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dc.contributorVirginia Techen_US
dc.contributor.authorWilder, F. D.en_US
dc.contributor.authorClauer, C. R.en_US
dc.contributor.authorBaker, Joseph B. H.en_US
dc.date.accessioned2014-02-05T14:20:25Z
dc.date.available2014-02-05T14:20:25Z
dc.date.issued2009-08-01
dc.identifier.citationWilder, F. D., C. R. Clauer, and J. B. H. Baker (2009), Reverse convection potential saturation during northward IMF under various driving conditions, J. Geophys. Res., 114, A08209, doi:10.1029/2009JA014266.
dc.identifier.issn0148-0227
dc.identifier.urihttp://hdl.handle.net/10919/25322
dc.description.abstractWe report the results of an investigation of the reverse convection potentials in the dayside high-latitude ionosphere during periods of steady northward interplanetary magnetic field ( IMF). While it has been demonstrated that the reverse convection potentials exhibit saturation behavior, an investigation into how the saturated reverse convection cells respond to various driving conditions has not yet been performed. We use the OMNI database from 1998 to 2007 to search for events in solar wind data propagated to the bow shock when the IMF is northward and when various driving parameters are stable for more than 40 min. We then use bin-averaged SuperDARN Doppler radar velocity data to apply a spherical harmonic fit to calculate the average potential pattern for various driving conditions. Results show that the saturated reverse convection potential during northward IMF is substantially lower than during southward IMF ( as expected), but the strength of the saturation electric field at a particular location is comparable during northward IMF to what it is during southward IMF. Seasonal dependence and dependence on the Alfvenic Mach number and solar wind beta are also investigated. It appears that the reverse convection potential demonstrates the opposite of what is expected for seasonal dependence, and that the Alfvenic Mach number is not the fundamental driver of its saturation.
dc.description.sponsorshipNational Science FoundationATM-0728538, ATM-0849031
dc.description.sponsorshipNASA NNG05GE25G
dc.format.mimetypeapplication/pdfen_US
dc.language.isoen_US
dc.publisherAmerican Geophysical Union
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjectAuroral radar networken_US
dc.subjectInterplanetary magnetic fieldsen_US
dc.subjectResistive mhd simulationsen_US
dc.subjectScale birkeland currentsen_US
dc.subjectCurrent systemsen_US
dc.subjectSolar-winden_US
dc.subjectGanymedes magnetosphereen_US
dc.subjectReconnection rateen_US
dc.subjectDependenceen_US
dc.subjectSuperDARNen_US
dc.titleReverse convection potential saturation during northward IMF under various driving conditionsen_US
dc.typeArticle - Refereeden_US
dc.contributor.departmentElectrical and Computer Engineeringen_US
dc.identifier.urlhttp://onlinelibrary.wiley.com/doi/10.1029/2009JA014266/pdf
dc.date.accessed2014-01-31
dc.title.serialJournal of Geophysical Research-Space Physics
dc.identifier.doihttps://doi.org/10.1029/2009ja014266
dc.type.dcmitypeTexten_US


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