Abstract
Abstract Solar ultraviolet fluxes in the wavelength region 1900 to 2300A were measured during the first balloon flight of Project stratoprobe on July 8, 1974, over a range of solar zenith angles at a float altitude of 28.6 km. High‐resolution computer simulations of the measured spectra were made for a range of solar zenith angles of 40° to 80° over the wavelength region 2050 to 2150A, and comparisons made with the observed spectra at 40° and 47 °. Qualitative agreements were obtained but there were significant discrepancies between the simulated and experimentally obtained fluxes. Sources of the discrepancies are discussed.
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