Effect of the solar wind velocity field vector on the polarization of the O VI 
λ1032 coronal line

Raouafi, N.-E.; Sahal-Bréchot, S.; Lemaire, P.

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Effect of the solar wind velocity field vector on the polarization of the O VI λ1032 coronal line

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Raouafi, N.-E.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

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Raouafi, N.-E., Sahal-Bréchot, S., & Lemaire, P. (2002). Effect of the solar wind velocity field vector on the polarization of the O VI λ1032 coronal line. In A. Wilson (Ed.), Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'' (pp. 471-474). Noordwijk: ESA Publ. Div.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-EAC4-5

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