Abstract
Photoelectric measurements of monochromatic spot intensities obtained with the domeless Coudé refractor in Anacapri are given. The scattered light superimposed on the spot, as deduced from measurements outside the sun's limb, amounts on the average to about 4% of the photospheric intensity. The accuracy of the derived spot intensities is better than 10%. Two of four investigated spots yielded temperatures below 3900K (ΔΘ > 0.5).
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References
Birkle, K. and Mattig, W.: 1965, Z. Astrophys. 60, 264.
David, K. H. and Elste, G.: 1962, Z. Astrophys. 54, 12.
Deubner, F. L.: 1966, in The Fine Structure of the Solar Atmosphere, Proceedings of Capri Colloquium, p. 26.
Fricke, K. and Elsässer, H.: 1965, Z. Astrophys. 63, 35.
Zwaan, C: 1965, Rech. Inst. Astron. Utrecht 17, (4).
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Kneer, F., Mattig, W. Sunspot intensities and their correction for scattered light. Sol Phys 5, 42–49 (1968). https://doi.org/10.1007/BF00147118
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DOI: https://doi.org/10.1007/BF00147118