The Fall 2000 and Fall 2001 SOHO-Ulysses quadratures

Citation
S. Suess et G. Poletto, The Fall 2000 and Fall 2001 SOHO-Ulysses quadratures, SPACE SCI R, 97(1-4), 2001, pp. 59-62
Citations number
2
Categorie Soggetti
Space Sciences
Journal title
SPACE SCIENCE REVIEWS
ISSN journal
00386308 → ACNP
Volume
97
Issue
1-4
Year of publication
2001
Pages
59 - 62
Database
ISI
SICI code
0038-6308(2001)97:1-4<59:TF2AF2>2.0.ZU;2-R
Abstract
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.