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    Elevated Potential Instability in the Comma Head: Distribution and Development

    Source: Monthly Weather Review:;2018:;volume 146:;issue 004::page 1259
    Author:
    Rosenow, Andrew A.
    ,
    Rauber, Robert M.
    ,
    Jewett, Brian F.
    ,
    McFarquhar, Greg M.
    ,
    Keeler, Jason M.
    DOI: 10.1175/MWR-D-17-0283.1
    Publisher: American Meteorological Society
    Abstract: AbstractThe development of elevated potential instability within the comma head of a continental winter cyclone over the north-central United States is examined using a 63-h Weather Research and Forecasting (WRF) Model simulation. The simulation is first compared to the observed cyclone. The distribution of most unstable convective available potential energy (MUCAPE) within the comma head is then analyzed. The region with positive MUCAPE was based from 2- to 4-km altitude with MUCAPE values up to 93 J kg?1. Backward trajectories from five sublayers within the region of elevated convection in the comma head were calculated to investigate how elevated potential instability developed. Air in the lowest sublayer, the source air for convective cells, originated 63 h earlier near Baja California at elevations between 2.25- and 2.75-km altitude. Air atop the layer where convection occurred originated at altitudes between 9.25 and 9.75 km in the Arctic, 5000 km away from the origin of air in the lowest sublayer. All air in the layer in which convection occurred originated over the Pacific coast of Mexico, the Pacific Ocean, or arctic regions of Canada. Diabatic processes strongly influenced air properties during transit to the comma head. Air underwent radiative cooling, was affected by mixing during passage over mountains, and underwent interactions with clouds and precipitation. Notably, no trajectory followed an isentropic surface during the transit. The changes in thermodynamic properties along the trajectories led to an arrangement of air masses in the comma head that promoted the development of potential instability and elevated convection.
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      Elevated Potential Instability in the Comma Head: Distribution and Development

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4261242
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    • Monthly Weather Review

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    contributor authorRosenow, Andrew A.
    contributor authorRauber, Robert M.
    contributor authorJewett, Brian F.
    contributor authorMcFarquhar, Greg M.
    contributor authorKeeler, Jason M.
    date accessioned2019-09-19T10:04:30Z
    date available2019-09-19T10:04:30Z
    date copyright3/14/2018 12:00:00 AM
    date issued2018
    identifier othermwr-d-17-0283.1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4261242
    description abstractAbstractThe development of elevated potential instability within the comma head of a continental winter cyclone over the north-central United States is examined using a 63-h Weather Research and Forecasting (WRF) Model simulation. The simulation is first compared to the observed cyclone. The distribution of most unstable convective available potential energy (MUCAPE) within the comma head is then analyzed. The region with positive MUCAPE was based from 2- to 4-km altitude with MUCAPE values up to 93 J kg?1. Backward trajectories from five sublayers within the region of elevated convection in the comma head were calculated to investigate how elevated potential instability developed. Air in the lowest sublayer, the source air for convective cells, originated 63 h earlier near Baja California at elevations between 2.25- and 2.75-km altitude. Air atop the layer where convection occurred originated at altitudes between 9.25 and 9.75 km in the Arctic, 5000 km away from the origin of air in the lowest sublayer. All air in the layer in which convection occurred originated over the Pacific coast of Mexico, the Pacific Ocean, or arctic regions of Canada. Diabatic processes strongly influenced air properties during transit to the comma head. Air underwent radiative cooling, was affected by mixing during passage over mountains, and underwent interactions with clouds and precipitation. Notably, no trajectory followed an isentropic surface during the transit. The changes in thermodynamic properties along the trajectories led to an arrangement of air masses in the comma head that promoted the development of potential instability and elevated convection.
    publisherAmerican Meteorological Society
    titleElevated Potential Instability in the Comma Head: Distribution and Development
    typeJournal Paper
    journal volume146
    journal issue4
    journal titleMonthly Weather Review
    identifier doi10.1175/MWR-D-17-0283.1
    journal fristpage1259
    journal lastpage1278
    treeMonthly Weather Review:;2018:;volume 146:;issue 004
    contenttypeFulltext
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