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 language | English |
|---|---|
| Article number | e2024GL109071 |
| Journal | Geophysical Research Letters |
| Volume | 51 |
| Issue number | 11 |
| DOIs | |
| State | Published - Jun 16 2024 |
Keywords
- disturbance dynamo
- equatorial plasma bubbles
- geomagnetic storms
- stormtime winds