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    Diabatically Driven Discrete Propagation of Surface Fronts: A Numerical Analysis

    Source: Journal of the Atmospheric Sciences:;2000:;Volume( 057 ):;issue: 013::page 2061
    Author:
    Bryan, George H.
    ,
    Fritsch, J. Michael
    DOI: 10.1175/1520-0469(2000)057<2061:DDDPOS>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Discrete frontal propagation has been identified as a process whereby a surface front discontinuously moves forward, without evidence of frontal passage across a mesoscale region. Numerical simulations are employed to examine the upper-level evolution of a discrete frontal propagation event and to explore the processes that were responsible for the discrete movement. Model results indicate that a frontal pressure trough was not able to penetrate through a deep surface-based layer of cool air created by a precipitating convective system several hundred kilometers in advance of the front. Meanwhile, a new low-level baroclinic zone formed well ahead of the front along the southern side of the cool layer. As the midlevel front moved continuously over the cool layer, a new low-level front developed in the new baroclinic zone and the original low-level front dissipated. At the surface, the simulated front did not pass through the cool layer. Frontogenesis terms reveal that the prefrontal circulation that becomes the new frontal circulation initially forms directly from diabatic frontogenesis. Daytime heating in the prefrontal boundary layer and cooling from thunderstorms combine to create a thermal gradient and a mesoscale pressure perturbation. Winds turn in response to the altered pressure field and form a convergent boundary, resulting in kinematic frontogenesis. The boundary subsequently undergoes rapid intensification. Sensitivity studies were conducted in which latent heating due to precipitation was withheld and the influence of clouds on the radiation scheme was ignored. In a simulation with both of these effects withheld, the original front passes continuously through the region, that is, there is no discrete propagation. Thus, diabatic processes associated with a large complex of thunderstorms were necessary to induce the discrete frontal propagation in this case. This conclusion contrasts with previous studies, where fronts were observed to propagate discretely in dry environments.
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      Diabatically Driven Discrete Propagation of Surface Fronts: A Numerical Analysis

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4159109
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    contributor authorBryan, George H.
    contributor authorFritsch, J. Michael
    date accessioned2017-06-09T14:36:19Z
    date available2017-06-09T14:36:19Z
    date copyright2000/07/01
    date issued2000
    identifier issn0022-4928
    identifier otherams-22637.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159109
    description abstractDiscrete frontal propagation has been identified as a process whereby a surface front discontinuously moves forward, without evidence of frontal passage across a mesoscale region. Numerical simulations are employed to examine the upper-level evolution of a discrete frontal propagation event and to explore the processes that were responsible for the discrete movement. Model results indicate that a frontal pressure trough was not able to penetrate through a deep surface-based layer of cool air created by a precipitating convective system several hundred kilometers in advance of the front. Meanwhile, a new low-level baroclinic zone formed well ahead of the front along the southern side of the cool layer. As the midlevel front moved continuously over the cool layer, a new low-level front developed in the new baroclinic zone and the original low-level front dissipated. At the surface, the simulated front did not pass through the cool layer. Frontogenesis terms reveal that the prefrontal circulation that becomes the new frontal circulation initially forms directly from diabatic frontogenesis. Daytime heating in the prefrontal boundary layer and cooling from thunderstorms combine to create a thermal gradient and a mesoscale pressure perturbation. Winds turn in response to the altered pressure field and form a convergent boundary, resulting in kinematic frontogenesis. The boundary subsequently undergoes rapid intensification. Sensitivity studies were conducted in which latent heating due to precipitation was withheld and the influence of clouds on the radiation scheme was ignored. In a simulation with both of these effects withheld, the original front passes continuously through the region, that is, there is no discrete propagation. Thus, diabatic processes associated with a large complex of thunderstorms were necessary to induce the discrete frontal propagation in this case. This conclusion contrasts with previous studies, where fronts were observed to propagate discretely in dry environments.
    publisherAmerican Meteorological Society
    titleDiabatically Driven Discrete Propagation of Surface Fronts: A Numerical Analysis
    typeJournal Paper
    journal volume57
    journal issue13
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(2000)057<2061:DDDPOS>2.0.CO;2
    journal fristpage2061
    journal lastpage2079
    treeJournal of the Atmospheric Sciences:;2000:;Volume( 057 ):;issue: 013
    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