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    Ship-Based Sun Photometer Measurements Using Microtops Sun Photometers

    Source: Journal of Atmospheric and Oceanic Technology:;2001:;volume( 018 ):;issue: 005::page 765
    Author:
    Porter, John N.
    ,
    Miller, Mark
    ,
    Pietras, Christophe
    ,
    Motell, Craig
    DOI: 10.1175/1520-0426(2001)018<0765:SBSPMU>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The use of hand-held Microtops II sun photometers (built by Solar Light Inc.) on ship platforms is discussed. Their calibration, filter stability, and temperature effects are also described. It is found that under rough conditions, the ship motion causes the largest error, which can result in a bias toward higher optical depths. In order to minimize this bias, a large number of sun photometer measurements (?25) should be taken in a short period of time, and the higher values should be discarded. Under rough ocean conditions, it is also best to shorten the Microtops sun photometer sampling period (less than 5 s) and save only a single value (no averaging) and remove the high optical depths in postprocessing. It is found that the Microtops should be turned off frequently to correct for zero drift caused by temperature effects. Calibration is maintained by routine Langley plot calibrations at the Mauna Loa Observatory for each unit or through cross calibration.
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      Ship-Based Sun Photometer Measurements Using Microtops Sun Photometers

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4154467
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    • Journal of Atmospheric and Oceanic Technology

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    contributor authorPorter, John N.
    contributor authorMiller, Mark
    contributor authorPietras, Christophe
    contributor authorMotell, Craig
    date accessioned2017-06-09T14:23:29Z
    date available2017-06-09T14:23:29Z
    date copyright2001/05/01
    date issued2001
    identifier issn0739-0572
    identifier otherams-1846.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4154467
    description abstractThe use of hand-held Microtops II sun photometers (built by Solar Light Inc.) on ship platforms is discussed. Their calibration, filter stability, and temperature effects are also described. It is found that under rough conditions, the ship motion causes the largest error, which can result in a bias toward higher optical depths. In order to minimize this bias, a large number of sun photometer measurements (?25) should be taken in a short period of time, and the higher values should be discarded. Under rough ocean conditions, it is also best to shorten the Microtops sun photometer sampling period (less than 5 s) and save only a single value (no averaging) and remove the high optical depths in postprocessing. It is found that the Microtops should be turned off frequently to correct for zero drift caused by temperature effects. Calibration is maintained by routine Langley plot calibrations at the Mauna Loa Observatory for each unit or through cross calibration.
    publisherAmerican Meteorological Society
    titleShip-Based Sun Photometer Measurements Using Microtops Sun Photometers
    typeJournal Paper
    journal volume18
    journal issue5
    journal titleJournal of Atmospheric and Oceanic Technology
    identifier doi10.1175/1520-0426(2001)018<0765:SBSPMU>2.0.CO;2
    journal fristpage765
    journal lastpage774
    treeJournal of Atmospheric and Oceanic Technology:;2001:;volume( 018 ):;issue: 005
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
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