The Sun’s supergranulation

Abstract Supergranulation is a fluid-dynamical phenomenon taking place in the solar photosphere, primarily detected in the form of a vigorous cellular flow pattern with a typical horizontal scale of approximately 30–35 Mm, a dynamical evolution time of 24–48 h, a strong 300–400 m/s (rms) horizontal...

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Bibliographic Details
Main Authors: François Rincon, Michel Rieutord
Format: Article
Language:English
Published: Springer 2018-09-01
Series:Living Reviews in Solar Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/s41116-018-0013-5