Investigation of the response of equatorial MLTI region during a partial solar eclipse through ground-based daytime optical technique

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dc.contributor.author Vineeth, C.
dc.contributor.author Pant, T.K.
dc.contributor.author Thampi, Smitha V.
dc.contributor.author Sridharan, R.
dc.contributor.author Ravindran, Sudha
dc.contributor.author Devasia, C.V.
dc.contributor.author Kumar, K. Kishore
dc.contributor.author Alex, S.
dc.date.accessioned 2015-09-11T11:28:16Z
dc.date.accessioned 2021-02-12T09:23:50Z
dc.date.available 2015-09-11T11:28:16Z
dc.date.available 2021-02-12T09:23:50Z
dc.date.issued 2008
dc.identifier.citation Journal of Geophysical Research, v.113, A03302, 2008, doi: 10.1029/2007JA012335 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/391
dc.description.abstract [1] First experimental evidence for solar eclipse induced changes in the equatorial mesopause and the thermosphere ionosphere regions using daytime optical photometer is presented. The photometer was operated in scanning mode to probe the thermosphere and mesopause regions simultaneously in North-South direction over Trivandrum (8.5°N; 77°E; dip lat. 0.5°N) during a partial solar eclipse event on 03 October 2005. This provided a unique data set of thermosphere and mesopause regions over a horizontal distance of 600 and 240 km respectively from zenith during this event. The striking feature observed during the eclipse is the enhancement in the thermospheric O(1D) 630 nm dayglow intensity and its equatorward movement. Another noteworthy observation is an overall enhancement in the mesopause temperature, more pronounced (∼25–30 K) over zenith. These observations are discussed in context of the vertical coupling of the mesopause with thermosphere-ionosphere region. en_US
dc.language.iso en en_US
dc.subject Equatorial MLTI en_US
dc.subject Equatorial mesopause en_US
dc.subject Thermosphere ionosphere en_US
dc.subject PSMOS en_US
dc.subject MLTI en_US
dc.title Investigation of the response of equatorial MLTI region during a partial solar eclipse through ground-based daytime optical technique en_US
dc.type Article en_US
dc.identifier.accession 090886


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