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Titel The effects of SDO-EVE measurements on ionospheric modeling
VerfasserIn Catalin Negrea, Timothy Fuller-Rowell, Mihail Codrescu, Frank Eparvier, Juan Fontenla
Konferenz EGU General Assembly 2013
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 15 (2013)
Datensatznummer 250072473
 
Zusammenfassung
Errors associated with ionosphere-thermosphere modeling can be attributed to a number of factors. Very often, they are caused by incomplete information regarding the forcings acting on the system. Empirical statistical models and proxies are used to compensate by making use of correlations between available measurements and quantities of interest. One such measurement, F10.7 index often serves as a proxy for Extreme Ultra Violet photon fluxes. While this approach has worked remarkably well, data from the Solar Dynamics Observatory mission allows us to improve the forcings and the model results. In this study, we investigate several alternatives to the F10 approach. We make use of SDO data and the Solar Radiation Physical Model, as well as TIMED-SEE. The effect on model results is presented and discussed, with the SDO / SRPM combination resulting in the greatest increase in model performance.