First Results from the Soho Ultraviolet Coronagraph Spectrometer


The SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) is being used to observe the extended solar corona from 1.25 to 10 R from Sun center. Initial observations of polar coronal holes and equatorial streamers are described. The observations include measurements of spectral line profiles for H I L and L , O VI 1032 Å and 1037 Å, Mg X 625 Å, Fe XII 1242… (More)


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@inproceedings{Kohl2003FirstRF, title={First Results from the Soho Ultraviolet Coronagraph Spectrometer}, author={John L. Kohl and Giancarlo Noci and Ester Antonucci and G. Tondello and Martin E. Huber and Larry D. Gardner and Placido Nicolosi and L. Strachan and Silvano Fineschi and John C. Raymond and Marco Romoli and D. Spadaro and A. PANASYUK and Oswarld H. W. Siegmund and Carlo Benna and A. CIARAVELLA and Steven R Cranmer and Stefano Giordano and M. KAROVSKA and R. Martin and J. G. Michels and Andrea Modigliani and G Naletto and Chiara Pernechele and Giannina Poletto and Pauline L Smith}, year={2003} }