English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
 
 
DownloadE-Mail
 DetailsSummary
  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.

Item is

 

show all hide all

Basic

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

Files

show Files

Locators

show

Creators

show
hide
 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              

Content

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

Details

show
hide
Language(s):
 Dates: 2002
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: BibTex Citekey: Raouafi:2002-071
 Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show
hide
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: -