Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nrl..reptq....s&link_type=abstract
Memorandum Report, Feb. 1980 - May 1981 Naval Research Lab., Washington, DC. Gamma and Cosmic Ray Astrophysics Branch.
Astronomy and Astrophysics
Astrophysics
Detection, Extraterrestrial Radiation, Gamma Rays, Geomagnetism, Nuclear Radiation, Scattering, Trapped Magnetic Fields, Electron Sources, Gamma Ray Spectra, Military Spacecraft, Neutron Sources, Positrons, Radiation Measurement
Scientific paper
The gamma-ray experiment on board NASA's Solar Maximum Mission Satellite (SMM) has detected nuclear radiation emitted from the reactor on COSMOS 1176. Direct observations of gamma-rays and possibly neutrons from this reactor were made at distances as close as about 350 km. Nuclear line features were observed in the gamma-ray spectrum. Explanations for some of these features are presented. The absolute power of the reactor is difficult to estimate at present; however, there is evidence that both the intensity and spectral shape of the emitted radiation changed significantly during the operational period of COSMOS. The reactor was also detected at distances of greater than or = 6,300 km in an indirect manner. Positrons and electrons escaping from the COSMOS spacecraft following production by the intense gamma-radiation are stored temporarily in the Earth's magnetic field and unambiguous signal due to their characteristic annihilation into gamma-rays at 511 keV. Details of these observations and their implications are discussed.
Chupp Edward L.
Eisele J. A.
Kurfess James D.
Marlow K. W.
Share Gerald H.
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