Physics
Scientist
C.E. Saclay, Gif-sur-Yvette, France
High energy cosmic ray results from the ULYSSES ascent to the solar south pole.
Latitudinal and radial variation of >2 GeV/n protons and alpha particles in the southern heliosphere at solar maximum: Ulysses cospinket and neutron monitor network observations
Modulation of galactic cosmic ray particles observed on board the ULYSSES spacecraft
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