On the energetic particle fluxes at 5 AU associated with the April/May 1998 solar activity: Ulysses observations

Details On the energetic particle fluxes at 5 AU associated with the April/May 1998 solar activity: Ulysses observations On the energetic particle fluxes at 5 AU associated with the April/May 1998 solar activity: Ulysses observations

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..609m&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 609-612 (1999).

Computer Science

Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

Located close to the ecliptic at 5.4 AU heliocentric distance, Ulysses observed energetic particle increases in April/May 1998 that were related to the second major episode of activity in the new solar cycle, the first being in November, 1997. In this paper, we report on the characteristics of the transient particle enhancements seen at Ulysses, including the compositional signatures, and suggest an interpretation in terms of the activity occurring at the Sun.

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