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High-Energy Cosmic-Ray Electrons: A New Measurement Using Transition-Radiation Detectors

G. Hartmann, Dietrich Müller, Thomas A. Prince

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Abstract

A new detector for cosmic-ray electrons, consisting of a combination of a transitionradiation detector and a shower detector, has been constructed, calibrated at accelerator beams, and exposed in a balloon flight under 5 g/${\mathrm{cm}}^{2}$ of atmosphere. The design of this instrument and the methods of data analysis are described. Preliminary results in the energy range 9-300 GeV are presented. The energy spectrum of electrons is found to be significantly steeper than that of protons, consistent with a long escape lifetime of cosmic rays in the galaxy.

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A new detector for cosmic-ray electrons, consisting of a combination of a transitionradiation detector and a shower detector, has been constructed, calibrated at accelerator beams, and exposed in a balloon flight under 5 g/${\mathrm{cm}}^{2}$ of atmosphere. The design of this instrument and the methods of data analysis are described. Preliminary results in the energy range 9-300 GeV are presented. The energy spectrum of electrons is found to be significantly steeper than that of protons, consistent with a long escape lifetime of cosmic rays in the galaxy.

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Available abstract

A new detector for cosmic-ray electrons, consisting of a combination of a transitionradiation detector and a shower detector, has been constructed, calibrated at accelerator beams, and exposed in a balloon flight under 5 g/${\mathrm{cm}}^{2}$ of atmosphere. The design of this instrument and the methods of data analysis are described. Preliminary results in the energy range 9-300 GeV are presented. The energy spectrum of electrons is found to be significantly steeper than that of protons, consistent with a long escape lifetime of cosmic rays in the galaxy.

Key concepts: Physics, Cosmic ray, Detector, Electron, Range (aeronautics), Nuclear physics, Radiation, Particle detector

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