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The proposed scheme of Fig. 8 with the newly postulated ^605-kev transition encounters difficulties when one considers the deexcitation of the 1365-kev level by only the 563-kev gamma ray. The situation would be partially alleviated if the 1367-kev gamma ray led from the 1365 level to the ground state. The measured conversion coefficient is then too small to be consistent with the spin assignments. In addition, the coincidence measurements indicate that more low-energy beta decays are followed by 605-kev gammas than by 796-kev gammas. The 1367-kev transition as shown has the appropriate "shunting" effect. For this reason too it is difficult to justify inverting the order of the 796 and 605 gammas, although such an inversion would improve the consistency of the 1038 and 1168 gamma rays.A ground-state spin of 4 has been measured for Cs 134

X-ray observations from Vela-5 spacecraft of five flares occurring in November and December 1969 were 1educed to temperatures and emission measures as a function of time. This reduction was done assuming a thermal spectrum including free-free and free-bound emission. A phenomenological model is proposed to explain the nature of the time behavior of the temperature and emission measure.

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