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Coronal Mass Ejections

  • Maher A. DayehEmail author
Reference work entry

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.

Keywords

Coronal mass ejections Solar wind Interplanetary coronal mass ejections Interplanetary shocks Geomagnetic storms Solar energetic particles Space weather 

Notes

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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Copyright information

© Springer International Publishing Switzerland 2015

Authors and Affiliations

  1. 1.Space Science and Engineering DivisionSouthwest Research InstituteSan AntonioUSA

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