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    High-Resolution Simulations of Lee Waves and Downslope Winds over the Sierra Nevada during T-REX IOP 6

    Source: Journal of Applied Meteorology and Climatology:;2012:;volume( 051 ):;issue: 007::page 1333
    Author:
    Sheridan, Peter
    ,
    Vosper, Simon
    DOI: 10.1175/JAMC-D-11-0207.1
    Publisher: American Meteorological Society
    Abstract: he downslope windstorm during intensive observation period (IOP) 6 was the most severe that was detected during the Terrain-Induced Rotor Experiment (T-REX) in Owens Valley in the Sierra Nevada of California. Cross sections of vertical motion in the form of a composite constructed from aircraft data spanning the depth of the troposphere are used to link the winds experienced at the surface to the changing structure of the mountain-wave field aloft. Detailed analysis of other observations allows the role played by a passing occluded front, associated with the rapid intensification (and subsequent cessation) of the windstorm, to be studied. High-resolution, nested modeling using the Met Office Unified Model (MetUM) is used to study qualitative aspects of the flow and the influence of the front, and this modeling suggests that accurate forecasting of the timing and position of both the front and strong mountaintop winds is crucial to capture the wave dynamics and accompanying windstorm. Meanwhile, far ahead of the front, simulated downslope winds are shallow and foehnlike, driven by the thermal contrast between the upstream and valley air mass. The study also highlights the difficulties of capturing the detailed interaction of weather systems with large and complex orography in numerical weather prediction.
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      High-Resolution Simulations of Lee Waves and Downslope Winds over the Sierra Nevada during T-REX IOP 6

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4216840
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    contributor authorSheridan, Peter
    contributor authorVosper, Simon
    date accessioned2017-06-09T16:48:48Z
    date available2017-06-09T16:48:48Z
    date copyright2012/07/01
    date issued2012
    identifier issn1558-8424
    identifier otherams-74598.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4216840
    description abstracthe downslope windstorm during intensive observation period (IOP) 6 was the most severe that was detected during the Terrain-Induced Rotor Experiment (T-REX) in Owens Valley in the Sierra Nevada of California. Cross sections of vertical motion in the form of a composite constructed from aircraft data spanning the depth of the troposphere are used to link the winds experienced at the surface to the changing structure of the mountain-wave field aloft. Detailed analysis of other observations allows the role played by a passing occluded front, associated with the rapid intensification (and subsequent cessation) of the windstorm, to be studied. High-resolution, nested modeling using the Met Office Unified Model (MetUM) is used to study qualitative aspects of the flow and the influence of the front, and this modeling suggests that accurate forecasting of the timing and position of both the front and strong mountaintop winds is crucial to capture the wave dynamics and accompanying windstorm. Meanwhile, far ahead of the front, simulated downslope winds are shallow and foehnlike, driven by the thermal contrast between the upstream and valley air mass. The study also highlights the difficulties of capturing the detailed interaction of weather systems with large and complex orography in numerical weather prediction.
    publisherAmerican Meteorological Society
    titleHigh-Resolution Simulations of Lee Waves and Downslope Winds over the Sierra Nevada during T-REX IOP 6
    typeJournal Paper
    journal volume51
    journal issue7
    journal titleJournal of Applied Meteorology and Climatology
    identifier doi10.1175/JAMC-D-11-0207.1
    journal fristpage1333
    journal lastpage1352
    treeJournal of Applied Meteorology and Climatology:;2012:;volume( 051 ):;issue: 007
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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