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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2997
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dc.contributor.authorRao, H. N. R-
dc.contributor.authorSastri, J. H-
dc.date.accessioned2008-08-04T11:27:00Z-
dc.date.available2008-08-04T11:27:00Z-
dc.date.issued1994-04-
dc.identifier.citationAnnales Geophysicae-Atmospheres Hydrospheres and Space Sciences, Vol. 12, No. 2 – 3, pp. 276 - 278en
dc.identifier.issn0992-7689-
dc.identifier.urihttp://hdl.handle.net/2248/2997-
dc.descriptionRestricted Access-
dc.description.abstractWe present the first results on the characteristics of the equatorial midnight temperature maximum (MTM) for the Indian sector. The results are based on measurements of the Doppler width of 630 nm night airglow emission at Kavalur (12.5° N, dip ∼ 9.5° N) during March-April 1992 and Nov 1992-April 1993. Clear evidence for MTM is found on ∼ 30 per cent of the nights at Kavalur. The MTM occurs, on the average, one hour after midnight in local winter and just before midnight in vernal equinox, a seasonal pattern that is in broad agreement with that at Jicamarca (12° S, dip 2° N) in the American sector. The MTM amplitude at Kavalur is in general larger than that at Jicamarca.en
dc.format.extent3894 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherINIST-CNRSen
dc.subjectEquatorial Ionosphereen
dc.subjectIonospheric F Regionen
dc.subjectNeutral Particle Temperatureen
dc.subjectMaximum Temperatureen
dc.subjectIndiaen
dc.subjectAsiaen
dc.titleCharacteristics of the equatorial midnight temperature maximum in the Indian sectoren
dc.typeArticleen
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