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

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

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cha%26a..14..155s&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 14, Issue 2, p. 155-166.

Astronomy and Astrophysics

Astrophysics

Sun, Magnetic Field, Spectral Lines

Scientific paper

To meet the calibration demands of the multi-channel solar magnetic telescope, we took the VAL quiet Sun atmosphere model and calculated the Stokes profiles of seven FeI photospheric lines, their formation depths, and contribution functions, thereby obtaining a more systematic picture of the features and properties of the abnormal and normal Zeeman lines and an explanation of the appearance of sharp peaks in the formation depth curves of the Stokes parameters Q and U near the line centre.

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