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dc.contributor.authorArballo, J.K.
dc.contributor.authorHo, Christian M.
dc.contributor.authorLakhina, G.S.
dc.contributor.authorTsurutani, B.T.
dc.contributor.authorZhou, X.-Y.
dc.contributor.authorKamide, Y.
dc.contributor.authorShue, J.-H.
dc.contributor.authorAkasofu, S.-I.
dc.contributor.authorLepping, R.P.
dc.contributor.authorGoodrich, C.C.
dc.contributor.authorPapadopoulos, K.
dc.contributor.authorSharma, A.S.
dc.contributor.authorLyon, J.G.
dc.date.accessioned2015-09-29T06:15:38Z
dc.date.accessioned2021-02-12T09:30:13Z-
dc.date.available2015-09-29T06:15:38Z
dc.date.available2021-02-12T09:30:13Z-
dc.date.issued1998
dc.identifier.citationSUBSTORMS-4, edited by S.Kokuburn and Y.Kamide, p.315-318, 1998en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/502-
dc.description.abstractThe January 10, 1997 interplanetary pressure pulse (observed at 0053 UT at Wind) caused a dayside aurora, as seen in Polar Ultraviolet Imager (UVI) data that propagates tailward and to lower L. After the solar wind has propagated -150 Re, downtail, a substorm pseu-dobreakup (PB) was detected at 68" N magnetic latitude, at local midnight. The PB dimmed on time scales of minutes and rebrightened 9 min. later. This happened several times in succession. A quasiperiod of approximately 10 min. was noted. The scale size of the PBs was -200 by 200 km in the ionosphere and there was no evidence of eastward drifts of the electrons causing the aurorat brightening.en_US
dc.language.isoenen_US
dc.subjectPseudobreakupsen_US
dc.subjectUltraviolet imageren_US
dc.subjectSolar winden_US
dc.subjectUVI imagesen_US
dc.titlePseudobreakups dring January 10, 1997en_US
dc.typeArticleen_US
dc.identifier.accession091013
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