Theory of line formation depth and its application. (III): Derivation of the structure of solar vector magnetic fields.

Details Theory of line formation depth and its application. (III): Derivation of the structure of solar vector magnetic fields. Theory of line formation depth and its application. (III): Derivation of the structure of solar vector magnetic fields.

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pabei..15..303q&link_type=abstract

Prog. Astron., Vol. 15, No. 4, p. 303 - 311

Astronomy and Astrophysics

Astronomy

Line Formation: Radiative Transfer, Solar Magnetic Fields: Structure

Scientific paper

The application of the theory of line formation depth to the derivation
of the structure of solar magnetic fields is described and some typical
samples are given. It is pointed out that it is more excellent for the
response function to derive the structure of the line parameters than
for the contribution function.

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