Energetic particle composition measurements at high heliographic latitudes around the solar activity maximum

Details Energetic particle composition measurements at high heliographic latitudes around the solar activity maximum Energetic particle composition measurements at high heliographic latitudes around the solar activity maximum

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..598..189h&link_type=abstract

SOLAR AND GALACTIC COMPOSITION: A Joint SOHO/ACE Workshop. AIP Conference Proceedings, Volume 598, pp. 189-193 (2001).

Computer Science

Particle Emission, Solar Wind, Composition, Time Series Analysis, Time Variability

Scientific paper

From 1999 until the end of 2000 the Ulysses spacecraft was traveling back towards the southern solar polar region from about 5 AU to less than 2.5 AU. In this time period the solar activity was close to the maximum. The results of a preliminary analysis of energetic particle composition data covering the energy range 4-20 MeV/n recorded by the COSPIN/LET instrument are shown. We attempt to use the composition signatures to identify the sources of energetic particles observed at high latitudes. .

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