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contributor authorHeymsfield, Gerald M.
date accessioned2017-06-09T14:21:02Z
date available2017-06-09T14:21:02Z
date copyright1979/11/01
date issued1979
identifier issn0022-4928
identifier otherams-17786.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4153718
description abstractThis paper presents a case study of the structure of a warm frontal region as deduced from Doppler radar observations. The precipitation occurring ahead of the surface warm front was banded. The dominant precipitation bands were oriented transverse to the mid-level winds, and they were spaced ?110 km apart. It is suggested that these bands were formed by highly organized vertical circulations in a 2.5 km thick layer just above the warm frontal zone. The precipitation bands extended from this layer down to the surface. Near the surface additional circulations were produced by pressure perturbations resulting from cooling associated with melting snow. Some diagnostic calculations of ageostrophic winds, frontogenesis and vorticity production are presented. The frontogenesis calculation gives approximately a 2?4 h doubling time of the horizontal potential temperature gradient associated with the warm front, at mid-levels. The highly organized band-associated circulations suggest the importance of their inclusion in diagnostic calculations.
publisherAmerican Meteorological Society
titleDoppler Radar Study of a Warm Frontal Region
typeJournal Paper
journal volume36
journal issue11
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1979)036<2093:DRSOAW>2.0.CO;2
journal fristpage2093
journal lastpage2107
treeJournal of the Atmospheric Sciences:;1979:;Volume( 036 ):;issue: 011
contenttypeFulltext


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