A New Hypothesis for Layers of High Reflectivity Seen in MST Radar Observations

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dc.creatorAsnani, G. C.
dc.creatorRaja, M. K. Rama Varma
dc.date2000-03-14
dc.date.accessioned2026-07-07T05:43:51Z
dc.date.available2026-07-07T05:43:51Z
dc.descriptionAnalysis of MST radar observations at Gadanki (near Tirupati, India), for a period of 14 months from 1995 September to 1996 November, shows that "Clear air Turbulence" is not the primary source of high MST radar reflectivity; this conventional idea needs to be modified. An alternative hypothesis based on the microphysics and microdynamics associated with aerosols and water substance in the atmosphere, is presented here.
dc.description5 pages, Revtex
dc.identifierhttps://arxiv.org/abs/physics/0003028
dc.identifierhttp://arxiv.org/abs/physics/0003028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/83411
dc.subjectAtmospheric and Oceanic Physics
dc.titleA New Hypothesis for Layers of High Reflectivity Seen in MST Radar Observations
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