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Erschienen in:
Introduction to the Handbook of Cosmic Hazards and Planetary Defense Kapitel lesen Erstes Kapitel lesen

2015 | OriginalPaper | Buchkapitel

Coronal Mass Ejections

verfasst von : Maher A. Dayeh

Erschienen in: Handbook of Cosmic Hazards and Planetary Defense

Verlag: Springer International Publishing

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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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Vorheriges Kapitel Solar Flares and Impact on Earth
Nächstes Kapitel Fundamental Aspects of Coronal Mass Ejections
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Metadaten
Titel
Coronal Mass Ejections
verfasst von
Maher A. Dayeh
Copyright-Jahr
2015
Buch
Handbook of Cosmic Hazards and Planetary Defense

Print ISBN: 978-3-319-03951-0

Electronic ISBN: 978-3-319-03952-7

Copyright-Jahr: 2015

DOI
https://doi.org/10.1007/978-3-319-03952-7_9

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