In this paper we describe the results of three Nike‐Cajun rocket flights made during the November 12, 1960, solar proton event. By means of Geiger counter and scintillation counter measurements the spectrum of protons has been extended downward in energy to 0.2 Mev. A group of particles with energy between 0.2 and 1 Mev has been found, and it is suggested that this group may not be part of the flare‐accelerated spectrum, but may be associated with the plasma in the earth‐sun region. The spectrum in the low‐energy region above 1 Mev cannot be represented by a simple extrapolation of the spectrum at higher energies as observed, for instance, by means of balloons.