Abstract
Coronal mass ejections (CMEs) are the most energetic solar phenomena in the inner heliosphere. CMEs are large structures of magnetized plasma that move away from the Sun into the interplanetary (IP) space, driven by the magnetic forces at the Sun. Solar energetic particles (SEPs) and geomagnetic storms are two primary CME consequences that drive space weather on and near Earth. This chapter summarizes current established knowledge of CME properties and their space weather consequences.
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Acknowledgments
The author would like to thank Heather Elliott for her constructive comments on the manuscript. This work was supported in part by NASA Award No. NNX13AE07G.
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Dayeh, M.A. (2015). Coronal Mass Ejections. In: Pelton, J., Allahdadi, F. (eds) Handbook of Cosmic Hazards and Planetary Defense. Springer, Cham. https://doi.org/10.1007/978-3-319-03952-7_9
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DOI: https://doi.org/10.1007/978-3-319-03952-7_9
Publisher Name: Springer, Cham
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