Magnetohydrodynamic simulation of non-flux rope coronal mass ejections
Magnetohydrodynamic simulation of non-flux rope coronal mass ejections
About this item
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Author / Creator
Publisher
Washington, DC: Blackwell Publishing Ltd
Journal title
Language
English
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Publisher
Washington, DC: Blackwell Publishing Ltd
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Scope and Contents
Contents
Observations at 1 AU indicate that only 1/3 of coronal mass ejections (CMEs) have a flux rope structure, while the other 2/3 of CMEs have a complex disordered magnetic field. The initiation of the flux rope CMEs has been extensively simulated with various magnetohydrodynamic (MHD) models. However, the initiation of the non–flux rope CMEs is rarely...
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Full title
Magnetohydrodynamic simulation of non-flux rope coronal mass ejections
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Record Identifier
TN_cdi_proquest_miscellaneous_34496374
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_34496374
Other Identifiers
ISSN
0148-0227
E-ISSN
2156-2202
DOI
10.1029/2008JA013860
