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    What Controls the Mean Depth of the PBL?

    Source: Journal of Climate:;2005:;volume( 018 ):;issue: 016::page 3157
    Author:
    Medeiros, Brian
    ,
    Hall, Alex
    ,
    Stevens, Bjorn
    DOI: 10.1175/JCLI3417.1
    Publisher: American Meteorological Society
    Abstract: The depth of the planetary boundary layer (PBL) is a climatologically important quantity that has received little attention on regional to global scales. Here a 10-yr climatology of PBL depth from the University of California, Los Angeles (UCLA) atmospheric GCM is analyzed using the PBL mass budget. Based on the dominant physical processes, several PBL regimes are identified. These regimes tend to exhibit large-scale geographic organization. Locally generated buoyancy fluxes and static stability control PBL depth nearly everywhere, though convective mass flux has a large influence at tropical marine locations. Virtually all geographical variability in PBL depth can be linearly related to these quantities. While dry convective boundary layers dominate over land, stratocumulus-topped boundary layers are most common over ocean. This division of regimes leads to a dramatic land?sea contrast in PBL depth. Diurnal effects keep mean PBL depth over land shallow despite large daytime surface fluxes. The contrast arises because the large daily exchange of heat and mass between the PBL and free atmosphere over land is not present over the ocean, where mixing is accomplished by turbulent entrainment. Consistent treatment of remnant air from the deep, daytime PBL is necessary for proper representation of this diurnal behavior over land. Many locations exhibit seasonal shifts in PBL regime related to changes in PBL clouds. These shifts are controlled by seasonal variations in buoyancy flux and static stability.
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      What Controls the Mean Depth of the PBL?

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    contributor authorMedeiros, Brian
    contributor authorHall, Alex
    contributor authorStevens, Bjorn
    date accessioned2017-06-09T17:00:44Z
    date available2017-06-09T17:00:44Z
    date copyright2005/08/01
    date issued2005
    identifier issn0894-8755
    identifier otherams-77895.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4220503
    description abstractThe depth of the planetary boundary layer (PBL) is a climatologically important quantity that has received little attention on regional to global scales. Here a 10-yr climatology of PBL depth from the University of California, Los Angeles (UCLA) atmospheric GCM is analyzed using the PBL mass budget. Based on the dominant physical processes, several PBL regimes are identified. These regimes tend to exhibit large-scale geographic organization. Locally generated buoyancy fluxes and static stability control PBL depth nearly everywhere, though convective mass flux has a large influence at tropical marine locations. Virtually all geographical variability in PBL depth can be linearly related to these quantities. While dry convective boundary layers dominate over land, stratocumulus-topped boundary layers are most common over ocean. This division of regimes leads to a dramatic land?sea contrast in PBL depth. Diurnal effects keep mean PBL depth over land shallow despite large daytime surface fluxes. The contrast arises because the large daily exchange of heat and mass between the PBL and free atmosphere over land is not present over the ocean, where mixing is accomplished by turbulent entrainment. Consistent treatment of remnant air from the deep, daytime PBL is necessary for proper representation of this diurnal behavior over land. Many locations exhibit seasonal shifts in PBL regime related to changes in PBL clouds. These shifts are controlled by seasonal variations in buoyancy flux and static stability.
    publisherAmerican Meteorological Society
    titleWhat Controls the Mean Depth of the PBL?
    typeJournal Paper
    journal volume18
    journal issue16
    journal titleJournal of Climate
    identifier doi10.1175/JCLI3417.1
    journal fristpage3157
    journal lastpage3172
    treeJournal of Climate:;2005:;volume( 018 ):;issue: 016
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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