Modeling the Development of an Equatorial Plasma Bubble During a Midnight Temperature Maximum With SAMI3/WACCM‐X
Abstract
We report results from a self‐consistent global simulation model in which a large‐scale equatorial plasma bubble (EPB) forms during a midnight temperature maximum (MTM). The global model comprises the ionospheric code SAMI3 and the atmosphere/thermosphere code WACCM‐X. We consider solar minimum conditions for the month of August. We show that an EPB forms during an MTM in the Pacific sector and is caused by equatorward neutral wind flows. Although this is consistent with the theoretical result that a meridional neutral wind (V) with a negative gradient (∂V/∂θ https://doi.org/10.1002/grl.50292] (where a northward meridional neutral wind V is positive and θ is the latitude and increases in the northward direction), we find that the primary cause of the EPB is the large decrease in the Pedersen conductance caused by the equatorward winds.
Document Details
- Document Type
- Pub Defense Publication
- Publication Date
- Aug 01, 2023
- Source ID
- 10.1029/2023gl104388
Entities
People
- Han-Li Liu
- J. D. Huba
- Joseph McInerney
Organizations
- Air Force Office of Scientific Research
- Directorate for Geosciences
- High Altitude Observatory
- National Aeronautics and Space Administration
- National Science Foundation
- Syntek Technologies