An empirical model of the OI FUV dayglow from DE-1 images |
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| Institution: | 1. Southwest Research Institute, San Antonio, TX, United States;2. University of Texas San Antonio, San Antonio, TX, United States;3. Marshall Space Flight Center, Huntsville, AL, United States;4. University of Arizona, Tucson, AZ, United States;5. Reflective X-Ray Optics LLC, New York, NY, United States;6. Lawrence Berkeley National Laboratory, Berkeley, CA, United States;7. Brigham Young University, Provo, UT, United States |
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| Abstract: | A refined empirical model of the Dynamics Explorer-1 far-ultraviolet (FUV) imaging photometer’s response to Earth’s quiet time FUV dayglow has been developed for thermospheric studies. The mean photometer response is based upon FUV observations in 156 images obtained during the first five months of imager operations (September 1981–January 1982) and is determined as a function of solar and satellite zenith angles, observational azimuth and solar clock angles, and solar radio flux. Variations with each parameter are characterized and, where possible, fitted with an appropriate function. The fitted response, based on the n-th power of the cosine of the solar zenith angle, is within 10% of actual mean values at all observed solar and satellite zenith angles and is consistent with the results of a first-principles calculation. Subtraction of the model background from other DE-1 images indirectly reveals the enhancement or diminution of thermospheric O/N2 column density ratios due to transport and Joule heating effects. An analysis of summer storm-time images from the Southern Hemisphere demonstrates the use of the model in revealing these effects. The technique developed here is readily applicable to other FUV data sets. |
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