On the basis of 48 random observations of the sun from June through December 1961 with a thin mica window Geiger tube on satellite Injun 1, it is found that: (a) The ‘quiet day’ solar X‐ray flux at 1 astronomical unit in the wavelength range λ < 14 A had a minimum value of 0.5×10−3 erg (cm2 sec)−1, a value which is approximately independent of the assumed blackbody temperature of the emitting areas of the sun over the temperature range 0.8 to 8×106 °K. (b) The solar X‐ray flux underwent substantial time variation, from the lowest value quoted in (a) to the highest value on July 20 during a Hα flare of importance 3. The X‐ray flux λ < 14 A on July 20 was 0.07 erg (cm2 sec)−1. (c) Three other high intensity values also appeared to be associated with visual flares, but no convincing relationship between intensity and flare activity was found among the other 44 cases. (d) The median flux observed in the 48 random observations was 1.7×10−3 erg (cm2 sec)−1 for λ < 14 A.