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dc.contributor.authorGurubaran, S.
dc.contributor.authorSridharan, S.
dc.contributor.authorRamkumar, T.K.
dc.contributor.authorRajaram, R.
dc.date.accessioned2015-05-21T06:38:52Z
dc.date.accessioned2021-02-12T09:56:35Z
dc.date.available2015-05-21T06:38:52Z
dc.date.available2021-02-12T09:56:35Z
dc.date.issued2001
dc.identifier.citationJournal of Atmospheric and Solar-Terrestrial Physics, v.63,p.975-985, 2001, doi: 10.1016/S1364-6826(01)00016-5en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/120
dc.description.abstractObservations of the quasi-2-day planetary wave over a period of two years with the medium frequency (MF) radar operated at Tirunelveli , India, are presented. The observational aspects of the characteristics of the wave over the low latitude station and its possible interaction with the mean wind and the diurnal tide are studied in detail. The amplitude of the 2-day wave has been observed to be larger in winter than in summer with noticeable inter-annual variability. The period of the wave varied between 46 and with a dependence on season. The vertical wavelength during large-amplitude wave bursts has been observed to be in the range of 35–. The clear anti-correlation between the diurnal tide and the quasi-2-day wave occurrences and the presence of the 16-h wave provide indications for their interaction, which might have extracted energy from the primary diurnal tide. The changes in the mean wind during the passage of the quasi-2-day wave reflect the importance of the wave in determining the mesospheric momentum budget.en_US
dc.language.isoenen_US
dc.subjectMF radaren_US
dc.subjectBaroclinic instabilityen_US
dc.subjectWave numberen_US
dc.subjectEvanescent modeen_US
dc.subjectVertical wavelengthen_US
dc.subjectWave–waveen_US
dc.subjectWave–meanflow interactionen_US
dc.titleThe mesospheric quasi-2-day wave over Tirunelveli(8.7degree N)en_US
dc.typeArticleen_US
dcterms.sourcedoi: 10.1016/S1364-6826(01)00016-5
dc.identifier.accession090625
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