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 |
Appears in Collections: | UAS_Reprints |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
LakhinGS_etal_SUBSTORMS-4_1998-1.pdf Restricted Access | 1.17 MB | Adobe PDF | View/Open Request a copy |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.