SOHO-Ulysses quadrature occurs when their included angle with the Sun is 90
degrees. At these times the same plasma leaving the Sun in the direction o
f Ulysses can first be remotely analyzed with SOHO and then later be sample
d in situ at Ulysses. Quadratures in Fall 2000/2001 are of special interest
because Ulysses will be near the south and north heliographic poles, respe
ctively, and it will be near sunspot maximum. But, the quadrature geometry
is complex - Ulysses is not in a true polar orbit and the orbital speed of
Ulysses and SOHO about the Sun will be comparable. In neither case is true
quadrature achieved, but this works to the observer's advantage. Here we sh
ow plots of the relative positions of SOHO and Ulysses throughout the two q
uadrature intervals.