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  • In this paper we study the evolution of the expanding solar wind plasma using a one-dimensional and a two-dimensional expanding box model (Grappin et al, 1993) implemented here within a hybrid code (Liewer et al, 2001). We first consider a plasma with protons and 5 % of alpha particles, without drift between the protons and alphas, considering successively the low-beta and high-beta cases. Then we consider a strong drift between protons and alphas, again separately the low-beta and high-beta case. Without drift, the evolution of the low-beta plasma is adiabatic. In the high-beta plasma without drift, the fire hose instabilites (both parallel and oblique) disrupt the adiabatic evolution. Finally, with a drift, the adiabatic evolution is stopped by the oblique Alfv'en instability and the parallel magnetosonic instability for low-beta plasma and for high-beta plasma, respectively. The two instabilities slow down the alphas and heat alphas and protons.
  • In this paper we study the evolution of the expanding solar wind plasma using a one-dimensional and a two-dimensional expanding box model (Grappin et al, 1993) implemented here within a hybrid code (Liewer et al, 2001). We first consider a plasma with protons and 5 % of alpha particles, without drift between the protons and alphas, considering successively the low-beta and high-beta cases. Then we consider a strong drift between protons and alphas, again separately the low-beta and high-beta case. Without drift, the evolution of the low-beta plasma is adiabatic. In the high-beta plasma without drift, the fire hose instabilites (both parallel and oblique) disrupt the adiabatic evolution. Finally, with a drift, the adiabatic evolution is stopped by the oblique Alfv'en instability and the parallel magnetosonic instability for low-beta plasma and for high-beta plasma, respectively. The two instabilities slow down the alphas and heat alphas and protons. (en)
Title
  • Hybrid simulations of the expanding solar wind: Temperatures and drift velocities.
  • Hybrid simulations of the expanding solar wind: Temperatures and drift velocities. (en)
skos:prefLabel
  • Hybrid simulations of the expanding solar wind: Temperatures and drift velocities.
  • Hybrid simulations of the expanding solar wind: Temperatures and drift velocities. (en)
skos:notation
  • RIV/68378289:_____/03:04033538!RIV/2004/AV0/A04004/N
http://linked.open.../vavai/riv/strany
  • 15;1-15-4
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(IAB3042106), Z(AV0Z3042911)
http://linked.open...iv/cisloPeriodika
  • 5
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
  • 609488
http://linked.open...ai/riv/idVysledku
  • RIV/68378289:_____/03:04033538
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • expanding solar wind; hybrid simulations (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [E39F8A0EF974]
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...ocetUcastnikuAkce
http://linked.open...nichUcastnikuAkce
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 30
http://linked.open...iv/tvurceVysledku
  • Trávníček, Pavel
  • Hellinger, Petr
  • Mangeney, A.
  • Grappin, R.
http://linked.open...n/vavai/riv/zamer
issn
  • 0094-8276
number of pages
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