Christoph U. Keller
Christoph U. Keller
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Solar Physics
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S.~K. Solanki
Latest
Infrared lines as probes of solar magnetic features. XV. Evershed flow in cool, weak penumbral fields
Center-to-limb variation of the second solar spectrum.
Inversion of Stokes V profiles: The structure of solar magnetic fluxtubes and its dependence on the filling factor.
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