The intensity and spectrum of the electron component of cosmic rays

Details The intensity and spectrum of the electron component of cosmic rays The intensity and spectrum of the electron component of cosmic rays

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974izssr..38.1816k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Kharkov, Ukrainian SSR, Sept. 25-28, 1973.) Akademiia Nauk SSSR, Izv

Physics

Cosmic Ray Showers, Electron Flux Density, Secondary Cosmic Rays, Stratosphere Radiation, Balloon-Borne Instruments, Geomagnetism, High Altitude Nuclear Detection, Nuclear Radiation Spectroscopy

Scientific paper

The electron spectrum in the stratosphere (up to 31 km) was studied with a balloon-born spectrometer both during the phase of ascent and during the 20-hr drift phase. The experiment was carried out on October 12, 1972. The characteristics of the instrument and its efficiency control parameters are described. The background of secondary electrons at the drift altitude is established by studying the spectrum of secondary electrons with energies below the geomagnetic threshold at various heights. The experimental and calculated differential spectra of electrons produced in the atmosphere are presented and discussed.

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