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Understanding interplanetary coronal mass ejection signatures
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DOI：10.1007/s11214-006-9017-x.png)
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While interplanetary coronal mass ejections (ICMEs) are understood to be the heliospheric counterparts of CMEs, with signatures undeniably linked to the CME process, the variability of these signatures and questions about mapping to observed CME features raise issues that remain on the cutting edge of ICME research. These issues are discussed in the context of traditional understanding, and recent results using innovative analysis techniques are reviewed.
Keyword:
coronal mass ejections
interplanetary physics
solar wind
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7.4
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4.2K
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