๐”– Bobbio Scriptorium
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On fine structure of the magnetic field and brightness in the penumbrae of sunspots

โœ Scribed by H. I. Abdussamatov

Publisher
Springer
Year
1976
Tongue
English
Weight
353 KB
Volume
48
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

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 filaments seen in the space between the dark features cannot be attributed to the ordinary undisturbed photosphere.

๐Ÿ“œ SIMILAR VOLUMES

Fine structure and evershed motions in t
Fine structure and evershed motions in the sunspot penumbra
โœ D. J. Galloway ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Springer ๐ŸŒ English โš– 348 KB

The observed inhomogeneity of the intensity and Evershed motions means any model of the penumbra must be essentially inhomogeneous. A simple model is put forward in which the interaction of convection rolls with an initially homogeneous magnetohydrostatic sunspot field causes a concentration of flux

The crossover effect in sunspots and the
The crossover effect in sunspots and the fine structure of penumbra
โœ A. A. Golovko ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 577 KB

The peculiarities of magnetosensitive lines in the penumbral spectrum and the abnormal distribution of circular polarization in them are explained satisfactorily in terms of superposition of radiation originating in different elements of penumbral fine structure. Complicated asymmetric rvcontours ca