Solar energetic photon transients - 50 keV-100 MeV

The observed properties of solar transient photon impulses between a few keV and 100 MeV recorded by the SMM are compared and reasons for continued monitoring of solar photon transients are discussed. Various solar flare events observed are reviewed, along with gamma ray measurements. It is calculated that the emission of energetic photons is due to ion and electron interactions with matter, with both species undergoing acceleration at close time intervals. The gamma ray events and microwave emissions showed time structures similar to previously recorded X ray emissions. Bursts of all three radiation types have displayed a quasi-periodicity of less than 10 sec. Data on the 2.223 MeV neutron capture line have shown a decay in line intensity to take about 50 sec, consistent with Monte Carlo calculation for a He-3/H abundance of 0.00005