𝔖 Bobbio Scriptorium
✦   LIBER   ✦

FLOCCULAR MASSES AND APPARENT ALTERATIONS IN SUNSPOT PENUMBRAE

✍ Scribed by BARTLETT, J. C.

Book ID
121138241
Publisher
American Association for the Advancement of Science
Year
1944
Tongue
English
Weight
95 KB
Volume
99
Category
Article
ISSN
0036-8075

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πŸ“œ SIMILAR VOLUMES

Fine structure and evershed motions in t
Fine structure and evershed motions in the sunspot penumbra
✍ D. J. Galloway πŸ“‚ Article πŸ“… 1975 πŸ› Springer 🌐 English βš– 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
✍ A. A. Golovko πŸ“‚ Article πŸ“… 1974 πŸ› Springer 🌐 English βš– 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

On fine structure of the magnetic field
On fine structure of the magnetic field and brightness in the penumbrae of sunspots
✍ H. I. Abdussamatov πŸ“‚ Article πŸ“… 1976 πŸ› Springer 🌐 English βš– 353 KB

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