Abstract
Further studies on the gamma-radiation from V48, N13, Cu64, Mg27, and Na24 have been carried out using a large hydrogen-filled cloud chamber and with several improvements in technique. The most striking feature of the spectra, is the presence of a large amount of 1 Mev radiation from V48. Comparison with the ordinary annihilation radiation indicates that there are four 1 Mev quanta emitted per positron. The possible origin of this radiation is discussed. A difference in the gamma-radiation emitted from N13 and Cu64 is noted, the latter having a more pronounced high energy tail. A small number of tracks from Mg27 have been measured and indicate a monochromatic line at 0.88±0.05 Mev. The radiation from Na24 has been re-examined. The results indicate that the quantum energy of the high energy line is 3.00±0.05 Mev. The two other lines with energies of 2 Mev and 1 Mev are confirmed.

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