Abstract
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.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsReferences
Beckers, J. M.: 1969, Solar Phys. 9, 372.
Göhring, R.: 1970, Dissertation, Freiburg.
Holweger, H.: 1967, Z. Astrophys. 65, 365.
Hubenet, H.: 1955, Z. Astrophys. 35, 245.
Kjeldseth Moe, O.: 1968, Solar Phys. 4, 267.
Kneer, F.: 1970, Dissertation, Freiburg.
Mattig, W.: 1966, in Atti del Convegno Sui Campi Magnetici Solari (ed. by M Cimino), G. Barbèra.
Firenze = Miti. Fraunhofer Inst. Nr. 62.
Michard, R.: 1961, Compt. Rend. 253, 2857.
Unno, W.: 1956, Publ. Astron. Soc. Japan 8, 108.
Wiehr, E.: 1968, Dissertation, Göttingen.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1971 International Astronomical Union
About this chapter
Cite this chapter
Göhring, R. (1971). Line Formation in Inhomogeneous Magnetic Fields. In: Howard, R. (eds) Solar Magnetic Fields. International Astronomical Union / Union Astronomique Internationale, vol 43. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3117-2_20
Download citation
DOI: https://doi.org/10.1007/978-94-010-3117-2_20
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3119-6
Online ISBN: 978-94-010-3117-2
eBook Packages: Springer Book Archive