Observations of High-energy Gamma Rays
The application of the Cerenkov light technique to detect the intensity and direction of incident gamma ray photons above 10 to the 11th power eV is studied.
Engineering topics
Publications and source records attributed to Fazio, G. G..
The application of the Cerenkov light technique to detect the intensity and direction of incident gamma ray photons above 10 to the 11th power eV is studied.
Ground based instruments designed to measure high energy gamma ray sources as a function of Cerenkov light bursts are described. Data are also included on the sensitivity, advantages, and disadvantages of the instruments.
A panel discussion was held on all data presented at the conference on Gamma Ray Astronomy. The present status and future directions of the science were outlined.
High energy break in isotropic gamma ray spectrum predicted from critical test of cosmological pion-decay hypothesis
Critical test of cosmological pion decay hypothesis for origin of isotropic gamma radiation above 1 MeV
Cosmic gamma radiation detection with vidicon spark chamber on high altitude balloon
Nucleon isobars and hyperons carrying off interstellar and intergalactic proton-proton collision energy, discussing high energy gamma ray decay product
Solar gamma-ray flux in high energy region analyzed using OSO-I satellite
Cosmic gamma radiation searched with vidicon spark chamber flown in high-altitude balloon
Spark chamber with vidicon readout for balloon- and satellite-borne high energy gamma ray astronomy analysis, noting Cerenkov counter
Gamma ray spectrum emitted by Sun and prediction of approximate fluxes at Earth based on solar flare model
Mechanisms of solar gamma radiation production - prediction of fluxes at earth
Brief review of the present status of high-energy gamma-ray astronomy and a report of results from the orbiting solar observatory