Coronal mass ejections and their sheath regions in interplanetary space

Coronal mass ejections and their sheath regions in interplanetary space

Abstract Interplanetary coronal mass ejections (ICMEs) are large-scale heliospheric transients that originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a shock wave develops ahead of the ICME. The turbulent region between the shock and the ICME is called the sh...

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Bibliographic Details
Main Authors: Emilia Kilpua, Hannu E. J. Koskinen, Tuija I. Pulkkinen
Format: Article
Language:English
Published: SpringerOpen 2017-11-01
Series:Living Reviews in Solar Physics
Subjects:
Coronal mass ejections
Solar wind
Space weather
Interplanetary shocks
Magnetic clouds
Online Access:http://link.springer.com/article/10.1007/s41116-017-0009-6

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http://link.springer.com/article/10.1007/s41116-017-0009-6

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