Low-energy ions near the termination shock

Details Low-energy ions near the termination shock Low-energy ions near the termination shock

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..858...73d&link_type=abstract

PHYSICS OF THE INNER HELIOSHEATH: Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics

Astronomy and Astrophysics

Astrophysics

13

Heliopause And Solar Wind Termination, Planetary Bow Shocks, Interplanetary Shocks, Particle Emission, Solar Wind, Energetic Particles

Scientific paper

This paper describes intensities, energy spectra, and anisotropies of ions 0.04-17.6 MeV measured at Voyager 1 in the solar wind and heliosheath, compares 3-17 MeV precursor proton angular distributions measured in the termination shock foreshock at Voyager 2 during 2005-06 with those measured at V1 during the latter half of 2002, and provides an update on estimates of the radial component of plasma flow speed in the heliosheath.

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