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Line Formation in Inhomogeneous Magnetic Fields

Published online by Cambridge University Press:  14 August 2015

R. Göhring
R. Göhring*
Affiliation:
Fraunhofer Institut, Freiburg, Germany

Extract

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Until now, analytic solutions for the problem of line formation in magnetic fields have been given only under special assumptions concerning either the magnetic field or the atmospheric model. Conditions are given for which the system of differential equations can be solved analytically. For the general case a method is given to solve the system in approximation and analytically. LTE is generally assumed which means that we use the system given by Unno (1956) or that given by Beckers (1969) including the Faraday rotation.

Type
Part II: The Interpretation of Magnetograph Results – The Formation of Absorption Lines in a Magnetic Field
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 162 - 164
Copyright
Copyright © Reidel 1971 

References

Beckers, J. M.: 1969, Solar Phys. 9, 372.Google Scholar
Göhring, R.: 1970, , Freiburg.Google Scholar
Holweger, H.: 1967, Z. Astrophys. 65, 365.Google Scholar
Hubenet, H.: 1955, Z. Astrophys. 35, 245.Google Scholar
Kjeldseth Moe, O.: 1968, Solar Phys. 4, 267.Google Scholar
Kneer, F.: 1970, , Freiburg.Google Scholar
Mattig, W.: 1966, in Atti del Convegno Sui Campi Magnetici Solari (ed. by Cimino, M.), G. Barbèra. Firenze = Mitt. Fraunhofer Inst. Nr. 62.Google Scholar
Michard, R.: 1961, Compt. Rend. 253, 2857.Google Scholar
Unno, W.: 1956, Publ. Astron. Soc. Japan 8, 108.Google Scholar
Wiehr, E.: 1968, , Göttingen.Google Scholar