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...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Springer
2017-11-01
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| Series: | Living Reviews in Solar Physics |
| Subjects: | |
| Online Access: | http://link.springer.com/article/10.1007/s41116-017-0009-6 |