Solar energetic particle propagation in 1997-99: Observations from ACE, Ulysses, and Voyagers 1 and 2

Details Solar energetic particle propagation in 1997-99: Observations from ACE, Ulysses, and Voyagers 1 and 2 Solar energetic particle propagation in 1997-99: Observations from ACE, Ulysses, and Voyagers 1 and 2

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..528..161d&link_type=abstract

ACCELERATION AND TRANSPORT OF ENERGETIC PARTICLES OBSERVED IN THE HELIOSPHERE: ACE 2000 Symposium. AIP Conference Proceedings, V

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Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays

Scientific paper

Solar energetic particles injected during intense activity in April-May 1998 and observed at ACE and Ulysses are identified in 0.5-1.5 MeV proton data from the LECP instrument on Voyager 2 (56 AU, 20 °S) and Voyager 1 (72 AU, 33 °N). A shell of ~1 MeV protons ~60 days wide reached peak intensity at Voyager 2 on 1998.7 and at Voyager 1 on 1998.8, some 6 months after the April-May 1998 solar activity. We interpret these results in terms of infrequent scattering during propagation from 1 to 72 AU in helioradius and over ~50° in latitude. .

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