About: Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks     Goto   Sponge   NotDistinct   Permalink

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  • 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. (en)
Title
  • Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks
  • Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks (en)
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  • Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks
  • Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks (en)
skos:notation
  • RIV/00216208:11320/13:10191776!RIV14-GA0-11320___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(GA205/09/0112), P(GAP209/12/1774), S, Z(MSM0021620860)
http://linked.open...iv/cisloPeriodika
  • 16
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 81194
http://linked.open...ai/riv/idVysledku
  • RIV/00216208:11320/13:10191776
http://linked.open...riv/jazykVysledku
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  • ion scale; interplanetary shock; solar wind (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [BCF6F9D6BE7C]
http://linked.open...i/riv/nazevZdroje
  • Geophysical Research Letters
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 40
http://linked.open...iv/tvurceVysledku
  • Němeček, Zdeněk
  • Přech, Lubomír
  • Šafránková, Jana
  • Goncharov, Oleksandr
  • Zastenker, G. N.
http://linked.open...ain/vavai/riv/wos
  • 000324529000002
http://linked.open...n/vavai/riv/zamer
issn
  • 0094-8276
number of pages
http://bibframe.org/vocab/doi
  • 10.1002/grl.50814
http://localhost/t...ganizacniJednotka
  • 11320
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