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

dc.contributor.authorVineeth, C.
dc.contributor.authorPant, T.K.
dc.contributor.authorThampi, Smitha V.
dc.contributor.authorSridharan, R.
dc.contributor.authorRavindran, Sudha
dc.contributor.authorDevasia, C.V.
dc.contributor.authorKumar, K. Kishore
dc.contributor.authorAlex, S.
dc.date.accessioned2015-09-11T11:28:16Z
dc.date.accessioned2021-02-12T09:23:50Z
dc.date.available2015-09-11T11:28:16Z
dc.date.available2021-02-12T09:23:50Z
dc.date.issued2008
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.identifier.accession090886
dc.identifier.citationJournal of Geophysical Research, v.113, A03302, 2008, doi: 10.1029/2007JA012335en_US
dc.identifier.urihttp://library.iigm.res.in:4000/handle/123456789/391
dc.language.isoenen_US
dc.subjectEquatorial MLTIen_US
dc.subjectEquatorial mesopauseen_US
dc.subjectThermosphere ionosphereen_US
dc.subjectPSMOSen_US
dc.subjectMLTIen_US
dc.titleInvestigation of the response of equatorial MLTI region during a partial solar eclipse through ground-based daytime optical techniqueen_US
dc.typeArticleen_US

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