Low latitude storm time ionospheric electrodynamics
By B. Fejer. 2002
167 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics
View Paper: https://www.semanticscholar.org/paper/62734c4383c222fee77f05920b45e30cd831d4dd
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In Astronomy and Astrophysics
- B. Fejer
- Shin-Yi Su
- B. Tsurutani
- J. W. Jensen
- W. Gonzalez
- Akinori Saito
- R. Skoug
- Anthony J. Mannucci
In Geophysics
Citations in the corpus
- Equatorial Ionospheric Electric Fields During the November 2004 Magnetic Storm (2007, unknown): “On the other hand, the large variability of these electric fields is not well understood [e.g., Fejer, 2002; Huang et al., 2005], which indicates that their magnitudes and lifetimes are also affected by additional solar wind, magnetospheric, and high and low latitude ionospheric processes [e.g., S”
- Low‐latitude ionosphere response to super geomagnetic storm of 17/18 March 2015: Results from a chain of ground‐based observations over Indian sector (2015, background): “But it has been also shown that PP electric fields during daytime from high to low latitudes as a contributing factor to TEC increase [Fejer, 2002; Fejer and Scherliess, 1997].”
- Unusual early morning development of the equatorial anomaly in the Brazilian sector during the Halloween magnetic storm (2006, unknown): “the empirical model of Scherliees and Fejer [1999]. A disturbance downward vertical drift (resembling the drift caused by a prompt penetration westward electric field) was”
- Dayside global ionospheric response to the major interplanetary events of October 29–30, 2003 “Halloween Storms” (2005, background): “…increases may be daytime eastward-directed electric fields penetrating promptly from high to low latitudes, as has been reported previously but primarily for dusk to midnight local times [Fejer, 2002; Tanaka and Ohtaka, 1996; Vlasov et al., 2003; Fejer and Scherliess, 1997; Greenspan et al., 1991].”
- Seasonal and longitudinal dependence of equatorial disturbance vertical plasma drifts (2008, result): “…the Peruvian equatorial region, the evening downward disturbance dynamo drifts during equinox are larger than during June solstice, and that the postmidnight upward drifts during these two seasons have comparable magnitudes [Fejer, 2002], which is again fully consistent with our satellite results.”