The charge state of the anomalous cosmic-ray component

Details The charge state of the anomalous cosmic-ray component The charge state of the anomalous cosmic-ray component

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...333l.109m&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 333, Oct. 15, 1988, p. L109-L112.

Astronomy and Astrophysics

Astrophysics

9

Energy Spectra, Interplanetary Medium, Interstellar Matter, Solar Activity, Solar Cosmic Rays, Solar Wind, Helium Ions, Ionized Gases, Nitrogen Ions, Oxygen Ions, Pioneer 10 Space Probe, Voyager 2 Spacecraft

Scientific paper

H, He, and O cosmic-ray energy spectra obtained in the outer heliosphere by the Voyager 2 and Pioneer 10 spacecraft during the most recent periods of declining solar activity are presented graphically and analyzed. The recovery of high-rigidity particles is shown to be significantly delayed relative to that of the low-rigidity particles. This finding and the demodulated source spectra are attributed to the presence of singly ionized anomalous He and O, as predicted by Fisk et al. (1974).

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