:projekt
n22:GAP209%2F12%2F1774 n22:GA205%2F09%2F0112
n4:rokUplatneniVysledku
n15:2013
n4:svazekPeriodika
40
n4:tvurceVysledku
Šafránková, Jana Zastenker, G. N. Goncharov, Oleksandr Přech, Lubomír Němeček, Zdeněk
n4:wos
000324529000002
n4:zamer
n8:MSM0021620860
s:issn
0094-8276
s:numberOfPages
5
n20:doi
10.1002/grl.50814
n7:organizacniJednotka
11320