Estimating daytime vertical ExB drift velocities in the equatorial F‐region using ground‐based magnetometer observations
By David Anderson, A. Anghel, K. Yumoto, M. Ishitsuka, E. Kudeki. 2002
340 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics
View Paper: https://www.semanticscholar.org/paper/b2b65cecbed4ae8b1a97c71ba31ac88079c8a74c
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Citations in the corpus
- Prompt penetration electric fields (PPEFs) and their ionospheric effects during the great magnetic storm of 30-31 October 2003 (2008, methodology): “We suggest that the Rostogi and Klobuchar [1990]/ Anderson et al. [2002] / McCreadie and Iyemori [2006] empirical technique, plus calculations presented here, be used to develop an empirical storm-time ionospheric PPEF model.”
- Global Assimilation of Ionospheric Measurements (GAIM) (2001, methodology): “…measurements during the daytime and Digisonde data at night are used to determine the equatorial electric field at specific locations as a function of time [Anderson et al., 2002], and these data are used to adjust the Scherliess and Fejer [1999] empirical model of equatorial electric fields.”
- Lunar‐dependent equatorial ionospheric electrodynamic effects during sudden stratospheric warmings (2010, methodology): “magnetic field measurements in the Peruvian region to estimate ionospheric vertical plasma drifts (zonal electric fields) using the methodology developed by Anderson et al. [2002]. These derived drifts are generally in good agreement with the vertical drifts measured by the Jicamarca radar, except b”
- Long‐duration penetration of the interplanetary electric field to the low‐latitude ionosphere during the main phase of magnetic storms (2005, background): “Anderson et al. [2002] showed that the difference in the H component (DH) between a magnetometer on the magnetic equator and one displaced 6–9 degrees away can be used to infer the vertical plasma drift velocity VEB.”
- Equatorial and Low Latitude Ionospheric Effects During Sudden Stratospheric Warming Events (2011, background): “Equatorial daytime vertical drifts are also now routinely derived from the difference of horizontal geomagnetic fields measured at pairs of stations, one very near the magnetic equator and another a few degrees off at about the same longitude (e.g., Anderson et al. 2002).”
- Sq and EEJ—A Review on the Daily Variation of the Geomagnetic Field Caused by Ionospheric Dynamo Currents (2017, methodology): “Building upon those early studies, Anderson et al. (2002) proposed empirical formulae to describe the relationship between the equatorial F-region vertical plasma drift velocity measured by the Jicamarca radar and the difference in H measured by a pair of magnetometers; equatorial station Canete…”