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Evolution of balanced flow in a simulated mesoscale convective complex

dc.contributor.authorOlsson, Peter Q., author
dc.date.accessioned2022-02-24T18:45:40Z
dc.date.available2022-02-24T18:45:40Z
dc.date.issued1994-11-28
dc.descriptionNovember 28, 1994.
dc.descriptionAlso issued as author's dissertation (Ph.D.) -- Colorado State University, 1995.
dc.description.abstractMCCs, a phenomenon occurring worldwide, by definition share certain structural and tem­poral features. Beyond the definition criteria, however, MCCs typically show a common organizational structure and evolution which cannot be directly attributed to the environ­ment in which they evolve. This suggests that their evolution is governed by a set of phys­ical laws which apply similarly to ensemble convective heating in a variety of mesoscale environments. In the middle latitudes, MCCs represent the extreme case of a large-amplitude energetic perturbation to the background environment. While substantial transients and observed, a separate class of non-radiating, balanced motions also evolve. These motions, and the altered thermal structure which balances them, are conveniently contained in a single quantity, the PV. The work described herein is an effort to understand the evolution of these balanced motions. To this end, a primitive equation (PE) numerical simulation of an MCC was per­formed. To isolate the balanced flow, a diagnostic system based on nonlinear balance is derived and discussed. This system is used to invert the PV and recover the rotational com­ponent of the balanced motion and the balanced mass field. A further application of the NLB approximation results in a diagnostic equation for the vertical velocity and, as well, a method for diagnosing the horizontal divergent motions which are "slaved" to it by the constraint of continuity. The PE simulation discussed herein agrees well with observations and produces many of the features frequently associated with MCCs including mesoscale convectively-induced vortices in the lower troposphere and a large anticyclone at upper levels. The nondivergent component of the PE model winds is found to consist, to a great degree, of balanced flow. More surprisingly, the storm-induced divergent model winds also remain reasonably bal­anced, though certainly less so than the nondivergent flow. The good agreement between model and balanced upward vertical mass flux suggests that the bulk of the three-dimen­sional unbalanced divergent motion may be attributed to gravity waves. The greatest dis­parity between the model and balanced circulations is found in the downward vertical motion, suggesting that the process of mass adjustment due to convective heating is largely dominated by unbalanced fast-manifold processes.
dc.description.sponsorshipSponsored by the National Science Foundation under grant ATM-9118963.
dc.format.mediumreports
dc.identifier.urihttps://hdl.handle.net/10217/234408
dc.languageEnglish
dc.language.isoeng
dc.publisherColorado State University. Libraries
dc.relationCatalog record number (MMS ID): 991023933819703361
dc.relationQC852 .C6 no. 570
dc.relation.ispartofAtmospheric Science Papers (Blue Books)
dc.relation.ispartofAtmospheric science paper, no. 570
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.subjectConvection (Meteorology)
dc.subjectAtmospheric circulation
dc.titleEvolution of balanced flow in a simulated mesoscale convective complex
dc.typeText
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