UVCS/SOHO: The First Two Years |
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| Authors: | S R Cranmer J L Kohl G Noci |
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| Institution: | (1) Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA, USA;(2) Università di Firenze, I-50125 Firenze, Italy |
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| Abstract: | The SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) has observed the extended solar corona between 1 and 10 R· for more
than two years. We review spectroscopic and polarimetric measurements made in coronal holes, equatorial streamers, and coronal
mass ejections, as well as selected non-solar targets. UVCS/SOHO has provided a great amount of empirical information about
the physical processes that heat and accelerate the solar wind, and about detailed coronal structure and evolution.
This revised version was published online in June 2006 with corrections to the Cover Date. |
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| Keywords: | Corona Solar Wind UV Radiation Spectroscopy Line Profiles |
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