Bibcode
Khomenko, E.; Collados, M.
Referencia bibliográfica
"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"
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2007
Número de citas
1
Número de citas referidas
1
Descripción
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.