Results 191 to 200 of about 426 (204)
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On the viscosity effects in the shock wave observed in the solar wind after the December 13, 2006 coronal mass ejection

Astrophysical Bulletin, 2015
Coronal mass ejections (CMEs) and solar wind are the main results of solar activity. These events can drive interplanetary shock waves and produce geomagnetic storms. The study of these events is very important for space weather purposes. The shock waves occur where the solar wind changes its characteristics from being supersonic (with respect to the ...
openaire   +2 more sources

Influence of a Coronal Mass Ejection on the Solar Cosmic Ray Acceleration by a Shock Wave in the Lower Solar Corona

Journal of Experimental and Theoretical Physics, 2022
S. N. Taneev   +2 more
openaire   +1 more source

Blast-wave and piston shocks connected with the formation and propagation of a coronal mass ejection

Astronomy Reports, 2013
M V Eselevich   +2 more
exaly  

Acceleration and transport of heavy ions at coronal mass ejection-driven shocks

Journal of Geophysical Research, 2005
Gang Li, G P Zank, Ken Rice
exaly  

Influence of coronal mass ejection interaction on propagation of interplanetary shocks

Journal of Geophysical Research, 2004
P K Manoharan, N Gopalswamy, S Yashiro
exaly  

Propagation of the 12 May 1997 interplanetary coronal mass ejection in evolving solar wind structures

Journal of Geophysical Research, 2005
D Odstrčil, V J Pizzo, C N Arge
exaly  

Energetic storm particle events in coronal mass ejection-driven shocks

Journal of Geophysical Research, 2011
P Mäkelä, N Gopalswamy, S Akiyama
exaly  

On the responses to solar X‐ray flare and coronal mass ejection in the ionospheres of Mars and Earth

Geophysical Research Letters, 2009
S A Haider, I S Batista, E Kallio
exaly  

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