scholarly journals Klein–Nishina Effect and the Cosmic Ray Electron Spectrum

2021 ◽  
Vol 38 (3) ◽  
pp. 039801 ◽  
Author(s):  
Kun Fang ◽  
Xiao-Jun Bi ◽  
Su-Jie Lin ◽  
Qiang Yuan
Keyword(s):  
Electron Spectrum ◽  
Cosmic Ray

scholarly journals Erratum: Signature of Energy Losses on the Cosmic Ray Electron Spectrum [Phys. Rev. Lett. 125 , 051101 (2020)]

2021 ◽  
Vol 126 (24) ◽  
Author(s):  
Carmelo Evoli ◽  
Pasquale Blasi ◽  
Elena Amato ◽  
Roberto Aloisio
Keyword(s):  
Electron Spectrum ◽  
Cosmic Ray ◽  
Energy Losses

Cosmic-Ray Electron Spectrum above 50 BeV and Its Implications for Cosmic-Ray Confinement

1968 ◽  
Vol 20 (14) ◽  
pp. 764-768 ◽  
Author(s):  
K. C. Anand ◽  
R. R. Daniel ◽  
S. A. Stephens
Keyword(s):  
Electron Spectrum ◽  
Cosmic Ray

scholarly journals Implications of the cosmic ray electron spectrum and anisotropy measured with Fermi-LAT

2011 ◽  
Vol 34 (7) ◽  
pp. 528-538 ◽  
Author(s):  
Giuseppe Di Bernardo ◽  
Carmelo Evoli ◽  
Daniele Gaggero ◽  
Dario Grasso ◽  
Luca Maccione ◽  
...  
Keyword(s):  
Electron Spectrum ◽  
Cosmic Ray

scholarly journals The primary cosmic-ray electron spectrum in the energy range from 300 MeV to 4 BeV from 1964 to 1966

1968 ◽  
Vol 46 (10) ◽  
pp. S892-S895 ◽  
Author(s):  
Jacques L'heureux ◽  
Peter Meyer
Keyword(s):  
Energy Spectrum ◽  
Electron Spectrum ◽  
Intensity Variation ◽  
Cosmic Ray ◽  
Primary Electron ◽  
Counter Telescope ◽  
Improved Accuracy ◽  
Primary Electrons

Measurements of the primary electron spectrum were made during the summers of 1964, 1965, and 1966 using a balloon-borne counter telescope flown from Fort Churchill, Manitoba. Several balloon flights were carried out in each year in order to eliminate short-term intensity variations. This paper addresses itself to two questions: (1) the determination of the energy spectrum of primary electrons in the energy interval from 300 MeV to 4 BeV; and (2) the long-term intensity variations of the primary electron flux from 1964 through 1966. The energy spectrum was determined with improved accuracy in 1966 and agrees with our previous results. Comparison of the electron spectra obtained in 1964, 1965, and 1966 shows that, within the errors of our measurements, no long-term intensity variation existed. The upper limit for the change of flux with respect to 1965 amounts to 20% in all energy intervals studied.[Formula: see text]

The cosmic-ray electron spectrum in a disc-halo galactic model

1967 ◽  
Vol 50 (2) ◽  
pp. 359-361
Author(s):  
R. F. O’Connell ◽  
S. Sofia
Keyword(s):  
Electron Spectrum ◽  
Cosmic Ray ◽  
Galactic Model
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