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    High-Resolution Modeling of the Cape Canaveral Area Land–Water Circulations and Associated Features

    Source: Monthly Weather Review:;1999:;volume( 127 ):;issue: 008::page 1808
    Author:
    Rao, P. Anil
    ,
    Fuelberg, Henry E.
    ,
    Droegemeier, Kelvin K.
    DOI: 10.1175/1520-0493(1999)127<1808:HRMOTC>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The Advanced Regional Prediction System is used to perform a three-dimensional numerical simulation of land?water circulations near Cape Canaveral, Florida. Three two-way nested grids having spacings of 1.6, 0.4, and 0.1 km are employed. Results show that the structures of both the sea and river breezes compare well with observation and theory. Horizontal convective rolls (HCRs), Kelvin?Helmholtz instability (KHI), and their interactions with the sea and river breezes also are investigated. HCRs form over the heated land surface at periodic intervals. The HCRs have two preferred spatial scales: large and small. Inclusion of both the large and small HCRs yields aspect ratios that are smaller than most previous observations. However, when considering only the larger HCRs, agreement is better. The smaller HCRs eventually dissipate or merge with their larger HCR counterparts. These mergers intensify the vertical motion within the larger circulations. The HCRs are observed to tilt upward in advance of the Indian River breeze (IRB), and then advect over and behind the land?water circulation. There is evidence that an HCR advects 2.5 km behind the surface front. The orientation of the IRB causes its interaction with an HCR to change from an intersection to a merger. This produces positive vertical vorticity that causes the IRB to rotate counterclockwise. The detailed physiography and surface characteristics used in this research allow these complex asymmetric interactions to be simulated. In addition, the configuration of this simulation allows an even smaller-scale feature, KHI, to be observed on top of and behind the Indian River breeze front. It appears as vortices or billows that grow in amplitude and propagate backward relative to the front. The structure of the billows agrees well with previous theoretical and modeling results. Local regions of upward motion associated with the billows may be a preferred area for postfrontal convection.
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      High-Resolution Modeling of the Cape Canaveral Area Land–Water Circulations and Associated Features

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4204340
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    contributor authorRao, P. Anil
    contributor authorFuelberg, Henry E.
    contributor authorDroegemeier, Kelvin K.
    date accessioned2017-06-09T16:12:31Z
    date available2017-06-09T16:12:31Z
    date copyright1999/08/01
    date issued1999
    identifier issn0027-0644
    identifier otherams-63347.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4204340
    description abstractThe Advanced Regional Prediction System is used to perform a three-dimensional numerical simulation of land?water circulations near Cape Canaveral, Florida. Three two-way nested grids having spacings of 1.6, 0.4, and 0.1 km are employed. Results show that the structures of both the sea and river breezes compare well with observation and theory. Horizontal convective rolls (HCRs), Kelvin?Helmholtz instability (KHI), and their interactions with the sea and river breezes also are investigated. HCRs form over the heated land surface at periodic intervals. The HCRs have two preferred spatial scales: large and small. Inclusion of both the large and small HCRs yields aspect ratios that are smaller than most previous observations. However, when considering only the larger HCRs, agreement is better. The smaller HCRs eventually dissipate or merge with their larger HCR counterparts. These mergers intensify the vertical motion within the larger circulations. The HCRs are observed to tilt upward in advance of the Indian River breeze (IRB), and then advect over and behind the land?water circulation. There is evidence that an HCR advects 2.5 km behind the surface front. The orientation of the IRB causes its interaction with an HCR to change from an intersection to a merger. This produces positive vertical vorticity that causes the IRB to rotate counterclockwise. The detailed physiography and surface characteristics used in this research allow these complex asymmetric interactions to be simulated. In addition, the configuration of this simulation allows an even smaller-scale feature, KHI, to be observed on top of and behind the Indian River breeze front. It appears as vortices or billows that grow in amplitude and propagate backward relative to the front. The structure of the billows agrees well with previous theoretical and modeling results. Local regions of upward motion associated with the billows may be a preferred area for postfrontal convection.
    publisherAmerican Meteorological Society
    titleHigh-Resolution Modeling of the Cape Canaveral Area Land–Water Circulations and Associated Features
    typeJournal Paper
    journal volume127
    journal issue8
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(1999)127<1808:HRMOTC>2.0.CO;2
    journal fristpage1808
    journal lastpage1821
    treeMonthly Weather Review:;1999:;volume( 127 ):;issue: 008
    contenttypeFulltext
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