Taking into account magneto-optical effects, we have obtained numerical solutions of the transfer equations for the Stokes parameters, calculated the linearly polarized intensity (0) and constructed its monochromatic images of unipolar sunspots. By comparison with the observational material of the v
Monochromatic images of sunspots in linearly polarized radiation and the structure of their magnetic fields
β Scribed by Shi-Hui Ye; Jie-Hai Jin
- Publisher
- Springer
- Year
- 1993
- Tongue
- English
- Weight
- 403 KB
- Volume
- 146
- Category
- Article
- ISSN
- 0038-0938
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From investigating spectrograms of penumbrae of some sunspots it is concluded that the maximum magnetic field strength occurs in dark filaments and amounts to 1800-1900 G; the intensity of the magnetic field in dark filaments is 100-400 G larger than in the neighbouring bright filaments; the bright
In continuation of our earlier investigation (referred to hereafter as part I) where we considered the mathematically simple case of magnetic ΓΏeld orientation along the Z-axis of the principal axes frame (PAF) of the electric quadrupole ΓΏeld, we take up here the general problem of arbitrary orientat