Pseudobreakups dring January 10, 1997
| 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.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.identifier.accession | 091013 | |
| dc.identifier.citation | SUBSTORMS-4, edited by S.Kokuburn and Y.Kamide, p.315-318, 1998 | en_US |
| dc.identifier.uri | http://library.iigm.res.in:4000/handle/123456789/502 | |
| 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 |