High energy electrons beyond 100 GEV observed by emulsion chamber

Details High energy electrons beyond 100 GEV observed by emulsion chamber High energy electrons beyond 100 GEV observed by emulsion chamber

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986icrc....9..539n&link_type=abstract

In NASA: Goddard Space Flight Center Nineteenth International Cosmic Ray Conference. Conference Papers: Invited Rapporteur, High

Statistics

Balloon-Borne Instruments, Cosmic Rays, High Energy Electrons, Nuclear Emulsions, Radiation Counters, Energy Spectra, Particle Tracks, Particle Trajectories

Scientific paper

Much efforts have been expended to observe the spectrum of electrons in the high energy region with large area emulsion chambers exposed at balloon altitudes, and now 15 electrons beyond 1 TeV have been observed. The observed integral flux at 1 TeV is (3.24 + or - 0.87)x10(-5)/sq m sec sr. The statistics of the data around a few hundred GeV are also improving by using new shower detecting films of high sensitivity. The astrophysical significance of the observed spectrum are discussed for the propagation of electrons based on the leaky box and the nested leaky box model.

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