When unipolar sunspots are observed in the linearly polarized radiation represented by the Stokes parameters Q and U of magneto-sensitive spectral lines, their images display a complicated and interesting configuration. This is caused by the magneto-optical effect and also is connected with the 3-D structure of spot magnetic fields. In the process of numerical simulation it is possible to infer the regularity of variation of the angle of inclination of magnetic lines of force with distance from the spot center.
Ye SH,JIN, JH,YE, SH. Monochromatic images of sunspots in linearly polarized radiation and the structure of their magnetic fields[J]. SOLAR PHYSICS,1993,146(2):229-239.
APA
叶式煇,JIN, JH,&YE, SH.(1993).Monochromatic images of sunspots in linearly polarized radiation and the structure of their magnetic fields.SOLAR PHYSICS,146(2),229-239.
MLA
叶式煇,et al."Monochromatic images of sunspots in linearly polarized radiation and the structure of their magnetic fields".SOLAR PHYSICS 146.2(1993):229-239.
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