Storm-time changes in the upper atmosphere at low latitudes

By T. Fuller‐Rowell, G. Millward, Arthur D. Richmond, M. Codrescu. 2002

249 citations recorded by the source corpus.

Citations in the corpus

Equatorial Ionospheric Electric Fields During the November 2004 Magnetic Storm (2007, unknown): “Relatively fast (occurring about 2–3 h after major increases in convection) disturbance dynamo electric fields [e.g., Scherliess and Fejer, 1997] are most likely due to the dynamo action of fast traveling equatorward wind surges [e.g., Fuller-Rowell et al., 2002 ], while slower disturbances (occurr”
Sq and EEJ—A Review on the Daily Variation of the Geomagnetic Field Caused by Ionospheric Dynamo Currents (2017, unknown): “Besides, storm-time thermospheric winds tend to drive a westward electric field in the dayside equatorial region through the mechanism known as disturbance dynamo (Blanc and Richmond 1980; Fuller-Rowell et al. 2002).”
Unusual early morning development of the equatorial anomaly in the Brazilian sector during the Halloween magnetic storm (2006, unknown): “According to that simulation, the waves could reach the equatorial latitudes in about 2 hours and cause significant disturbances in the ionosphere [see also Fuller-Rowell et al., 2002 ].”