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    Characterization of the Nimbus-7 SBUV Radiometer for the Long-Term Monitoring of Stratospheric Ozone 

    Source: Journal of Atmospheric and Oceanic Technology:;1988:;volume( 005 ):;issue: 002:;page 215
    Author(s): Cebula, R. P.; Park, H.; Heath, D. F.
    Publisher: American Meteorological Society
    Abstract: Precise knowledge of in-orbit sensitivity change is critical for the successful monitoring of stratosphere ozone by satellite-based remote sensors. This paper evaluates those aspects of the in-flight operation that influence ...
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    Instrument Characterization for the Detection of Long-term Changes in Stratospheric Ozone: An Analysis of the SBUY/2 Radiometer 

    Source: Journal of Atmospheric and Oceanic Technology:;1986:;volume( 003 ):;issue: 003:;page 472
    Author(s): Frederick, S. E.; Cebula, R. P.; Heath, D. F.
    Publisher: American Meteorological Society
    Abstract: The scientific objective of unambiguously detecting subtle global trends in upper stratospheric ozone requires that one maintain a thorough understanding of the satellite-based remote sensors intended for this task. The ...
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    Total Ozone Variations 1970-74 Using Backscattered Ultraviolet (BUV) and Ground-Based Observations 

    Source: Journal of Applied Meteorology:;1982:;volume( 021 ):;issue: 005:;page 621
    Author(s): Miller, A. J.; Nagatani, R. M.; Rogers, T. G.; Fleig, A. J.; Heath, D. F.
    Publisher: American Meteorological Society
    Abstract: The most long-lived satellite set of ozone observations, to date, is that derived from the Backscatter Ultraviolet (BUV) ozone sensor on Nimbus 4 and extends from April 1970 through 1976. Unfortunately, this experiment ...
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    Ozone Abundances in the Lower Mesosphere Deduced from Backscattered Solar Radiances 

    Source: Journal of the Atmospheric Sciences:;1977:;Volume( 034 ):;issue: 012:;page 1987
    Author(s): Frederick, J. E.; Hays, P. B.; Guenther, B. W.; Heath, D. F.
    Publisher: American Meteorological Society
    Abstract: Backscatter ultraviolet data obtained by the Explorer E satellite imply very large ozone column abundances above 56 km in the tropics during mid-day. The number of molecules in a vertical column decays by a factor of 2?3 ...
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