The anomalous cosmic-ray component

Details The anomalous cosmic-ray component The anomalous cosmic-ray component

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ippe.conf..133c&link_type=abstract

In Jet Propulsion Lab., California Inst. of Tech., Interplanetary Particle Environment. Proceedings of a Conference p 133-134 (S

Physics

Cosmic Rays, Energy Spectra, Solar Magnetic Field, Sun, Graphs (Charts), Solar Physics

Scientific paper

This brief report is intended to update the anomalous component section of the summary report of the galactic cosmic-ray working group (Mewaldt et al., 1987), which was drafted at the March 1987 Workshop on the Interplanetary Charged Particle Environment at the Jet Propulsion Laboratory. The description of the spectrum of the anomalous cosmic-ray component is contained in section 3.3 of that report. That description is based on data analyzed through day 310 of 1986, and in it we proposed that the energy spectrum of the various species of the anomalous component could be derived by scaling from two generic spectra. Two generic spectra were required because the energy spectrum of the anomalous component changed shape near the time of the solar magnetic field reversal in 1980. These two generic spectra are shown in Figure 2 of the summary report.

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