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dc.contributor.authorSridharan, S.
dc.contributor.authorPrasanth, P. Vishnu
dc.contributor.authorKumar, Y. Bhavani
dc.contributor.authorRamkumar, Geetha
dc.contributor.authorSathishkumar, S.
dc.contributor.authorRaghunath, K.
dc.date.accessioned2015-10-26T09:11:51Z
dc.date.accessioned2021-02-12T09:35:52Z-
dc.date.available2015-10-26T09:11:51Z
dc.date.available2021-02-12T09:35:52Z-
dc.date.issued2009
dc.identifier.citationJournal of Atmospheric and Solar-Terrestrial Physics, v.71, p.575–582, 2009, doi: 10.1016/j.jastp.2008.12.002en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/641-
dc.description.abstractResonance lidar observations of sodium density in the upper mesosphere region over Gadanki (13.5°N, 79.2°E) rarely show complex structures with rapid enhancements of sodium density, completely different from normal sporadic sodium structures. The hourly averaged meteor radar zonal winds over Trivandrum (8.5°N, 76.5°E) show an eastward shear with altitude during the nights, when these events are formed. As suggested by Kane et al. [2001. Joint observations of sodium enhancements and field-aligned ionospheric irregularities. Geophysical Research Letters 28, 1375–1378], our observations show that the complex structures may be formed due to Kelvin–Helmholtz instability, which can occur in the region of strong wind shear.en_US
dc.language.isoenen_US
dc.subjectResonance lidaren_US
dc.subjectSporadic sodium layersen_US
dc.subjectMeteor radaren_US
dc.subjectWind shearen_US
dc.subjectSodium densityen_US
dc.titleObservations of peculiar sporadic sodium structures and their relation with wind variationsen_US
dc.typeArticleen_US
dc.identifier.accession091303
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