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A new solar windâ driven global dynamic plasmapause model: 1. Database and statistics
dc.contributor.authorZhang, Xiao‐xin
dc.contributor.authorHe, Fei
dc.contributor.authorLin, Rui‐lin
dc.contributor.authorFok, Mei‐ching
dc.contributor.authorKatus, Roxanne M.
dc.contributor.authorLiemohn, Michael W.
dc.contributor.authorGallagher, Dennis L.
dc.contributor.authorNakano, Shinya
dc.date.accessioned2017-10-05T18:19:22Z
dc.date.available2018-09-13T15:12:06Zen
dc.date.issued2017-07
dc.identifier.citationZhang, Xiao‐xin ; He, Fei; Lin, Rui‐lin ; Fok, Mei‐ching ; Katus, Roxanne M.; Liemohn, Michael W.; Gallagher, Dennis L.; Nakano, Shinya (2017). "A new solar windâ driven global dynamic plasmapause model: 1. Database and statistics." Journal of Geophysical Research: Space Physics 122(7): 7153-7171.
dc.identifier.issn2169-9380
dc.identifier.issn2169-9402
dc.identifier.urihttps://hdl.handle.net/2027.42/138358
dc.description.abstractA large database, possibly the largest plasmapause location database, with 49,119 plasmapause crossing events from the in situ observations and 3957 plasmapause profiles (corresponding to 48,899 plasmapause locations in 1 h magnetic local time (MLT) intervals) from optical remote sensing from 1977 to 2015 by 18 satellites is compiled. The responses of the global plasmapause to solar wind and geomagnetic changes and the diurnal, seasonal, solar cycle variations of the plasmapause are investigated based on this database. It is found that the plasmapause shrinks toward the Earth globally and a clear bulge appears in the afternoon to premidnight MLT sector as the solar wind or geomagnetic conditions change from quiet to disturbed. The bulge is clearer during storm times or southward interplanetary magnetic field. The diurnal variations of the plasmapause are most probably the result of the difference between the magnetic dipole tilt and the Earth’s spin axis. The seasonal variations of the plasmapause are characterized by equinox valleys and solstice peaks. It is also found that the plasmapause approaches the Earth during high solar activity and expands outward during low solar activity. This database will help us study and understand the evolution properties of the plasmapause shape and the interaction processes of the plasmasphere, the ring current, and the radiation belts in the magnetosphere.Key PointsThe largest currently available plasmapause location database is compiled based on observations from 18 satellites from 1977 to 2015This database reveals the responses of the global plasmapause locations to solar wind and geomagnetic changesThe plasmapause locations exhibit clear MLTâ dependent diurnal, seasonal, and solar cycle variations
dc.publisherOxford
dc.publisherWiley Periodicals, Inc.
dc.subject.otherstatistics
dc.subject.otherdatabase
dc.subject.othersolar activity
dc.subject.otherplasmapause
dc.subject.otherplasmasphere
dc.subject.othergeomagnetic activity
dc.titleA new solar windâ driven global dynamic plasmapause model: 1. Database and statistics
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/2027.42/138358/1/jgra53617_am.pdf
dc.description.bitstreamurlhttps://deepblue.lib.umich.edu/bitstream/2027.42/138358/2/jgra53617.pdf
dc.identifier.doi10.1002/2017JA023912
dc.identifier.sourceJournal of Geophysical Research: Space Physics
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dc.owningcollnameInterdisciplinary and Peer-Reviewed


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