Streamer HI Ly-α Line Profiles During the Spartan 201-05/SOHO Coordinated Observations

Details Streamer HI Ly-α Line Profiles During the Spartan 201-05/SOHO Coordinated Observations Streamer HI Ly-α Line Profiles During the Spartan 201-05/SOHO Coordinated Observations

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.448.1193m&link_type=abstract

Magnetic Fields and Solar Processes. The 9th European Meeting on Solar Physics, held 12-18 September, 1999, in Florence, Italy.

Physics

Scientific paper

We present H I Lyalpha observations of coronal streamers obtained by UVCS/SOHO during the coordinated observations with UVCS/Spartan on 1 3 November 1998. Two different streamer regions were observed, one relatively stable above the Northeast limb, and a postCME streamer complex above the Southwest limb. H~I Lyalpha profiles and intensities were measured at ~1.5 and 2 Ro in the NE streamer and its boundary regions, and also at heights ranging from 1.5 to 2.5 Ro in the SW streamer complex. We analyze integrated intensities and line widths in each streamer structure.

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