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dc.contributor.authorSridharan, S.
dc.contributor.authorGurubaran, S.
dc.contributor.authorRajaram, R.
dc.date.accessioned2015-08-25T10:56:54Z
dc.date.accessioned2021-02-12T09:27:44Z-
dc.date.available2015-08-25T10:56:54Z
dc.date.available2021-02-12T09:27:44Z-
dc.date.issued2003
dc.identifier.citationEarth, Planets Space, v.55/11, p.687-696, 2003, doi: 10.1186/BF0335247en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/285-
dc.description.abstractMF radar observations of hourly mean zonal and meridional winds at 86 km over Tirunelveli (8.7°N, 77.8°E), India, over a period of five years (1993–1997) are utilized to study the possible influence of stratospheric quasibiennial oscillation (QBO) on the vertical propagation of planetary-scale waves. The radiosonde winds at Singapore are used to identify the phase of the stratospheric QBO at 30 hPa. The study reflects that the interannual variability of the planetary waves may be explained partly by the direction of the stratospheric QBO winds. Limitations of the present work are: (i) the QBO cycles considered are not many and (ii) the observed waves are presumed to originate from below and propagate through the stratospheric QBO wind system.en_US
dc.language.isoenen_US
dc.subjectQBOen_US
dc.subjectPlanetary wavesen_US
dc.subjectMesosphereen_US
dc.subjectMLT regionen_US
dc.subjectSemi-annual oscillationen_US
dc.subjectWave-mean flow interactionen_US
dc.subjectMF radaren_US
dc.subjectQuasibiennial oscillation (QBO)en_US
dc.titleQBO influences on the variability of planetary waves in the equatorial mesopause regionen_US
dc.typeArticleen_US
dc.identifier.accession090774
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