We describe the specifications for an ultraviolet radiometer for measuring the F-region electron density gradients from the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC). We also present a technique for determining the two-dimensional structure of the ionosphere using the measured ionospheric gradients inferred from observation of the radiative recombination emission at 1356 A in conjunction with occultations of Global Positioning System satellites observed from the COSMIC satellites. Our scheme uses a nadir viewing UV photometer to characterize the F-region gradients while obtaining altitude information about the F-region from the GPS occultation measurements. We present the results of simulations that demonstrate the applicability and accuracy of the technique and observational concept.
CITATION STYLE
Dymond, K. F., Nee, J. B., & Thomas, R. J. (2000). The tiny ionospheric photometer: An instrument for measuring ionospheric gradients for the COSMIC constellation. Terrestrial, Atmospheric and Oceanic Sciences, 11(1), 273–290. https://doi.org/10.3319/TAO.2000.11.1.273(COSMIC)
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