Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/502
Title: Pseudobreakups dring January 10, 1997
Authors: 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.
Keywords: Pseudobreakups
Ultraviolet imager
Solar wind
UVI images
Issue Date: 1998
Citation: SUBSTORMS-4, edited by S.Kokuburn and Y.Kamide, p.315-318, 1998
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.
URI: http://localhost:8080/xmlui/handle/123456789/502
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