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Primary Cosmic-Ray Electron Energy Spectrum from 10 to 200 MeV Observed in Interplanetary Space

C. Y. Fan*, J. L'Heureux*, and Peter Meyer

  • Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637

  • *Present address: Department of Physics, The University of Arizona, Tucson, Ariz.
  • Also Department of Physics.

Phys. Rev. Lett. 23, 877 – Published 13 October, 1969

DOI: https://doi.org/10.1103/PhysRevLett.23.877

Abstract

We have measured the quiet-time flux and energy spectrum of primary cosmic-ray electrons in the energy range from 10 to 200 MeV in interplanetary space. This investigation was carried out with an instrument on board the satellite OGO-5 and covers the period from 25 March to 25 April 1968.

References (6)

  1. K. P. Beuermann, C. J. Rice, E. C. Stone, and R. E. Vogt, Phys. Rev. Letters 22, 412 (1969)
  2. J. L'Heureux and P. Meyer, Can. J. Phys. 46, S892 (1968)
  3. J. Rockstroh and W. R. Webber, University of Minnesota Publication No. CR-126, 1969
  4. G. M. Simnett and F. B. McDonald, Goddard Space Flight Center Report No. X-611-68-450, 1968 (to be published)
  5. W. R. Webber, J. Geophys. Res. 73, 4905 (1968)
  6. P. B. Abraham, K. A. Brunstein, and T. L. Cline, Phys. Rev. 150, 1088 (1966)

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