The relation between transpolar potential and reconnection rates during sudden enhancement of solar wind dynamic pressure: OpenGGCM-CTIM results-Reference-Cited by-同舟云学术

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The relation between transpolar potential and reconnection rates during sudden enhancement of solar wind dynamic pressure: OpenGGCM-CTIM results

Published:2014-05 Issue:5 Volume:119 Page:3411-3429
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Connor H. K.¹²,Zesta E.³,Ober D. M.²,Raeder J.⁴

Affiliation:

1. Configurable Space Microsystems Innovations and Applications Center; University of New Mexico; Albuquerque New Mexico USA

2. Air Force Research Laboratory; Kirtland AFB; Albuquerque New Mexico USA

3. NASA Goddard Space Flight Center; Greenbelt Maryland USA

4. Space Science Center; University of New Hampshire; Durham New Hampshire USA

Funder

Air Force Office of Scientific Research

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference50 articles.

1. Measurements of the magnetotail reconnection rate;Blanchard;J. Geophys. Res.,1996

2. Accuracy of using the 6300 Å auroral emission to identify the magnetic separatrix on the nightside of the Earth;Blanchard;J. Geophys. Res.,1997

3. Effect of solar wind pressure pulses on the size and strength of the auroral oval;Boudouridis;J. Geophys. Res.,2003

4. Evaluation of the Hill-Siscoe transpolar potential saturation model during a solar wind dynamic pressure pulse;Boudouridis;Geophys. Res. Lett.,2004a

5. Magnetospheric reconnection driven by solar wind pressure fronts;Boudouridis;Ann. Geophys.,2004b

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