Abstract
It is confirmed that the penumbral bright grains are moving towards the sunspots umbra. At the umbra-penumbra boundary their horizontal velocity is about 0.5 km s−1 and their displacement is inclined downwards with an angle of 5° to 20°.
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References
Beckers, J. M. and Schröter, E. H.: 1969, Solar Phys. 10, 384.
Muller, R.: 1973, Solar Phys. 29, 55.
Schröter, E. H.: 1965, Z. Astrophys. 62, 228.
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Muller, R. Characteristics of the displacement of the penumbral bright grains of sunspots. Sol Phys 48, 101–102 (1976). https://doi.org/10.1007/BF00153335
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DOI: https://doi.org/10.1007/BF00153335