The Connection of Fine-Structure Photospheric Features in Active Regions with Magnetic Fields

N. V. Steshenko

doi:10.1007/978-94-011-6815-1_29

The Connection of Fine-Structure Photospheric Features in Active Regions with Magnetic Fields

N. V. Steshenko

https://doi.org/10.1007/978-94-011-6815-1_29

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Publication Date: Jan 1, 1968

Citations: 1

Affiliation: Special Astrophysical Observatory

#Features In Active Regions #Penumbral Filaments + Show 6 more

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Abstract

1. The fine structure of the proton sunspot group of July 4–8, 1966 was studied on the basis of high-resolution heliograms. The comparison of the orientation between penumbral filaments and the transverse magnetic fields (observed by A.B. Severny and T. T. Tsap) shows that the direction of the filaments coincides in general with that of the magnetic field.

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