Daytime altitude variations of the equatorial, topside magnetic field-aligned ion transport at solar minimum
Author:
Affiliation:
1. Department of Atmospheric, Oceanic and Space Sciences; University of Michigan; Ann Arbor Michigan USA
2. William B. Hanson Center for Space Sciences; The University of Texas at Dallas; Richardson Texas USA
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/jgra.50284/fullpdf
Reference30 articles.
1. The influence of hemispheric asymmetries on field-aligned ion drifts at the geomagnetic equator;Burrell;Geophys. Res. Lett.,2012
2. Latitude and local time variations of topside magnetic field-aligned ion drifts at solar minimum;Burrell;J. Geophys. Res.,2011
3. Equatorial longitude and local time variations of topside magnetic field-aligned ion drifts at solar minimum;Burrell;J. Geophys. Res.,2012
4. Ion temperature crests and troughs in the morning sector of the low-latitude and midlatitude topside ionosphere;Chao;J. Geophys. Res.,2004
5. Field-aligned plasma diffusive fluxes in the topside ionosphere from radio occultation measurements by CHAMP;Chen;J. Atmos. Sol.-Terr. Phys.,2009
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