Other
Scientific paper
Oct 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.446..567r&link_type=abstract
8th SOHO Workshop: Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona. Proceedings of the Conference hel
Other
Scientific paper
The linear polarization parameters of the O VI 103.2 nm coronal line are sensitive to the magnetic field and the solar wind velocity vector effects (via the Hanle effect and the Doppler dimming effect respectively). These parameters (degree and direction of linear polarization) are measured by interpreting observations taken by the SUMER spectrometer aboard of SOHO. SUMER is sensitive to the linear polarization state of the observed radiation. The profile and the shift of the O VI 103.2 nm and 103.7 nm lines and of the other lines measured during the observations will also be reported. These results should permit to obtain information on the velocity distribution of the coronal O VI ions.
Lemaire Philippe
Raouafi Nour-Eddine
Sahal-Bréchot Sylvie
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