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Solar Physics

, Volume 41, Issue 2, pp 449–458 | Cite as

Heavy solar cosmic rays in the January 25, 1971 solar flare

  • Charles J. PellerinJr.
Article

Abstract

A detailed study of the charge composition of heavy solar cosmic rays measured in the January 25, 1971 solar flare including differential fluxes for the even charged nuclei from carbon through argon is presented. The measurements are obtained for varying energy intervals for each nuclear species in the energy range from 10 to 35 MeV nucleon−1. In addition, abundances relative to oxygen are computed for all the above nuclei in the single energy interval from 15 to 25 MeV nucleon−1. This interval contains measurements for all of the species and as a result requires no spectral extrapolations. An upper limit for the abundance of calcium nuclei is also presented.

These measurements, when combined with other experimental results, enable the energy dependence of abundance measurements as a function of nuclear charge to be discussed. It is seen that at energies above about 10 MeV nucleon−1, the variations of abundance ratios are limited to about a factor of 3 from flare to flare, in spite of large variations in other characteristics of these solar events.

Keywords

Oxygen Calcium Argon Flare Energy Range 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© by D. Reidel Publishing Company 1975

Authors and Affiliations

  • Charles J. PellerinJr.
    • 1
  1. 1.NASA/Goddard Space Flight CenterGreenbeltU.S.A.

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