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Eruptive event generator based on the Gibson‐Low magnetic configuration
dc.contributor.authorBorovikov, D.
dc.contributor.authorSokolov, I. V.
dc.contributor.authorManchester, W. B.
dc.contributor.authorJin, M.
dc.contributor.authorGombosi, T. I.
dc.date.accessioned2017-10-23T17:30:45Z
dc.date.available2018-10-02T19:49:01Zen
dc.date.issued2017-08
dc.identifier.citationBorovikov, D.; Sokolov, I. V.; Manchester, W. B.; Jin, M.; Gombosi, T. I. (2017). "Eruptive event generator based on the Gibson‐Low magnetic configuration." Journal of Geophysical Research: Space Physics 122(8): 7979-7984.
dc.identifier.issn2169-9380
dc.identifier.issn2169-9402
dc.identifier.urihttps://hdl.handle.net/2027.42/138857
dc.description.abstractCoronal mass ejections (CMEs), a kind of energetic solar eruptions, are an integral subject of space weather research. Numerical magnetohydrodynamic (MHD) modeling, which requires powerful computational resources, is one of the primary means of studying the phenomenon. With increasing accessibility of such resources, grows the demand for user‐friendly tools that would facilitate the process of simulating CMEs for scientific and operational purposes. The Eruptive Event Generator based on Gibson‐Low flux rope (EEGGL), a new publicly available computational model presented in this paper, is an effort to meet this demand. EEGGL allows one to compute the parameters of a model flux rope driving a CME via an intuitive graphical user interface. We provide a brief overview of the physical principles behind EEGGL and its functionality. Ways toward future improvements of the tool are outlined.Key PointsIncrease visibility of a recently developed online tool, EEGGLProvide brief overview of the basic principles EEGGL is based onOutline the direction of future development of EEGGL
dc.publisherTERRAPUB
dc.publisherWiley Periodicals, Inc.
dc.subject.othermethods: numerical
dc.subject.othermagnetohydrodynamics (MHD)
dc.subject.otherSun: coronal mass ejections (CMEs)
dc.titleEruptive event generator based on the Gibson‐Low magnetic configuration
dc.typeArticleen_US
dc.rights.robotsIndexNoFollow
dc.subject.hlbsecondlevelAstronomy and Astrophysics
dc.subject.hlbtoplevelScience
dc.description.peerreviewedPeer Reviewed
dc.description.bitstreamurlhttps://deepblue.lib.umich.edu/bitstream/2027.42/138857/1/jgra53711.pdf
dc.description.bitstreamurlhttps://deepblue.lib.umich.edu/bitstream/2027.42/138857/2/jgra53711_am.pdf
dc.identifier.doi10.1002/2017JA024304
dc.identifier.sourceJournal of Geophysical Research: Space Physics
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dc.owningcollnameInterdisciplinary and Peer-Reviewed


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