Line ratio method applied to inter-network magnetic fields

Bibcode
2007msfa.conf..303K
Khomenko, E.; Collados, M.
Bibliographical reference

"Modern solar facilities - advanced solar science, Proceedings of a Workshop held at Göttingen September 27-29, 2006 ISBN 978-3-938616-84-0 382 pages, many illustrations, soft-bound, Price: 23.- Euros Published by Universitätsverlag Göttingen (http://univerlag.uni-goettingen.de The online edition (PDF, 12 MB) is available free of charge at: http://webdoc.sub.gwdg.de/univerlag/2007/solar_science_book.pdf, p.303"

Advertised on:
0
2007
Number of authors
2
IAC number of authors
0
Citations
1
Refereed citations
1
Description
We investigate the validity of the Stokes V amplitude ratio as an indicator of the magnetic field strength in solar inter-network regions with the help ofMHD simulations. We show that the Stokes V amplitude ratio of the Fe I 15652-15648 Å lines and Fe I 5247-5250 Å lines show a good correlation with the magnetic field strength even for magnetic fields with a complex internal structure like those in MHD simulations. However, in the latter case, the amplitude ratio sub-estimates the magnetic field strength, always revealing sub-kG values. The Stokes V amplitude ratio of the Fe I 6301-6302 Å lines shows no correlation with the magnetic field strength. The reasons of this behaviour are explained.
Type
Non-refereed

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