Abstract
Solar granules are classified into four groups according to their shapes and splitting by sharp rifts crossing them. The appearance and evolution of ‘white-light dark networks’ is described.
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References
Bahng, J. and Schwarzschild, M.: 1961, Astrophys. J. 134, 312.
Beckers, J. M.: 1966, in K. O. Kiepenheuer (ed.), The Fine Structure of the Solar Atmosphere, Franz Steiner Verlag, Heisbaden.
Bray, R. J. and Loughhead, R. E.: 1977, Solar Phys. 54, 319.
Bray, R. J., Loughhead, R. E., and Durrant, C. J.: 1984, The Solar Granulation, Cambridge University Press, Cambridge.
Harvey, J. W.: 1965, Publ. Astron. Soc. Pacific 77, 129.
Kitai, R. and Hawaguchi, I.: Solar Phys. 64, 3.
Koutchmy, S.: 1977, Solar Phys. 54, 268.
Rösch, J.: 1959, Am. Astrophys. 22, 584.
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Graves, J.E., Pierce, A.K. The morphology of solar granulations and dark networks. Sol Phys 106, 249–250 (1986). https://doi.org/10.1007/BF00158495
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DOI: https://doi.org/10.1007/BF00158495