Statistics – Computation
Scientific paper
Jun 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508..403r&link_type=abstract
In: Proceedings of the SOHO 11 Symposium on From Solar Min to Max: Half a Solar Cycle with SOHO, 11-15 March 2002, Davos, Switze
Statistics
Computation
Polarization, Resonance Scattering, Solar Wind, Sun: Magnetic Field
Scientific paper
Numerical computation results of the combination of the Hanle effect (due to the coronal magnetic field) and to the Doppler redistribution effect (due to the solar wind velocity field) on the linear polarization parameters of the O VI λ1032 coronal line (D2 line) are presented. Constraints on the magnetic field and the solar wind velocity field vectors are obtained by comparing the present results and the measurements of the polarization parameters of the O VI D2 coronal line by using SUMER/SoHO polarimetric observations done in the south coronal polar hole during the minimum of the solar activity cycle.
Lemaire Philippe
Raouafi Nour-Eddine
Sahal-Bréchot Sylvie
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