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    On the Information Content of Umkehr Observations 

    Source: Journal of the Atmospheric Sciences:;1965:;Volume( 022 ):;issue: 004:;page 370
    Author(s): Mateer, Carlton L.
    Publisher: American Meteorological Society
    Abstract: Principal component analysis has been used to determine the number of linearly independent pieces of information that may be inferred from Umkehr observations. The analysis indicates that there are at most four such pieces ...
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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(s): Dave, J. V.; Mateer, Carlton L.
    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 ...
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    On the Application of the Optimum Statistical Inversion Technique to the Evaluation of Umkehr Observations 

    Source: Journal of Applied Meteorology:;1971:;volume( 010 ):;issue: 002:;page 328
    Author(s): Deluisi, John J.; Mateer, Carlton L.
    Publisher: American Meteorological Society
    Abstract: The optimum statistical inversion technique is applied to the evaluation of Umkehr observations from Arosa (46.5N, 9.4E), Aspendale (38.0S, 145.IE) and Tallahassee (30.2N, 84.2W). A Priori statistical information on the ...
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    Estimation of Total Ozone from Satellite Measurements of Backscattered Ultraviolet Earth Radiance 

    Source: Journal of the Atmospheric Sciences:;1971:;Volume( 028 ):;issue: 007:;page 1307
    Author(s): Mateer, Carlton L.; Heath, Donald F.; Krueger, Arlin J.
    Publisher: American Meteorological Society
    Abstract: Total ozone is estimated from Nimbus IV satellite measurements of the attenuation of backscattered radiances at wavelengths between 3100 and 3400 Å. A measurement of the backscattered radiance at 3800 Å, outside the O3 ...
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