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, firstname.lastname@example.org
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© ESO, 2002