UVCS/SOHO observations of coronal streamers

Details UVCS/SOHO observations of coronal streamers UVCS/SOHO observations of coronal streamers

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..235f&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 235-238 (1999).

Physics

Ultraviolet

Scientific paper

We used the Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) to obtain line profiles in mid-latitude coronal streamers between 1.3 Rsolar and 5.5 Rsolar during a period of moderate solar activity. We present a summary of the preliminary results. These results clearly indicate that the mid-latitude streamers observed during this time period have very different spectral properties than the equatorial streamers observed near solar minimum.

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