UVCS/SOHO: The First Two Years

Details UVCS/SOHO: The First Two Years UVCS/SOHO: The First Two Years

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ssrv...85..341c&link_type=abstract

Space Science Reviews, v. 85, Issue 1/2, p. 341-348 (1998).

Physics

5

Corona, Solar Wind, Uv Radiation, Spectroscopy, Line Profiles

Scientific paper

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.

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