Slow mode structure in the nightside magnetosheath related to IMF draping-Reference-Cited by-同舟云学术

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Slow mode structure in the nightside magnetosheath related to IMF draping

Published:2014-02 Issue:2 Volume:119 Page:1121-1128
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Erkaev N. V.¹²,Farrugia C. J.³,Mezentsev A. V.²,Torbert R. B.³,Biernat H. K.⁴⁵

Affiliation:

1. Institute of Computational Modeling SB RAS; Krasnoyarsk Russia

2. Siberian Federal University; Krasnoyarsk Russia

3. Space Science Center and Department of Physics; University of New Hampshire; Durham New Hampshire USA

4. Space Research Institute; Austrian Academy of Sciences; Graz Austria

5. Institute of Physics; Karl-Franzens-University of Graz; Graz Austria

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2013JA019514/fullpdf

Reference23 articles.

1. Aspects of MHD flow about Venus;Biernat;J. Geophys. Res.,1999

2. Anomalous aspects of magnetosheath flow and of the shape and oscillations of the magnetopause during an interval of strongly northward interplanetary magnetic field;Chen;J. Geophys. Res.,1993

3. Results of the investigation of MHD flow around the magnetosphere;Erkaev;Geomagn. Aeron.,1988

4. On accelerated magnetosheath flows under northward IMF;Erkaev;Geophys. Res. Lett.,2011

5. Accelerated magnetosheath flows caused by IMF draping: Dependence on latitude;Erkaev;Geophys. Res. Lett.,2012

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