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University of Illinois at Urbana-Champaign

Idealized modeling of the role of stability and shear on mesoscale gravity wave evolution

Abstract

dc:description

Mesoscale Gravity Waves (MGWs) are large pressure perturbations that form in the presence of a stable layer at the surface either behind Mesoscale Convective Systems (MCSs) in summer or over warm frontal surfaces behind elevated convection in winter. MGWs are associated with damaging winds, moderate to heavy precipitation, and occasional heat bursts at the surface. The forcing mechanism for MGWs in this study is hypothesized to be evaporative cooling occurring behind a convective line. This evaporatively-cooled air generates a downdraft that then depresses the surface-based stable layer and causes pressure decreases, strong wind speeds and MGW genesis. Using the Weather Research and Forecast Model (WRF) version 3.0, evaporative cooling is simulated using an imposed cold thermal. Sensitivity studies examine the response of MGW structure to different thermal and shear profiles where the strength and depth of the inversion are varied, as well as the amount of wind shear. MGWs are characterized in terms of response variables, such as wind speed perturbations (U'), temperature perturbations (T'), pressure perturbations (P'), potential temperature perturbations (Θ'), and the correlation coefficient (R) between U' and P'. Regime Diagrams portray the response of MGW to the above variables in order to better understand the formation, causes, and intensity of MGWs. The results of this study indicate that shallow, weak surface layers coupled with deep, neutral layers above favor the formation of waves of elevation. Conversely, deep strong surface layers coupled with deep, neutral layers above favor the formation of waves of depression. This is also the type of atmospheric setup that tends to produce substantial surface heating at the surface.

Degree

thesis:*
Name thesis:degree_name
M.S.
Level thesis:degree_level
Thesis
Discipline thesis:degree_discipline
Atmospheric Sciences
Grantor
University of Illinois at Urbana-Champaign
Year dc:date
2010

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Pitcel, Michelle M.
Contributors dc:contributor
  • Rauber, Robert M.
  • Jewett, Brian F.
  • McFarquhar, Greg M.

Subjects

dc:subject × 6

Rights

dc:rights
Statement dc:rights
  • Copyright 2010 Michelle M. Pitcel
Language dc:language
en

Identifiers

dc:identifier.*
Handle dc:identifier
http://hdl.handle.net/2142/16155
OAI identifier oai:identifier
oai:www.ideals.illinois.edu:2142/16155

Chain of custody

source
Harvested from
University of Illinois - Urbana-Champaign
Base URL
www.ideals.illinois.edu/oai-pmh
Last updated
2026-07-22
Source record
OAI-PMH GetRecord
citation

Pitcel, Michelle M.. Idealized modeling of the role of stability and shear on mesoscale gravity wave evolution. Thesis thesis, University of Illinois at Urbana-Champaign, 2010. http://hdl.handle.net/2142/16155