A summary of full-disk solar fluxes for the wavelength region 250--1940 ¿ compiled from data obtained from six Air Force Geophysics Laboratory rocket spectrometers flown during the period 1969--1976 is presented. The intense spectral lines in the wavelength region from 300 to 1220 ¿ are emitted predominantly from the solar chromosphere and the chromosphere-corona transition region. The data indicate that the flux in this wavelength region increases generally by less than 10% with increasing values of the solar F10.7cm emission from 70 to 177 in units of 10-22 W m-2 Hz-1.