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dc.contributor.authorNayak, C.K.
dc.contributor.authorYadav, Virendra
dc.contributor.authorKakad, Bharati
dc.contributor.authorSripathi, S.
dc.contributor.authorEmperumal, K.
dc.contributor.authorPant, T.K.
dc.contributor.authorBhattacharyya, A.
dc.contributor.authorJin, Shuanggen
dc.date.accessioned2015-12-03T10:17:22Z
dc.date.accessioned2021-02-12T09:48:38Z-
dc.date.available2015-12-03T10:17:22Z
dc.date.available2021-02-12T09:48:38Z-
dc.date.issued2014
dc.identifier.citationJGR, v.119, p. 8685-8696, 2014, doi: 10.1002/2014JA020135en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/757-
dc.description.abstractWe present the seasonal and local time occurrence of ionospheric F3 layer over Tirunelveli (geographic longitude 77.8°E, geographic latitude 8.7°N, dip 0.7°) during extremely low and prolonged solar activity period (2007–2009). Canadian Advanced Digital Ionosonde observations from this station are used in the present study. We find that the occurrence of F3 layer is nearly 3 times higher during 2009 (∼ 48%) as compared to that during 2007 (∼16%). The increase of this order just within the low solar activity period is unusual. In earlier studies similar increase in F3 occurrence has been reported when solar activity changes from high (F10.7=182) to low (F10.7=72). The other important feature is the presence of postnoon F3 layers which are observed dominantly during summer solstice of 2009. Such occurrence of postnoon F3 layers was nearly absent during summer solstice of the previous solar minimum (1996) over nearby dip equatorial station Trivandrum. We take equatorial electrojet (EEJ) as a proxy for eastward electric field. It is noticed that the EEJ strength and the maximum rate of change of EEJ are higher for F3 days as compared to those on non-F3 days. We find that the peak occurrence of prenoon F3 layer closely coincides with the time of maximum rate of change of EEJ. It is in general accordance with the theory proposed by Balan et al. (1998) that suggests the formation of F3 through vertically upward E × B drift in presence of equatorward neutral wind. The present study reveals that the rate of change of eastward electric field (dE/dt) as well plays an important role in the formation of F3 layer.en_US
dc.language.isoenen_US
dc.subjectIonospheric F3 layeren_US
dc.subjectEquatorial electrojeten_US
dc.subjectSolar activityen_US
dc.titlePeculiar features of ionospheric F3 layer during prolonged solar minimum (2007–2009)en_US
dc.typeArticleen_US
dc.identifier.accession091421
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