SPARTAN-201 CORONAL SPECTROSCOPY DURING THE POLAR PASSES OF ULYSSES

Spartan 201 is a shuttle deployed spacecraft that is scheduled to perf orm ultraviolet spectroscopy and white light polarimetry of the extend ed solar corona during two 40 hour missions to occur in September 1994 and August 1995. The spectroscopy is done with an ultraviolet coronal spectrometer which measures the intensity and spectral line profile o f HI Ly alpha up to heliocentric heights of 3.5 solar radii. It also m easures the intensities of the OVI doublet at 1032 and 1037 Angstrom a nd of Fe XII at 1242 Angstrom. The HI Ly alpha line profile measuremen ts are used to determine the random velocity distribution of coronal p rotons along the line-of-sight. The absolute HI Ly alpha intensities c an be used together with electron densities from the white light coron agraph to estimate electron temperatures from hydrogen ionization bala nce calculations, and bulk outflow velocities from models of Doppler d immed resonant scattering. Intensities of minor ion lines are used to determine coronal abundances and outflow velocities of O5+. Ultraviole t spectroscopy of extended coronal regions from the 11 April 1993 miss ion of Spartan 201 are discussed.