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    A Tropical Squall Line Observed during TOGA COARE: Extended Comparisons between Simulations and Doppler Radar Data and the Role of Midlevel Wind Shear

    Source: Monthly Weather Review:;2000:;volume( 128 ):;issue: 011::page 3709
    Author:
    Montmerle, Thibaut
    ,
    Lafore, Jean-Philippe
    ,
    Redelsperger, Jean-Luc
    DOI: 10.1175/1520-0493(2001)129<3709:ATSLOD>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Results from a three-dimensional cloud model are extensively compared with airborne Doppler radar data in the case of a tropical oceanic squall line observed during the Tropical Ocean Global Atmosphere Coupled Ocean?Atmosphere Response Experiment. The comparison is based on the precipitation patterns, the dynamical and thermodynamical distributions, and the vertical transport of horizontal momentum. The model simulates the evolution of the mesoscale convective system (MCS) frontal convective line from a quasi-linear to a broken pattern. The area located south of the ?break,? which designates the region where the MCS leading edge reorientates from the N?S to the E?W direction, is composed of a pronounced bow-shaped structure with two vortices located on both sides of a strong rear inflow. The vertical circulation is characterized by a jump updraft and an overturning downdraft. Both structures exhibit a vertical, intense updraft in the break zone, whereas the jump updraft is more sloped and less intense in the bow region. Front-to-rear momentum is injected mainly by the jump updraft. Both observations and simulation indicate the major role played by convective eddies in the vertical transport of cross-line and parallel-line horizontal momentum. A synthesis summarizes the complex three-dimensional structure of the simulated system, based on three salient features and their relative locations: the deep convection region, the leading edge of the cold pool, and the melting area. The relative positions between the two last mentioned explains the observed asymmetric structure and the existence of more upright and narrow updrafts in the northern part of the system. Numerical experiments suggest that the wind profile at midlevel is mainly responsible for the location of the melting area relative to the cold pool. The system tends to generate new convective elements organized along the direction that reduces the angle between the convective line and the midlevel shear vector.
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      A Tropical Squall Line Observed during TOGA COARE: Extended Comparisons between Simulations and Doppler Radar Data and the Role of Midlevel Wind Shear

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4204895
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    • Monthly Weather Review

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    contributor authorMontmerle, Thibaut
    contributor authorLafore, Jean-Philippe
    contributor authorRedelsperger, Jean-Luc
    date accessioned2017-06-09T16:14:05Z
    date available2017-06-09T16:14:05Z
    date copyright2000/11/01
    date issued2000
    identifier issn0027-0644
    identifier otherams-63847.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4204895
    description abstractResults from a three-dimensional cloud model are extensively compared with airborne Doppler radar data in the case of a tropical oceanic squall line observed during the Tropical Ocean Global Atmosphere Coupled Ocean?Atmosphere Response Experiment. The comparison is based on the precipitation patterns, the dynamical and thermodynamical distributions, and the vertical transport of horizontal momentum. The model simulates the evolution of the mesoscale convective system (MCS) frontal convective line from a quasi-linear to a broken pattern. The area located south of the ?break,? which designates the region where the MCS leading edge reorientates from the N?S to the E?W direction, is composed of a pronounced bow-shaped structure with two vortices located on both sides of a strong rear inflow. The vertical circulation is characterized by a jump updraft and an overturning downdraft. Both structures exhibit a vertical, intense updraft in the break zone, whereas the jump updraft is more sloped and less intense in the bow region. Front-to-rear momentum is injected mainly by the jump updraft. Both observations and simulation indicate the major role played by convective eddies in the vertical transport of cross-line and parallel-line horizontal momentum. A synthesis summarizes the complex three-dimensional structure of the simulated system, based on three salient features and their relative locations: the deep convection region, the leading edge of the cold pool, and the melting area. The relative positions between the two last mentioned explains the observed asymmetric structure and the existence of more upright and narrow updrafts in the northern part of the system. Numerical experiments suggest that the wind profile at midlevel is mainly responsible for the location of the melting area relative to the cold pool. The system tends to generate new convective elements organized along the direction that reduces the angle between the convective line and the midlevel shear vector.
    publisherAmerican Meteorological Society
    titleA Tropical Squall Line Observed during TOGA COARE: Extended Comparisons between Simulations and Doppler Radar Data and the Role of Midlevel Wind Shear
    typeJournal Paper
    journal volume128
    journal issue11
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(2001)129<3709:ATSLOD>2.0.CO;2
    journal fristpage3709
    journal lastpage3730
    treeMonthly Weather Review:;2000:;volume( 128 ):;issue: 011
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian