Modeling Equatorial Plasma Bubbles With SAMI3/WACCM-X: September 2017 Storm

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Abstract

We report results from a global simulation of the September 2017 geomagnetic storm. The global model comprises the ionospheric code SAMI3 and the atmosphere/thermosphere code WACCM-X. We show that a train of large-scale EPBs form in the Pacific sector during the storm recovery phase on 8 September 2017. The EPBs are associated with storm-induced modification of the zonal and meridional winds. These changes lead to an eastward electric field which in turn causes an upward E × B drift in the post-midnight sector. A large decrease in the Pedersen conductance caused by meridional equatorward winds leads to an increase in the growth rate of the generalized Rayleigh-Taylor instability that causes EPBs to develop. Interestingly, several EPBs reach altitudes above 3,000 km.

Original languageEnglish
Article numbere2024GL109071
JournalGeophysical Research Letters
Volume51
Issue number11
DOIs
StatePublished - Jun 16 2024

Keywords

  • disturbance dynamo
  • equatorial plasma bubbles
  • geomagnetic storms
  • stormtime winds

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