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    A Preliminary Study on the Possibility of Estimating Total Atmospheric Ozone from Satellite Measurements

    Source: Journal of the Atmospheric Sciences:;1967:;Volume( 024 ):;issue: 004::page 414
    Author:
    Dave, J. V.
    ,
    Mateer, Carlton L.
    DOI: 10.1175/1520-0469(1967)024<0414:APSOTP>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: This paper is concerned with a preliminary study of the feasibility of determining total atmospheric ozone from satellite measurements of the solar ultraviolet radiation diffusely reflected by the earth's atmosphere. The atmospheric model used is plane-stratified, and the evaluation of the radiation field takes into account all orders of Rayleigh scattering. In addition, the model provides for variations in the total amount and vertical distribution of ozone, as well as the Lambert reflectivity and pressure at the effective base of the atmosphere. The results indicate that the wavelength region in which measurements should be made lies between about 3125 and 3175 Å, if the observations are restricted to the nadir direction. Wavelengths shorter than 3125 Å do not penetrate adequately through the ozone layer and do not, therefore, contain information on total ozone content. On the other hand, wavelengths much longer than 3175 Å although they penetrate the ozone layer, in general offer rather poor sensitivity to total ozone. The accuracy of total ozone determinations, based on measurements at a single wavelength, is not likely to be better than 10% even if the intensity ratio (diffusely reflected to extraterrestrial input flux) is measured within 1%, reflectivity within 0.05, and cloud-top or surface pressure within 50 mb. More accurate determinations of surface reflectivity are essential for improving the accuracy of the total ozone determination. Measurements on a pair of wavelengths, one within the 3125?3175 Å range and the second at 3300 Å, are found to reduce the effects of reflectivity. Over a moderate range of solar zenith angle, measurements on the wavelength pair (3175, 3300,Å) will permit deduction of total ozone within 5%, provided the various quantities are determined with the above-noted accuracies. When the zenith angle of the sun exceeds about 60°, penetration of the ozone layer is incomplete and a simultaneous determination of the high level ozone distribution from measurements at still shorter wavelengths is necessary for optimum accuracy of the total ozone determination.
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      A Preliminary Study on the Possibility of Estimating Total Atmospheric Ozone from Satellite Measurements

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4150998
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    • Journal of the Atmospheric Sciences

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    contributor authorDave, J. V.
    contributor authorMateer, Carlton L.
    date accessioned2017-06-09T14:14:10Z
    date available2017-06-09T14:14:10Z
    date copyright1967/07/01
    date issued1967
    identifier issn0022-4928
    identifier otherams-15337.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150998
    description abstractThis paper is concerned with a preliminary study of the feasibility of determining total atmospheric ozone from satellite measurements of the solar ultraviolet radiation diffusely reflected by the earth's atmosphere. The atmospheric model used is plane-stratified, and the evaluation of the radiation field takes into account all orders of Rayleigh scattering. In addition, the model provides for variations in the total amount and vertical distribution of ozone, as well as the Lambert reflectivity and pressure at the effective base of the atmosphere. The results indicate that the wavelength region in which measurements should be made lies between about 3125 and 3175 Å, if the observations are restricted to the nadir direction. Wavelengths shorter than 3125 Å do not penetrate adequately through the ozone layer and do not, therefore, contain information on total ozone content. On the other hand, wavelengths much longer than 3175 Å although they penetrate the ozone layer, in general offer rather poor sensitivity to total ozone. The accuracy of total ozone determinations, based on measurements at a single wavelength, is not likely to be better than 10% even if the intensity ratio (diffusely reflected to extraterrestrial input flux) is measured within 1%, reflectivity within 0.05, and cloud-top or surface pressure within 50 mb. More accurate determinations of surface reflectivity are essential for improving the accuracy of the total ozone determination. Measurements on a pair of wavelengths, one within the 3125?3175 Å range and the second at 3300 Å, are found to reduce the effects of reflectivity. Over a moderate range of solar zenith angle, measurements on the wavelength pair (3175, 3300,Å) will permit deduction of total ozone within 5%, provided the various quantities are determined with the above-noted accuracies. When the zenith angle of the sun exceeds about 60°, penetration of the ozone layer is incomplete and a simultaneous determination of the high level ozone distribution from measurements at still shorter wavelengths is necessary for optimum accuracy of the total ozone determination.
    publisherAmerican Meteorological Society
    titleA Preliminary Study on the Possibility of Estimating Total Atmospheric Ozone from Satellite Measurements
    typeJournal Paper
    journal volume24
    journal issue4
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1967)024<0414:APSOTP>2.0.CO;2
    journal fristpage414
    journal lastpage427
    treeJournal of the Atmospheric Sciences:;1967:;Volume( 024 ):;issue: 004
    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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