Physics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh31a1155w&link_type=abstract
American Geophysical Union, Fall Meeting 2004, abstract #SH31A-1155
Physics
7599 General Or Miscellaneous, 7811 Discontinuities, 2164 Solar Wind Plasma, 2169 Sources Of The Solar Wind
Scientific paper
Using sample crossings of the heliospheric plasma sheet by the Ulysses spacecraft, we compare the abundances of heavy elements (Z > 2) near and within the sheet with the abundances found generally in the solar wind. The primary motivation for this study is to ascertain first if the sheet abundances are in fact different from those in the general solar wind, and, if so, to what extend the abundances reflect those known to be at the sun. A close relationship would confirm the sun to be the source of the plasma sheet, and may identify the source region. Variations of the abundances measured in the sheet from those near the sun will yield details of the transport mechanism.
Gloeckler George
Velli M. M.
Winterhalter Daniel
Woo Richard
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