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  • Results of two global three-dimensional hybrid simulations of the solar wind interaction with the Hermean magnetosphere are presented for southward and northward interplanetary magnetic field (IMF) orientations. Important dawn-dusk asymmetries of the Hermean bow shock and magnetosheath are observed depending on the IMF orientation. For the southward IMF, the dawnside has a thicker magnetosheath with higher beta values and slower bulk velocities compared to the duskside, whereas for the northward IMF, the duskside has a thicker and higher beta magnetosheath with slower bulk velocities. Mirror mode activity consequently appears at the dawnside for the southward IMF and at the duskside for the northward IMF. A mechanism for the bow shock and magnetosheath asymmetries is proposed and discussed in the context of the Hermean and terrestrial magnetosheaths.
  • Results of two global three-dimensional hybrid simulations of the solar wind interaction with the Hermean magnetosphere are presented for southward and northward interplanetary magnetic field (IMF) orientations. Important dawn-dusk asymmetries of the Hermean bow shock and magnetosheath are observed depending on the IMF orientation. For the southward IMF, the dawnside has a thicker magnetosheath with higher beta values and slower bulk velocities compared to the duskside, whereas for the northward IMF, the duskside has a thicker and higher beta magnetosheath with slower bulk velocities. Mirror mode activity consequently appears at the dawnside for the southward IMF and at the duskside for the northward IMF. A mechanism for the bow shock and magnetosheath asymmetries is proposed and discussed in the context of the Hermean and terrestrial magnetosheaths. (en)
Title
  • Mirror mode structures in the asymmetric Hermean magnetosheath: Hybrid simulations
  • Mirror mode structures in the asymmetric Hermean magnetosheath: Hybrid simulations (en)
skos:prefLabel
  • Mirror mode structures in the asymmetric Hermean magnetosheath: Hybrid simulations
  • Mirror mode structures in the asymmetric Hermean magnetosheath: Hybrid simulations (en)
skos:notation
  • RIV/68407700:21340/13:00205229!RIV14-MSM-21340___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I
http://linked.open...iv/cisloPeriodika
  • 1
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
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http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 88517
http://linked.open...ai/riv/idVysledku
  • RIV/68407700:21340/13:00205229
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • Mercury; Mirror waves; Magnetsheat asymmetry (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [9352119587C0]
http://linked.open...i/riv/nazevZdroje
  • Journal of Geophysical Research
http://linked.open...in/vavai/riv/obor
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http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 118
http://linked.open...iv/tvurceVysledku
  • Johnson, J. R.
  • Herčík, David
  • Hellinger, P.
  • Kim, E.-H.
  • Trávníček, P. M.
http://linked.open...ain/vavai/riv/wos
  • 000317858600038
issn
  • 0148-0227
number of pages
http://bibframe.org/vocab/doi
  • 10.1029/2012JA018083
http://localhost/t...ganizacniJednotka
  • 21340
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