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UVCS/SOHO: The First Two Years (1998)

Cranmer, S. R. ; Kohl, J. L. ; Noci, G.

Springer

Space science reviews 85 (1998), S. 341-348

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Details

ISSN: 1572-9672

Schlagwort(e): Corona ; Solar Wind ; UV Radiation ; Spectroscopy ; Line Profiles

Quelle: Springer Online Journal Archives 1860-2000

Thema: Physik

Notizen: 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.

Materialart: Digitale Medien

URL: http://dx.doi.org/10.1023/A:1005175106042

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