Abstract
Based on pinhole photometer observations in 4–6 wavelength regions we have searched for a connection between the intensities of the umbra and the penumbra of sunspots. For the 1.67 μm wavelength region it is apparent that spots with dark umbrae also have dark penumbrae. In the other wavelength regions similar relations are found. The darkness of the spot is probably connected with the degree of complexity of the spot.
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References
Ekmann, G. and Maltby, P.: 1974, Solar Phys. 35, 317.
Eriksen, G. and Maltby, P.: 1973, in I. Xanthakis (ed.), Proc. First Europ. Astron. Meeting, Solar Activity and Related Interplanetary and Terrestrial Phenomena, Vol. I, p. 87.
Hall, D. N. B.: 1973, An Atlas of Infrared Spectra of the Solar Photosphere and of Sunspot Umbrae, Kitt Peak National Observatory.
Kjeldseth Moe, O. and Maltby, P.: 1974, Solar Phys. 36, 109.
Maltby, P.: 1972, Solar Phys. 26, 76.
Mykland, N.: 1973, Solar Phys. 28, 49.
Rossbach, M. and Schröter, E. H.: 1970, Solar Phys. 12, 95.
Staveland, L.: 1972, Inst. Theor. Astrophysics Report, No. 36.
Zwaan, C.: 1965, Rech. Astron. Obs. Utrecht. 17, Part 4.
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Ekmann, G. The relation between the intensities of umbra and penumbra of large sunspots. Sol Phys 38, 73–75 (1974). https://doi.org/10.1007/BF00161825
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DOI: https://doi.org/10.1007/BF00161825