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    Nocturnal Planetary Boundary Layer Structure and Turbulence Episodes during the Project STABLE Field Program

    Source: Journal of Applied Meteorology:;1991:;volume( 030 ):;issue: 008::page 1117
    Author:
    Weber, A. H.
    ,
    Kurzeja, R. J.
    DOI: 10.1175/1520-0450(1991)030<1117:NPBLSA>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: This paper summarizes the results of meteorological and dispersion measurements during Savannah River Laboratory's Project STABLE (Stable Boundary Layer Experiment) field program. The field program took place at the Savannah River site on three nights during 12?17 April 1988. Meteorological data were collected from a 304-m tower, an array of eight 60-m towers, two sodars, a tethersonde, and a sonic anemometer. Based on the classification scheme of Kurzeja et al. (1991) the first and third nights were classified as unsteady type IV nights because of the passage of microfronts on each night. The second night exhibited a continuous level of high turbulence with a weak surface-based inversion and was classified as a steady type III night. The third night was especially interesting because of the considerable directional wind shear with height and the occurrence of two turbulent episodes. The directional shear may have been related to the passage of a high pressure center during the night. The turbulent episodes lasted from 5 to 30 min and had a horizontal extent of at least 30 km. They were preceded by cooling near the surface and a shift to lower frequencies of the Brunt-Väisälä frequency NBV. It is suggested that a decrease with time of NBV or an increase in the standard deviation of the vertical component of velocity (σw) or σw/NBV might be used to forecast the onset of turbulent episodes reaching the surface. Sulfur hexafluoride (SF6) tracer was released continuously during the experiments and measured 10?20 km downwind by a mobile continuous analyzer. The tracer transport was shown to be consistent with low-level winds on the 304-m tower, except on the third night. It was hypothesized that on the third night the spatial variability of the wind field was much more extreme than on the other nights and, hence, the winds from the 304-m tower did not reflect the true plume movement. A spatially averaged mean wind was more successful in explaining the observed horizontal plume movement. The wider-than-expected across-are concentration distribution on the third night was attributed to continuously varying shear; whereas the occasional secondary maxima in the tracer pattern were due to discontinuities in the vertical wind shear.
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      Nocturnal Planetary Boundary Layer Structure and Turbulence Episodes during the Project STABLE Field Program

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4146966
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    • Journal of Applied Meteorology

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    contributor authorWeber, A. H.
    contributor authorKurzeja, R. J.
    date accessioned2017-06-09T14:03:36Z
    date available2017-06-09T14:03:36Z
    date copyright1991/08/01
    date issued1991
    identifier issn0894-8763
    identifier otherams-11708.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4146966
    description abstractThis paper summarizes the results of meteorological and dispersion measurements during Savannah River Laboratory's Project STABLE (Stable Boundary Layer Experiment) field program. The field program took place at the Savannah River site on three nights during 12?17 April 1988. Meteorological data were collected from a 304-m tower, an array of eight 60-m towers, two sodars, a tethersonde, and a sonic anemometer. Based on the classification scheme of Kurzeja et al. (1991) the first and third nights were classified as unsteady type IV nights because of the passage of microfronts on each night. The second night exhibited a continuous level of high turbulence with a weak surface-based inversion and was classified as a steady type III night. The third night was especially interesting because of the considerable directional wind shear with height and the occurrence of two turbulent episodes. The directional shear may have been related to the passage of a high pressure center during the night. The turbulent episodes lasted from 5 to 30 min and had a horizontal extent of at least 30 km. They were preceded by cooling near the surface and a shift to lower frequencies of the Brunt-Väisälä frequency NBV. It is suggested that a decrease with time of NBV or an increase in the standard deviation of the vertical component of velocity (σw) or σw/NBV might be used to forecast the onset of turbulent episodes reaching the surface. Sulfur hexafluoride (SF6) tracer was released continuously during the experiments and measured 10?20 km downwind by a mobile continuous analyzer. The tracer transport was shown to be consistent with low-level winds on the 304-m tower, except on the third night. It was hypothesized that on the third night the spatial variability of the wind field was much more extreme than on the other nights and, hence, the winds from the 304-m tower did not reflect the true plume movement. A spatially averaged mean wind was more successful in explaining the observed horizontal plume movement. The wider-than-expected across-are concentration distribution on the third night was attributed to continuously varying shear; whereas the occasional secondary maxima in the tracer pattern were due to discontinuities in the vertical wind shear.
    publisherAmerican Meteorological Society
    titleNocturnal Planetary Boundary Layer Structure and Turbulence Episodes during the Project STABLE Field Program
    typeJournal Paper
    journal volume30
    journal issue8
    journal titleJournal of Applied Meteorology
    identifier doi10.1175/1520-0450(1991)030<1117:NPBLSA>2.0.CO;2
    journal fristpage1117
    journal lastpage1133
    treeJournal of Applied Meteorology:;1991:;volume( 030 ):;issue: 008
    contenttypeFulltext
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