Long-term variations in the gamma-ray background on SMM

Details Long-term variations in the gamma-ray background on SMM Long-term variations in the gamma-ray background on SMM

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aipc..186..250k&link_type=abstract

IN: High-energy radiation background in space (A90-25305 09-93). New York, American Institute of Physics, 1989, p. 250-258.

Astronomy and Astrophysics

Astronomy

5

Background Radiation, Gamma Ray Spectrometers, Satellite Observation, Solar Maximum Mission, Data Bases, Gamma Ray Astronomy, Oso-7, Satellite-Borne Instruments, Temporal Distribution

Scientific paper

Long-term temporal variations in the various components of the background radiation detected by the gamma-ray spectrometer on the Solar Maximum Mission are presented. The SMM gamma-ray spectrometer was launched in February, 1980 and continues to operate normally. The extended period of mission operations has provided a large data base in which it is possible to investigate a variety of environmental and instrumental background effects. In particular, several effects associated with orbital precession are introduced and discussed.

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