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dc.contributor.authorTulasiram, S.
dc.contributor.authorBalan, N.
dc.contributor.authorVeenadhari, B.
dc.contributor.authorGurubaran, S.
dc.contributor.authorRavindran, S.
dc.contributor.authorTsugawa, T.
dc.contributor.authorLiu, H.
dc.contributor.authorNiranjan, K.
dc.contributor.authorNagatsuma, T.
dc.date.accessioned2016-01-19T09:44:34Z
dc.date.accessioned2021-02-12T09:42:57Z-
dc.date.available2016-01-19T09:44:34Z
dc.date.available2021-02-12T09:42:57Z-
dc.date.issued2012
dc.identifier.citationJGR-Space Physics, v.117/A9, 2012, doi: 10.1029/2012JA018045en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/848-
dc.description.abstractThe strong westward electrojet and simultaneous upward drift of the equatorial ionospheric peak observed over South-East Asia and Indian equatorial regions during the prolonged Dst minimum phase of an intense geomagnetic storm during 14–15 December 2006 are investigated for the altitudinal variation of zonal electric field polarity using ground based and space-borne observations. The results show first observational evidence for simultaneous existence of daytime westward and eastward zonal electric fields at equatorial E and F region altitudes, respectively, in a wide longitude sector. While the westward electric fields at E region altitudes cause westward electrojet, at the same time, the eastward zonal electric fields atFregion altitudes cause the upward drift of the equatorial ionospheric peak and reinforcement of the equatorial ionization anomaly (EIA) even in the topside ionosphere (∼660 km). The reversal of the electric fields is found to occur at ∼280 km height. A clear bifurcation of F region plasma at ∼280 km is evident in the iso-electron density contours due to these oppositely polarized zonal electric fields, which manifests as an unusually deep cusp between F1 and F2 layers on equatorial ionograms.en_US
dc.language.isoenen_US
dc.subjectElectric fieldsen_US
dc.subjectGeomagnetic stormsen_US
dc.titleFirst observational evidence for opposite zonal electric fields in equatorial E and F region altitudes during a geomagnetic storm perioden_US
dc.typeArticleen_US
dc.identifier.accession091242
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