Voyager 1 and 2 Measurements of the Energy Spectra of Cosmic-Ray C, N, O, Ne, Mg, Si and Fe Nuclei in the Outer Heliosphere at the 1997-1998 Solar Minimum Activity

Details Voyager 1 and 2 Measurements of the Energy Spectra of Cosmic-Ray C, N, O, Ne, Mg, Si and Fe Nuclei in the Outer Heliosphere at the 1997-1998 Solar Minimum Activity Voyager 1 and 2 Measurements of the Energy Spectra of Cosmic-Ray C, N, O, Ne, Mg, Si and Fe Nuclei in the Outer Heliosphere at the 1997-1998 Solar Minimum Activity

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aps..aprh14003l&link_type=abstract

American Physical Society, April Meeting, April 28 - May 1, 2001 Washington, DC Bulletin of the American Physical Society, Vol.

Physics

Scientific paper

Data from the High-Energy Telescopes of the CRS experiments on Voyagers 1 and 2 at distances of 69 AU and 54 AU in 1997-98 have been used to measure the spectra and charge ratios of various primary nuclei such as C, O, Ne, Mg, Si and Fe in Galactic cosmic rays. This is a new measurement of the primary/primary ratios from Voyager 1 and 2 in the extended energy range. The new extended Voyager energy spectra ranges are: for carbon 17-230 MeV/n, for silicon 20-350 MeV/n, and for iron 65-1750 MeV/n. The solar modulation level relevant for this data is estimated to be 300 MV.

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