Experimental determination of the spectrum of gamma photons in the atmosphere at 12 GV geomagnetic cutoff

Physics

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Background Radiation, Balloon-Borne Instruments, Gamma Rays, Geomagnetism, Stratosphere Radiation, X Ray Spectra, Atmospheric Pressure, Monte Carlo Method, Radiant Flux Density, Radiation Detectors, Scintillation Counters

Scientific paper

The paper analyzes data on the gamma-ray photon flux between 0.9 and 18.0 MeV as a function of altitude obtained in two stratospheric balloon flights. Cutoff rigidity was 12 GV. A 4-inch by 4-inch NaI(Tl) crystal detector encapsulated in a 1-cm thick plastic scintillator operating in anticoincidence was used. Above 20 g per sq cm, the differential spectrum could be represented by a power law with exponent 1.0 plus or minus 0.1, independently of altitude. From 20 to 760 g per sq cm the spectrum was steeper, with spectral index of 1.3 plus or minus 0.1. At 3.5 g per sq cm, the gamma-ray flux was 0.30 photons per sq cm sec. The measurements permit determination of the background noise of cosmic gamma radiation.

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