Preliminary results from SPARTAN 201: coronal streamer observations

Details Preliminary results from SPARTAN 201: coronal streamer observations Preliminary results from SPARTAN 201: coronal streamer observations

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70..263s&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 263-266

Physics

7

Coronal Streamers, Solar Wind, Uv Spectroscopy

Scientific paper

The Ultraviolet Coronal Spectrometer on Spartan 201 obtained measurements of HI Ly α line profiles and O VI λ103.2/103.7 nm integrated intensities in a helmet streamer. Similar measurements were made on the solar disk to characterize the incident radiation which is the source for the resonantly scattered component of the lines. A description of the H I Ly α observations in the streamer will be presented. A more complete physical description of the observed coronal regions will become available after the analysis of additional data from coordinated observations made by visible coronagraphs and x-ray telescopes.

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