The abstract is below, and I've made a ps version of the paper which can be downloaded from:

ftp://ws2.scibernet.com

password: your E-mail address

cd pub/outgoing/wsm-riley-paper

Unfortunately, I cannot easily make ps files of two of the figures. If you want them, please let me know and I can either fax you a copy, or mail you a copy.

If you have any questions, please E-mail me. uk2@scibernet.com


Relationship Between Ulysses Plasma Observations and Solar Observations
during the Whole Sun Month Campaign

Pete Riley, J. T. Gosling, D. J. McComas, V. J. Pizzo, J. G. Luhmann, D.
Biesecker, R. J. Forsyth, J. T. Hoeksema, A. Lecinski, B. J. Thompson

In this report, we summarize measurements made by the plasma experiment on
the Ulysses spacecraft during the period designated as ``Whole Sun Month''
(WSM, August 10 - September 8, 1996).  This interval coincided with the
return of solar wind variability at Ulysses. Ulysses was located at $\sim
28\deg N$ heliographic latitude, at a heliocentric distance of 4.25 AU, and
on the opposite side of the Sun from Earth.  In particular, we explore the
evolution of the solar wind between the Sun and Ulysses for several
rotations surrounding WSM.  Specifically, we map Ulysses measurements back
toward the Sun by applying a 2--dimensional inverse--MHD algorithm.  This
approach is compared with the commonly used constant speed (or ballistic)
approximation.  We find that the MHD mapping technique produces
substantially better results when compared with solar observations.  Both
the Ulysses MHD--mapped results and the solar observations are consistent
with a picture of a modestly tilted streamer belt ($< 10 \deg$) that was
deformed northward by an active region at $240 - 270 \deg$ longitude.