Occurrence of blanketing Es layer (Esb) over the equatorial region during the peculiar minimum of solar cycle 24

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dc.contributor.author Yadav, Virendra
dc.contributor.author Kakad, Bharati
dc.contributor.author Nayak, C.K.
dc.contributor.author Surve, G.
dc.contributor.author Emperumal, K.
dc.date.accessioned 2015-12-02T09:00:59Z
dc.date.accessioned 2021-02-12T09:46:36Z
dc.date.available 2015-12-02T09:00:59Z
dc.date.available 2021-02-12T09:46:36Z
dc.date.issued 2014
dc.identifier.citation Ann. Geophys, v.32, p.553-562, 2014, doi: 10.5194/angeo-32-553-2014 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/733
dc.description.abstract A thin and highly dense sporadic E layer, which can occasionally block the upper ionospheric layers, is called blanketing sporadic E (Esb). We present the statistical seasonal local time occurrence pattern of Esb at equatorial station Tirunelveli (8.7° N, 77.8° E, dip latitude 0.7° N) during the extended minimum of solar cycle 24 (2007–2009). In spite of nearly the same average solar activity during both 2007 and 2009, considerable differences are noticed in the seasonal occurrence of Esb during this period. The percentage of Esb occurrence is found to be the highest during the summer solstice (≥ 50%) for both 2007 and 2009, which is in general accordance with the earlier studies. The occurrences of Esb during the vernal equinox (~ 33%) and January–February (~ 28%) are substantial in 2009 as compared to those during the same seasons in 2007. We find that, during winter (January–February), ~ 75% of Esb occurred during or just after the period of sudden stratospheric warming (SSW). We suggest that enhanced Esb occurrence during winter (January–February) and the vernal equinox of 2009 could be associated with SSW-driven changes in the E region ambient conditions. Furthermore, the close association of Esb with counter equatorial electrojet (CEEJ) suggested by earlier studies is re-examined carefully using the scenario of Esb occurrence on non-CEEJ days. Such an exercise is crucial as we are unaware whether the physical mechanisms driving Esb and CEEJ are linked or not. We find that, of all the seasons, the association of Esb and CEEJ is strongest during winter (November–December). en_US
dc.language.iso en en_US
dc.subject Ionospheric irregularities en_US
dc.subject Counter equatorial electrojet en_US
dc.subject Equatorial ionosphere en_US
dc.subject Equatorial electrojet en_US
dc.subject Solar cycle en_US
dc.title Occurrence of blanketing Es layer (Esb) over the equatorial region during the peculiar minimum of solar cycle 24 en_US
dc.type Article en_US
dc.identifier.accession 091397


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