An analysis of the formation in magnetic field and the formation depth of seven solar photospheric Fe I lines.

Details An analysis of the formation in magnetic field and the formation depth of seven solar photospheric Fe I lines. An analysis of the formation in magnetic field and the formation depth of seven solar photospheric Fe I lines.

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990acaps..10...56s&link_type=abstract

(Acta Astrophysica Sinica, vol. 10, no. 1, 1990, p. 56-67) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 14, June 19

Astronomy and Astrophysics

Astrophysics

1

Line Spectra, Solar Magnetic Field, Zeeman Effect, Radiative Transfer, Stokes Law Of Radiation, Telescopes

Scientific paper

To meet the calibration demands of a multichannel solar magnetic telescope, the VAL quiet-sun atmosphere model is used to calculate the Stokes profiles of seven Fe I photospheric lines, their formation depths, and contribution functions. The results are (1) a more systematic picture of the features and properties of the abnormal and normal Zeeman lines and (2) an explanation of the appearance of sharp peaks in the formation-depth curves of the Stokes parameters Q and U near the line center.

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