On the alpha-particle abundance and the origin of slow solar wind: Ulysses observations

Details On the alpha-particle abundance and the origin of slow solar wind: Ulysses observations On the alpha-particle abundance and the origin of slow solar wind: Ulysses observations

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..219b&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 219-221 (1999).

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Solar Wind Plasma, Sources Of Solar Wind, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays

Scientific paper

We extend a recent study on the relationship between the alpha-particle abundance and the solar wind velocity at different heliographic latitudes. Our results confirm that in the region at the mid-latitude boundary of the fast polar wind there is no evidence of correlation between these two quantities, in contrast to what is found in the near-equatorial solar wind. This may depend upon a different relevance, in different regions, of the processes at the origin of low-velocity flows.

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