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Conference Paper

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

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http://pubman.mpdl.mpg.de/cone/persons/resource/persons104142

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: http://hdl.handle.net/11858/00-001M-0000-0014-EAC4-5
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