The Dayside Ionospheric “Superfountain” (DIS), plasma transport and other consequences

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dc.contributor.authorTsurutani, B.T.
dc.contributor.authorSaito, A.
dc.contributor.authorVerkhoglyadova, O.P.
dc.contributor.authorMannucci, A.J.
dc.contributor.authorAbdu, M.A.
dc.contributor.authorAraki, T.
dc.contributor.authorGonzalez, W.D.
dc.contributor.authorIijima, B.A.
dc.contributor.authorLakhina, G.S.
dc.contributor.authorMcCreadie, H.
dc.contributor.authorSobral, J.H.A.
dc.contributor.authorTsuda, T.
dc.contributor.authorYumoto, K.
dc.contributor.authorVasyliunas, V.M.
dc.date.accessioned2015-09-08T09:31:24Z
dc.date.accessioned2021-02-12T09:48:25Z
dc.date.available2015-09-08T09:31:24Z
dc.date.available2021-02-12T09:48:25Z
dc.date.issued2006
dc.description.abstractPrompt penetration electric fields (PPEFs) and the consequential dayside ionospheric superfountain (DIS) are reviewed. An example of O+ uplift to ~840 km altitude at ~0940 local time (DMSP F15) during the superstorm of 30 October 2003 is illustrated. The SAMI-2 model is modified to incorporate intense superstorm electric fields. With an inclusion of a ~4 mV/m eastward electric field, SAMI-2* modeling results show many of the expected DIS effects.en_US
dc.identifier.accession090850
dc.identifier.citationILWS Workshop 2006, Goa, 2006en_US
dc.identifier.urihttp://library.iigm.res.in:4000/handle/123456789/357
dc.language.isoenen_US
dc.subjectDayside ionospheric superfountain effectsen_US
dc.subjectIonospheric stormsen_US
dc.subjectMagnetic stormsen_US
dc.subjectPrompt penetration electric fieldsen_US
dc.subjectPlasma transporten_US
dc.subjectPPEFen_US
dc.titleThe Dayside Ionospheric “Superfountain” (DIS), plasma transport and other consequencesen_US
dc.typeArticleen_US

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