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dc.contributor.authorSripathi, S.
dc.contributor.authorBanola, S.
dc.contributor.authorEmperumal, K.
dc.contributor.authorKumar, B. Suneel
dc.contributor.authorRadicella, Sandro M.
dc.date.accessioned2011-06-17T23:31:48Z
dc.date.accessioned2021-02-12T10:11:39Z-
dc.date.available2011-06-17T23:31:48Z
dc.date.available2021-02-12T10:11:39Z-
dc.date.issued2018
dc.identifier.citationJGR, 123, 2336–2350, doi: 10.1002/2017JA024956en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/1210-
dc.description.abstractWe investigate the role of storm time electrodynamics in suppressing the equatorial plasma bubble (EPB) development using multi-instruments over India during a moderate geomagnetic storm that occurred on 2 October 2013 where Dst minimum reached ~ 80 nT. This storm produced unique signatures in the equatorial ionosphere such that equatorial electrojet strength showed signatures of an abrupt increase of its strength to 150 nT and occurrence of episodes of counter electrojet events. During the main phase of the storm, the interplanetary magnetic field Bz is well correlated with the variations in the equatorial electrojet/counter electrojet suggesting the role of undershielding/overshielding electric fields of magnetospheric origin. Further, observations showed the presence of strong F3 layers at multiple times at multiple stations due to undershielding electric field. Interestingly, we observed simultaneous presence of F3 layers and suppression of EPBs in the dusk sector during the recovery phase. While strong EPBs were observed before and after the day of the geomagnetic storm, suppression of the EPBs on the storm day during “spread F season” is intriguing. Our further analysis using low-latitude station, Hyderabad, during the time of prereversal enhancement suggests that intense Esb layers were observed on the storm day but were absent/weak on quiet days. Based on these results, we suggest that the altitude/latitude variation of disturbance dynamo electric fields/disturbance winds may be responsible for simultaneous detection of F3 layers, occurrence of low-latitude Es layers, and suppression of EPBs during the storm day along the sunset terminator.en_US
dc.language.isoen_USen_US
dc.subjectElectrodynamicsen_US
dc.subjectGeomagnetic stormen_US
dc.subjectEquatorial Plasma bubbleen_US
dc.subjectEPBsen_US
dc.titleThe Role of Storm Time Electrodynamics in Suppressing the Equatorial Plasma Bubble Development in the Recovery Phase of a Geomagnetic Stormen_US
dc.typeArticleen_US
dc.identifier.accession091744
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