Computer Science – Sound
Scientific paper
Sep 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jgr....84.5279r&link_type=abstract
Journal of Geophysical Research, vol. 84, Sept. 1, 1979, p. 5279-5288.
Computer Science
Sound
9
Angular Distribution, Atmospheric Radiation, Energy Distribution, Gamma Rays, Incident Radiation, Balloon Sounding, Gamma Ray Telescopes, Vertical Motion, Zenith
Scientific paper
Differential fluxes of gamma rays were calculated for energies of 2-25 MeV, zenith angles of 0-50 deg and 180-130 deg, and atmospheric depths from nominal sea level, 1000 g/sq cm, to float altitude, 3.5 g/sq cm residual atmosphere. Above 100 g/sq cm growth curves were constructed to estimate the contribution of the extraterrestrial gamma ray flux to the total downward-moving flux, while the upward-moving gamma rays were taken to be strictly of atmospheric origin. Below 100 g/sq cm, all gamma rays originate in the atmosphere. The downward atmospheric flux increases by almost two orders of magnitude between float altitude and the Pfotzer maximum, while the extraterrestrial flux is attenuated exponentially. Gamma rays produced by neutron interactions with the carbon in the scintillator liquid are eliminated by constructing growth curves for downward-moving gamma rays at high altitudes and are negligible compared with downward-moving gamma rays at lower altitudes and upward-moving gamma rays at all altitudes.
Jennings Mark C.
Radwin M. D.
Ryan Michael J.
White Steven R.
Zych Allen D.
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