Modeling the ionosphere-thermosphere response to a geomagnetic storm using physics-based magnetospheric energy input: OpenGGCM-CTIM results-Reference-Cited by-同舟云学术

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Modeling the ionosphere-thermosphere response to a geomagnetic storm using physics-based magnetospheric energy input: OpenGGCM-CTIM results

Published:2016 Issue: Volume:6 Page:A25
ISSN:2115-7251
Container-title:Journal of Space Weather and Space Climate
language:
Short-container-title:J. Space Weather Space Clim.

Author:

Connor Hyunju Kim,Zesta Eftyhia,Fedrizzi Mariangel,Shi Yong,Raeder Joachim,Codrescu Mihail V.,Fuller-Rowell Tim J.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Atmospheric Science

Link

http://www.swsc-journal.org/10.1051/swsc/2016019/pdf

Reference60 articles.

1. Effect of solar wind pressure pulses on the size and strength of the auroral oval

2. Magnetospheric reconnection driven by solar wind pressure fronts

3. Enhanced solar wind geoeffectiveness after a sudden increase in dynamic pressure during southward IMF orientation

4. Temporal evolution of the transpolar potential after a sharp enhancement in solar wind dynamic pressure

5. Statistical study of the effect of solar wind dynamic pressure fronts on the dayside and nightside ionospheric convection

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