Pseudobreakups dring January 10, 1997

Arballo, J.K.; Ho, Christian M.; Lakhina, G.S.; Tsurutani, B.T.; Zhou, X.-Y.; Kamide, Y.; Shue, J.-H.; Akasofu, S.-I.; Lepping, R.P.; Goodrich, C.C.; Papadopoulos, K.; Sharma, A.S.; Lyon, J.G.

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dc.contributor.author	Arballo, J.K.
dc.contributor.author	Ho, Christian M.
dc.contributor.author	Lakhina, G.S.
dc.contributor.author	Tsurutani, B.T.
dc.contributor.author	Zhou, X.-Y.
dc.contributor.author	Kamide, Y.
dc.contributor.author	Shue, J.-H.
dc.contributor.author	Akasofu, S.-I.
dc.contributor.author	Lepping, R.P.
dc.contributor.author	Goodrich, C.C.
dc.contributor.author	Papadopoulos, K.
dc.contributor.author	Sharma, A.S.
dc.contributor.author	Lyon, J.G.
dc.date.accessioned	2015-09-29T06:15:38Z
dc.date.accessioned	2021-02-12T09:30:13Z
dc.date.available	2015-09-29T06:15:38Z
dc.date.available	2021-02-12T09:30:13Z
dc.date.issued	1998
dc.identifier.citation	SUBSTORMS-4, edited by S.Kokuburn and Y.Kamide, p.315-318, 1998	en_US
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/502
dc.description.abstract	The 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.iso	en	en_US
dc.subject	Pseudobreakups	en_US
dc.subject	Ultraviolet imager	en_US
dc.subject	Solar wind	en_US
dc.subject	UVI images	en_US
dc.title	Pseudobreakups dring January 10, 1997	en_US
dc.type	Article	en_US
dc.identifier.accession	091013