Volume 395, Number 3, December I 2002
|Page(s)||975 - 975|
|Section||Planets and planetary systems|
|Published online||18 November 2002|
UV line intensity and flow velocity distributions in two coronal mass ejections as deduced by UVCS-SOHO observations
Osservatorio Astrofisico, Città Universitaria, Via S. Sofia 78, 95125 Catania, Italy
2 Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
Corresponding author: R. Ventura, email@example.com
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© ESO, 2002
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