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The comparison of the magnetographic magnetic field measured in different spectral lines

# The comparison of the magnetographic magnetic field measured in different spectral lines,10.1007/BF00152808,Solar Physics,S. I. Gopasyuk,V. A. Kotov,A

The comparison of the magnetographic magnetic field measured in different spectral lines
The discrepancies in the values of longitudinal magnetic field obtained from magnetographic records in different spectral lines are considered. On the basis of extensive data including 60 pairs of magnetographic maps for 11 spectral lines, obtained simultaneously for one of these lines and ?6103 with the aid of the Crimean double channel magnetograph, the following conclusions have been reached. The relative field strength $$\delta (\lambda i) = {{H\parallel (\lambda _i )} \mathord{\left/ {\vphantom {{H\parallel (\lambda _i )} {H\parallel }}} \right. \kern-\nulldelimiterspace} {H\parallel }}$$ (6103) depends partly on the distance from the center of the disk (Figure 4) and mainly on the magnetic sensitivity of the line g?2 (Figure 3), pointing to the primary role of saturation effect. The possible influence of line asymmetry on these discrepancies is also suggested.
Journal: Solar Physics - SOL PHYS , vol. 31, no. 2, pp. 307-316, 1973
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## References (6)

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Journal: Solar Physics - SOL PHYS , vol. 22, no. 2, pp. 402-417, 1972

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Published in 1942.
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## Citations (10)

### Fine structure of solar magnetic fields

Journal: Bulletin of The Crimean Astrophysical Observatory , vol. 106, no. 1, pp. 49-53, 2010

### Two-dimensional MHD models of solar magnetogranulation. Dynamics of magnetic elements

Published in 2010.

### Spectro-Polarimetric Observations of Solar Magnetic Fields and the SOHO/MDI Calibration Issue

Journal: Solar Physics - SOL PHYS , vol. 260, no. 2, pp. 261-270, 2009

### Comparison of Solar Magnetic Fields Measured at Different Observatories: Peculiar Strength Ratio Distributions Across the Disk(Citations: 3)

Journal: Solar Physics - SOL PHYS , vol. 250, no. 2, pp. 279-301, 2008

### Observational evidences for multi-component magnetic field structure in solar flares(Citations: 1)

Journal: Journal of Astrophysics and Astronomy - J ASTROPHYS ASTRON , vol. 29, no. 3, pp. 387-404, 2008