Abstract
Until recently the theory of the photospheric structure has had a modest role. This situation has qualitatively changed with the appearance of the numerical simulations of Nordlund [1], Uus [2], Gadun [3], and others.
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To the memory of the late Prof. V.A. Krat
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Karpinsky, V.N. (1990). Properties Of The Solar Granulation. In: Stenflo, J.O. (eds) Solar Photosphere: Structure, Convection, and Magnetic Fields. International Astronomical Union, vol 138. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1061-4_7
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DOI: https://doi.org/10.1007/978-94-009-1061-4_7
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