Voyager 1 Observations of the Anisotropies of Enhanced MeV Ion Fluxes at 85 AU

Details Voyager 1 Observations of the Anisotropies of Enhanced MeV Ion Fluxes at 85 AU Voyager 1 Observations of the Anisotropies of Enhanced MeV Ion Fluxes at 85 AU

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....7.3777c&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

2

Scientific paper

We report on the diffusive flow anisotropies observed in low-energy protons during intensity increases at Voyager 1 in 2001 and 2002. We propose that the unusual increased intensities after mid-2002 are due to particles accelerated by the solar wind termination shock or by the turbulent interface between the high-sp eed and low-sp eed solar wind flows. Fig. 1. (top) Three-day moving average intensity of 2-3 MeV protons at V1 and V2 vs. time. (b ottom) Five-day moving average intensity of electrons and >70 MeV/nuc galactic cosmic rays at V1.

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