Magnetic field strength in solar flux tubes - A model atmosphere independent determination
The "line ratio method" (Stenflo, 1973) has been extensively used in the past to carry out measurements of the magnetic field strength in spatially unresolved magnetic flux concentrations. The authors present here a new variant of this technique, which is particularly simple as it does not depend on any radiative transfer calculations and thus the
Sanchez Almeida, J. et al.
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1988