The longitudinal magnetic field observation calibration of several solar photospheric Fe I lines for multichannel birefringence filter solar magnetic field telescope. II.

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Scientific paper

The changes of the formation depth of 6 Fe I lines, used by the multichannel birefringence filter solar magnetic field telescope, are studied. The mean square root errors at certain points from the line-center, corresponding to the narrowest and the widest bandwidth of the filter, are computed. Hence general properties of the formation depth of the normal and anomalous Zeeman lines passing through the multichannel filter, are summarized. The best place for the filter to be set from the line-center in an appropriate area, is obtained by computing the magnetic field response of Stokes V parameter.

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