Modeled solar EUV flux during the Equinox Transition Study - September 17-24, 1984

Computer Science – Sound

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Equinoxes, Extreme Ultraviolet Radiation, Flux Transfer Events, Solar Activity, Solar Flux, Chromosphere, Remote Sensing, Rocket Sounding, Stellar Models

Scientific paper

A new empirical model of solar extreme ultraviolet (EUV) irradiance variability has been developed based on satellite and rocket EUV observations for all levels of solar activity. Its results for the Equinox Transition Study (ETS) period of Septebmer 17-24, 1984, have been calculated, and the tabulated results of photon and energy fluxes for each day of this period are presented. The model average total EUV full-disk energy flux for the spectral range between 1.9 and 105.0 nm for the ETS period is 2.9 ergs/sq cm/s, with a general secular increase in the total flux level between September 17 and September 24. This modeled rise corresponds to the increased EUV irradiance variability due to active region evolution and passage across the disk.

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