Physics
Scientific paper
May 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh31a03p&link_type=abstract
American Geophysical Union, Spring Meeting 2001, abstract #SH31A-03
Physics
2162 Solar Cycle Variations (7536), 2164 Solar Wind Plasma, 2169 Sources Of The Solar Wind
Scientific paper
In November 2000 the Ulysses spacecraft reached the southernmost heliographic latitudes (-80 deg) for the second time in its 10 year cruise of the 3D heliosphere. The circumstances differ significantly though from its last passage during the solar minimum, which was dominated by uniform polar coronal hole flow. This time, highly variable elemental and charge state composition features are observed in the solar wind. Firstly, we present the complete, up-to-date SWICS dataset of the southern polar pass into the early stages of Ulysses' solar maximum fast latitude scan that is currently in progress. Secondly, connections of Ulysses/SWICS observations to quasi-stationary, transient, and corotating structures will be pointed out and highlighted with remote sensing observations of the solar corona.
Fisk Len A.
Gloeckler George
Posner Arik
Schwadron Nathan A.
Zurbuchen Thomas H.
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