SOLAR-WIND CHARGE STATES MEASURED BY ULYSSES SWICS IN THE SOUTH POLAR HOLE

The Ulysses mission now has an extensive data base covering several passes of the south polar coronal hole as the spacecraft proceeds to higher latitudes. Using composition measurements from the SWIGS experiment on the Ulysses spacecraft, we have obtained charge state distributions, and hence inferred coronal ionization temperatures, for several solar wind species. In particular, we present an overview of Oxygen ionization temperature measurements, based on the O7+/O6+ ratio, for the period January 1993 until April 1994 (similar to 23 degrees S to similar to 61 degrees S heliographic latitude), and detailed Oxygen, Silicon and Iron charge state distributions of the south polar hole during a two month period of nearly continuous hole coverage, Dec 1993 - Jan 1994 (similar to 45 degrees S to 52 degrees S heliographic latitude).