Peculiar features of ionospheric F3 layer during prolonged solar minimum (2007–2009)

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dc.contributor.author Nayak, C.K.
dc.contributor.author Yadav, Virendra
dc.contributor.author Kakad, Bharati
dc.contributor.author Sripathi, S.
dc.contributor.author Emperumal, K.
dc.contributor.author Pant, T.K.
dc.contributor.author Bhattacharyya, A.
dc.contributor.author Jin, Shuanggen
dc.date.accessioned 2015-12-03T10:17:22Z
dc.date.accessioned 2021-02-12T09:48:38Z
dc.date.available 2015-12-03T10:17:22Z
dc.date.available 2021-02-12T09:48:38Z
dc.date.issued 2014
dc.identifier.citation JGR, v.119, p. 8685-8696, 2014, doi: 10.1002/2014JA020135 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/757
dc.description.abstract We 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.iso en en_US
dc.subject Ionospheric F3 layer en_US
dc.subject Equatorial electrojet en_US
dc.subject Solar activity en_US
dc.title Peculiar features of ionospheric F3 layer during prolonged solar minimum (2007–2009) en_US
dc.type Article en_US
dc.identifier.accession 091421


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