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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

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.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-EAC2-9 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-EAC3-7
Genre: Conference Paper

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 Creators:
Raouafi, N.-E.1, Author              
Lemaire, P., Author
Sahal-Bréchot, S., Author
Affiliations:
1IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290              

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Free keywords: -
 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: SOHO: SUMER
 Abstract: -

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 Dates: 2002
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: BibTex Citekey: Raouafi:2002-071
 Degree: -

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Title: Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO''
Source Genre: Proceedings
 Creator(s):
Wilson, A., Editor
Affiliations:
-
Publ. Info: Noordwijk : ESA Publ. Div.
Pages: - Volume / Issue: (ESA SP-508) Sequence Number: - Start / End Page: 403 - 406 Identifier: -