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Volumn 672, Issue 2, 2008, Pages 1221-1227
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Using global simulations to relate the three-part structure of coronal mass ejections to in situ signatures
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Author keywords
Solar wind; Sun: activity; Sun: corona; Sun: coronal mass ejections (CMEs); Sun: magnetic fields
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Indexed keywords
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EID: 40249095929
PISSN: 0004637X
EISSN: 15384357
Source Type: Journal
DOI: 10.1086/523893 Document Type: Article |
Times cited : (70)
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References (45)
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