EPG. Table.2ui-lists yields obtained by Program 10 for shots fired in the ie Total thermal radiation measured on Teak. wae Although time interval was measured, the value obtained is probably low by about 10 per cent. The Teller light which provides time interval in- formation originates at approximately 25 to 30 km above sea level, where the main gamma ray flux is stopped. The slow apparent rise time of the rather weak primary signal and unfavorable geometry related to the error in burst position may have caused a delay in the recording of the first signal. It is expected that a correction can be applied after further analysis. The results of the experiments designed to attain the third and main objective of the two programs were unfavorably affected by the burst location error. Specifically, information on the very early development of the fireball could not be obtained, since none of the collimated instrument channels covered the true burst location. However the limb and so-called "envelope spaces" between radii of 4 and 12 km yielded interesting time-resolved spectroscopic data for times up to 5 min after the burst. They require much specific attention and analysis. Generally one can say that the records will provide information on the fluorescent yield of gamma ray and x-ray excited air, on the energy deposition in the air versus distance from source and thus in- directly on source strength, on transition processes in the medium and low energy deposition range, on gas temperatures and cooling rates, and about early recombination processes. One record shows neutron flux effects on “air. Cursory inspection of the spectrograms and oscilloscope traces indicates higher temperatures and a greater degree of ionization at a given radius than expected and thus larger dimensions of the luminous fireball. This is borne out by the observation that the emission by molecular species at 12 km from burst center was of almost equal magnitude as the originally expected signal from the 6-km location. Closer in, singly and doubly ionized atomic species show up where the appearance of molecular species was expected. On the other hand there are indications that the core area of the fireball was less bright than predicted, indicating a higher rate of cooling by radiation flow towards the edges. The project plans to analyze high speed photographic data for radius versus time and brightness versus time information. The combined information may suffice to check and revise current theory and provide a reasonably comprehensive understanding of high altitude fireball phenomenology. After failure to obtain early fireball core data from Teak shot, an at- tempt was made to obtain such data from Orange, although one had to ex- pect very high reaction rates, namely of the order of at least per second, Many instruments were therefore pointed st the burst location and set for highest possible time resolution. Unfortunately the shot was fired under deteriorating weather conditions, resulting in a mean diffuse optical transmission of only 6 per cent; the transmission for the collimated observation channels was even less, Instrument and station performance was 44