Keywords (1)

Academic
Publications
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   (Citations: 10)
BibTex | RIS | RefWorks Download
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
Cumulative Annual
View Publication
The following links allow you to view full publications. These links are maintained by other sources not affiliated with Microsoft Academic Search.
Sort by: