The spectrum of primary electrons with energies exceeding 3 GeV

Details The spectrum of primary electrons with energies exceeding 3 GeV The spectrum of primary electrons with energies exceeding 3 GeV

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..529i&link_type=abstract

(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest

Computer Science

Sound

Balloon Sounding, Cosmic Ray Showers, Electron Energy, Energy Spectra, Midlatitude Atmosphere, Balloon-Borne Instruments, Cosmic Ray Albedo, Magnetic Rigidity, Primary Cosmic Rays

Scientific paper

The paper presents results on the energy spectra of cosmic ray shower electrons observed in 1972 and 1973 from high-altitude balloons in the midlatitude atmosphere. The magnetic cut-off rigidity was about 3.1 GeV and the electron energy was measured by a cosmic ray shower spectrometer capable of measuring energies up to 20 GeV. Differential energy spectra are presented for primary electrons at various pressures of the atmosphere as is the differential energy spectrum of albedo electrons at a pressure of 13.5 g/sq cm.

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