Gamma ray spectroscopy in astrophysics: Solar gamma ray astronomy on solar maximum mission

Details Gamma ray spectroscopy in astrophysics: Solar gamma ray astronomy on solar maximum mission Gamma ray spectroscopy in astrophysics: Solar gamma ray astronomy on solar maximum mission

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978grsa.rept..558f&link_type=abstract

In NASA. Goddard Space Flight Center Gamma Ray Spectry. in Astrophys. p 558-574 (SEE N78-31971 22-88)

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Experiment Design, Gamma Ray Astronomy, Solar Maximum Mission, Solar Spectrometers, International Cooperation, Mission Planning, Radiation Detectors, Satellite-Borne Instruments, Solar Flares

Scientific paper

The SMM gamma ray experiment and the important scientific capabilities of the instrument are discussed. The flare size detectable as a function of spectrum integration time was studied. A preliminary estimate indicates that a solar gamma ray line at 4.4 MeV one-fifth the intensity of that believed to have been emitted on 4 August 1972 can be detected in approximately 1000 sec with a confidence level of 99%.

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