On the origin of plasma sheet reconfiguration during the substorm growth phase
Author:
Affiliation:
1. Department of Earth's Physics; Saint Petersburg State University; Saint Petersburg Russia
2. Applied Physics Laboratory; The John Hopkins University; Laurel Maryland USA
3. NASA Goddard Space Flight Center; Greenbelt Maryland USA
Funder
Russian Science Foundation
National Aeronautics and Space Administration
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/2017GL074539/fullpdf
Reference21 articles.
1. Properties of current sheet thinning at x ∼ 10 to 12RE;Artemyev;J. Geophys. Res. Space Physics,2016
2. Changes in magnetospheric configuration during the substorm growth phase;Coroniti;J. Geophys. Res.,1972
3. Can the ionosphere regulate magnetospheric convection?;Coroniti;J. Geophys. Res.,1973
4. Excitation and decay of solarwind driven flows in the magnetosphere-ionosphere system;Cowley;Ann. Geophys.,1992
5. A quasi-static magnetospheric convection model in two dimensions;Erickson;J. Geophys. Res.,1992
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