The gamma ray spectrometer for the Solar Maximum Mission

✍ Scribed by D. J. Forrest; E. L. Chupp; J. M. Ryan; M. L. Cherry; I. U. Gleske; C. Reppin; K. Pinkau; E. Rieger; G. Kanbach; R. L. Kinzer; G. Share; W. N. Johnson; J. D. Kurfess

• Publisher: Springer
• Year: 1980
• Tongue: English
• Weight: 498 KB
• Volume: 65
• Category: Article
• ISSN: 0038-0938
• DOI: 10.1007/bf00151381

✦ Synopsis

The Solar Maximum Mission Gamma Ray Experiment (SMM GRE) utilizes an actively shielded, multicrystal scintillation spectrometer to measure the flux of solar gamma rays. The instrument provides a 476-channel pulse height spectrum (with energy resolution of ~7% at 662 keV) every 16.38 s over the energy range 0.3-9 MeV. Higher time resolution (2 s) is available in three windows between 3.5 and 6.5 MeV to study prompt gamma ray line emission at 4.4 and 6.1 MeV. Gamma ray spectral analysis can be extended to -> 15 MeV on command. Photons in the energy band from 300-350 keV are recorded with a time resolution of 64 ms. A high energy configuration also gives the spectrum of photons in the energy range from 10-100 MeV and the flux of neutrons ~>20 MeV. Both have a time resolution of 2 s. Auxiliary X-ray detectors will provide spectra with 1-sec time resolution over the energy range of 10-140 keV. The instrument is designed to measure the intensity, energy, and Doppler shift of narrow gamma ray lines as well as the intensity of extremely broadened lines and the photon continuum. The main objective is to use this time and spectral information from both nuclear gamma ray lines and the photon continuum in a direct study of the dynamics of the solar flare/particle acceleration phenomena.