Results 191 to 200 of about 426 (204)
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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
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
Blast-wave and piston shocks connected with the formation and propagation of a coronal mass ejection
Astronomy Reports, 2013M V Eselevich +2 more
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Acceleration and transport of heavy ions at coronal mass ejection-driven shocks
Journal of Geophysical Research, 2005Gang Li, G P Zank, Ken Rice
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The association of coronal mass ejection transients with other forms of solar activity
Solar Physics, 1979R H Munro, J T Gosling, E Hildner
exaly
Influence of coronal mass ejection interaction on propagation of interplanetary shocks
Journal of Geophysical Research, 2004P K Manoharan, N Gopalswamy, S Yashiro
exaly
Energetic storm particle events in coronal mass ejection-driven shocks
Journal of Geophysical Research, 2011P 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, 2009S A Haider, I S Batista, E Kallio
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