On the spatial structure of a penumbra
β Scribed by R. B. Teplitskaya
- Publisher
- Springer
- Year
- 1985
- Tongue
- English
- Weight
- 242 KB
- Volume
- 95
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
A series of spatial intensity profiles across the sunspot penumbra is obtained at different wavelengths within the CaII K line (see Figure 1). A number of photometric properties of the penumbra are outlined, which may be useful for constructing a relevant inhomogeneous model.
π SIMILAR VOLUMES
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
We present a discussion of the gradual burst event on May 13, 1985 which is based on observations of the RATAN-600 telescope at ten fixed frequencies in the range between 37.5 and 0.95 GHz (0.8 and 31.6 cm wavelength) and on time profiles of patrol observations of the Observatory for Solar Radio Ast