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Effect of the coronal magnetic field and the solar wind velocity field vectors on the polarization of the O VI λ1032 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., Lemaire, P., & Sahal-Bréchot, S. (2002). Effect of the coronal magnetic field and the solar wind velocity field vectors on the polarization of the O VI λ1032 line. In A. Wilson (Ed.), Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'' (pp. 403-406). Noordwijk: ESA Publ. Div.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-EAC2-9
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