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Observations of a midlatitude squall line boundary layer wake

dc.contributor.authorHamilton, Paul J., author
dc.contributor.authorJohnson, Richard H. (Richard Harlan), author
dc.contributor.authorDepartment of Atmospheric Science, Colorado State University, publisher
dc.date.accessioned2016-07-26T13:52:27Z
dc.date.available2016-07-26T13:52:27Z
dc.date.issued1987
dc.descriptionIncludes bibliographical references (pages 90-93).
dc.descriptionJune 1987.
dc.description.abstractMesoscale pressure perturbations frequently observed with mesoscale convective systems (MCS) are examined with special emphasis on the characteristics, structure, lifecycle and driving mechanism of the "wake depression" found in the wake region of the convection. A severe squall line which traversed the OK PRE-STORM surface and upper air mesonetwork on 10-11 June 1985 is the focus of this observational study. Extensive surface, upper air and digitized radar data collected during the OK PRE-STORM field experiment were used for analysis. Various mesoanalyses of this squall line at the surface and aloft have allowed for intensive examination of three pressure features observed with this squall line: the mesohigh, wake depression and pre-squall mesolow. Their relationship to and interaction with other meteorological parameters such as precipitation, temperature, potential temperature and moisture are explored. Furthermore, the mesoscale system-relative "jets" observed with midlatitude squall lines are examined for their possible influence on the pressure field. The mesohigh develops quickly during the early growth of the squall line and precedes the wake depression by several hours. The predominant mesohigh is linked to the formation of a large cold pool which developed as a result of widespread hail and intense rainfall from a supercell ahead of the young squall line. Analyses show that the wake depression is not a uniform, stagnant feature behind the mesohigh but has embedded small-scale features, a distinct lifecycle and can undergo rapid intensification. The wake depression also is related to some aspects of the squall line's precipitation pattern. The low consistently "hugs" the back edge of the stratiform precipitation and is observed to split into two separate lows as the convective line splits. Additionally, the wake depression is a hydrostatic response to a layer of warm, dry air (produced by subsidence) found just above the surface. It is suggested that the wake depression is in part a surface manifestation of forced subsidence by the descending rear inflow jet.
dc.description.sponsorshipSponsored by the National Science Foundation - ATM-8507961.
dc.format.mediumreports
dc.identifier.urihttp://hdl.handle.net/10217/176167
dc.languageEnglish
dc.language.isoeng
dc.publisherColorado State University. Libraries
dc.relationCatalog record number (MMS ID): 991023639799703361
dc.relationQC852.C6 no.414
dc.relation.ispartofAtmospheric Science Papers (Blue Books)
dc.relation.ispartofAtmospheric science paper, no. 414
dc.rightsCopyright and other restrictions may apply. User is responsible for compliance with all applicable laws. For information about copyright law, please see https://libguides.colostate.edu/copyright.
dc.subject.lcshSquall lines
dc.subject.lcshBoundary layer (Meteorology)
dc.titleObservations of a midlatitude squall line boundary layer wake
dc.typeText
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