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    A Deep Convection Event above the Tunuyán Valley near the Andes Mountains

    Source: Monthly Weather Review:;2004:;volume( 132 ):;issue: 009::page 2259
    Author:
    de la Torre, A.
    ,
    Daniel, V.
    ,
    Tailleux, R.
    ,
    Teitelbaum, H.
    DOI: 10.1175/1520-0493(2004)132<2259:ADCEAT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Deep convection in the Tunuyán Valley region (33°?34°S, 69°?70°W) on the eastern side of the highest peaks of the Andes Mountains is sometimes associated with damaging hail. Understanding the physical mechanisms responsible for the occurrence of deep convection in that region is therefore a central part of the development of hail suppression projects. In this paper, a case of deep convection that occurred on 22 January 2001 is studied in detail through a combined analysis of radar, satellite, and radiosonde data and numerical simulations using a nonhydrostatic mesoscale atmospheric (Meso-NH) model. The time evolution and stability characteristics are first documented using the data. In order to get insight into the main causes for the deep convection event, numerical simulations of that day were performed. These results are compared with the results corresponding to conditions of 4 January 2001 when no deep convection occurred. The comparison between the 2 days strongly suggests that the deep convection event occurred because of the simultaneous presence of anabatic winds, accumulation of moist enthalpy, and the stability conditions. The present results should be helpful in designing future observational programs in the region.
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      A Deep Convection Event above the Tunuyán Valley near the Andes Mountains

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4205442
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    • Monthly Weather Review

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    contributor authorde la Torre, A.
    contributor authorDaniel, V.
    contributor authorTailleux, R.
    contributor authorTeitelbaum, H.
    date accessioned2017-06-09T16:15:38Z
    date available2017-06-09T16:15:38Z
    date copyright2004/09/01
    date issued2004
    identifier issn0027-0644
    identifier otherams-64339.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4205442
    description abstractDeep convection in the Tunuyán Valley region (33°?34°S, 69°?70°W) on the eastern side of the highest peaks of the Andes Mountains is sometimes associated with damaging hail. Understanding the physical mechanisms responsible for the occurrence of deep convection in that region is therefore a central part of the development of hail suppression projects. In this paper, a case of deep convection that occurred on 22 January 2001 is studied in detail through a combined analysis of radar, satellite, and radiosonde data and numerical simulations using a nonhydrostatic mesoscale atmospheric (Meso-NH) model. The time evolution and stability characteristics are first documented using the data. In order to get insight into the main causes for the deep convection event, numerical simulations of that day were performed. These results are compared with the results corresponding to conditions of 4 January 2001 when no deep convection occurred. The comparison between the 2 days strongly suggests that the deep convection event occurred because of the simultaneous presence of anabatic winds, accumulation of moist enthalpy, and the stability conditions. The present results should be helpful in designing future observational programs in the region.
    publisherAmerican Meteorological Society
    titleA Deep Convection Event above the Tunuyán Valley near the Andes Mountains
    typeJournal Paper
    journal volume132
    journal issue9
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(2004)132<2259:ADCEAT>2.0.CO;2
    journal fristpage2259
    journal lastpage2268
    treeMonthly Weather Review:;2004:;volume( 132 ):;issue: 009
    contenttypeFulltext
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