Saturation of superstorms and finite compressibility of the magnetosphere: Results of the magnetogram inversion technique and global PPMLR-MHD model
Author:
Affiliation:
1. ISTP SB RAS; Irkutsk Russia
2. CALT; CASC; Beijing China
3. NSSC; CAS; Beijing China
Funder
RFBR
NSFC
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/2016GL069649/fullpdf
Reference32 articles.
1. Geomagnetic signatures during the intense geomagnetic storms of 29 October and 20 November 2003;Alex;J. Atmos. Sol. Terr. Phys.,2006
2. Polar cap potential saturation, dayside reconnection, and changes to the magnetosphere;Borovsky;J. Geophys. Res.,2009
3. Two models of cross polar cap potential saturation compared: Siscoe - Hill model versus Kivelson-Ridley model;Gao;J. Geophys. Res. Space Physics,2013
4. Magnetic merging line and reconnection voltage versus IMF clock angle: Results from global MHD simulations;Hu;J. Geophys. Res.,2009
5. April 2000 magnetic storm: Solar wind driver and magnetospheric response;Huttunen;J. Geophys. Res.,2002
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