Low energy gamma ray enhancement observed during a stratospheric balloon flight

Details Low energy gamma ray enhancement observed during a stratospheric balloon flight Low energy gamma ray enhancement observed during a stratospheric balloon flight

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982rbrfi..12..501r&link_type=abstract

Revista Brasileira de Fisica (ISSN 0374-4922), vol. 12, Sept. 1982, p. 501-515.

Computer Science

Sound

Balloon Sounding, Gamma Rays, Secondary Cosmic Rays, Stratosphere, Supernova Remnants, Energy Spectra, Gamma Ray Spectra, Radiation Detectors, Seyfert Galaxies

Scientific paper

An omnidirectional gamma ray detector was flown on a stratospheric balloon on December 15, 1978 from Sao Josedos Campos, Brazil. After reaching ceiling, an increase in the count rate was observed. After considering the probable sources causing this increase, it is suggested that this increase might be due to the supernova remnant, first observed optically in May 1978 in galaxy MCG-4-32-23. The energy spectrum of supernova shows a flattening of slope above 1.5 MeV.

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