Monochromatic images in stokes parameters and the structure of magnetic fields in sunspots
โ Scribed by Ye Shi-Hui; Jin Jie-Hai
- Publisher
- Springer
- Year
- 1986
- Tongue
- English
- Weight
- 475 KB
- Volume
- 104
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
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 vector magnetograph of the Marshall Space Flight Center, Huntsville (Alabama), we have found that the model of radial magnetic fields may give rise to 0 monochromatic images close to those observed. The same conclusion has been obtained previously by Landi Degl' Innocenti (1979), although his analysis was performed with the Milne-Eddington approximation instead of a detailed sunspot model. Moreover, we have shown that the model of spiral magnetic fields leads to results in contrast with observations. * The exact definitions of these quantities are given later by formulae (5).
๐ SIMILAR VOLUMES
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
We obtained simultaneous spectra with a spatial resolution of 89 and a temporal resolution of 15 s in Hc~, Can-K, Car1 8542 A, and three FeI lines of the sunspot group responsible for the large flares of August, 1972 (McMath No. 11976). A time series taken 1972, August 3 in the Fe16173 A. Zeeman sen