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The Sun’s magnetized plasma atmosphere is the source of various forms of activity, the most dramatic of which are coronal mass ejections (CMEs). These ejections are a bulk expulsion of plasma and magnetic field that travel out into the heliosphere, causing space weather effects on any planetary environments that they interact with.
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Initiation of Coronal Mass Ejections
2003Abstract : The over-arching objective of this research was to improve the quantitative basis for prediction of the occurrence of Coronal Mass Ejections (CMEs) and their impact on space weather. The most directly useful discovery, from the point of view of Space Weather forecasting, is that a CME associated with an erupting X-ray sigmoid is more likely ...
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MAVEN observations of the response of Mars to an interplanetary coronal mass ejection
Science, 2015B M Jakosky, C M Fowler, J-A Sauvaud
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The association of coronal mass ejection transients with other forms of solar activity
Solar Physics, 1979J T Gosling
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Coronal Waves and Oscillations
Living Reviews in Solar Physics, 2005Valery M Nakariakov, Erwin Verwichte
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