Interstellar Cosmic Ray Spectra from the Nonthermal Radio Background from 0.4 to 400 MHz

Details Interstellar Cosmic Ray Spectra from the Nonthermal Radio Background from 0.4 to 400 MHz Interstellar Cosmic Ray Spectra from the Nonthermal Radio Background from 0.4 to 400 MHz

May 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970phrvl..24.1193g&link_type=abstract

Physical Review Letters, vol. 24, Issue 21, pp. 1193-1196

Physics

56

Scientific paper

We deduce the interstellar electron spectrum from the nonthermal radio background. From 200 MeV to a few GeV the spectral index is 1.8 and there is evidence for residual solar modulation. Above a few GeV, the spectrum is steeper and the intensity is similar to that observed at earth. A consistent modulation for electrons and protons of the same rigidity can be obtained by using the complete diffusion-convection energy-loss theory of solar modulation.

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