Average radial structures of gas convection in the solar granulation

10 Jan 2020 Oba T. Iida Y. Shimizu T.

Gas convection is observed in the solar photosphere as the granulation, i.e., having highly time-dependent cellular patterns, consisting of numerous bright cells called granules and dark surrounding-channels called intergranular lanes. Many efforts have been made to characterize the granulation, which may be used as an energy source for various types of dynamical phenomena... (read more)

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  • SOLAR AND STELLAR ASTROPHYSICS