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• W2497729047 abstract "The magnetic field of the Sun is mainly concentrated into intense magnetic flux tubes having field strengths of the order of 1 kG. In this paper an overview is given of the thermal and magnetic properties of these flux tubes, which are known to exhibit a large range in size, from the smallest magnetic elements to sunspots. Differences and similarities between the largest and smallest features are stressed. Some thoughts are also presented on how the properties of magnetic flux tubes are expected to scale from the solar case to that of solar-like stars. For example, it is pointed out that on giants and supergiants turbulent pressure may dominate over gas pressure as the main confining agent of the magnetic field. Arguments are also presented in favour of a highly complex magnetic geometry on very active stars. Thus the very large starspots seen in Doppler images probably are conglomerates of smaller (but possibly still sizable) spots." @default.
• W2497729047 created "2016-08-23" @default.
• W2497729047 creator A5048198842 @default.
• W2497729047 date "1996-01-01" @default.
• W2497729047 modified "2023-09-23" @default.
• W2497729047 title "Solar and stellar magnetic flux tubes" @default.
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• W2497729047 doi "https://doi.org/10.1017/s0074180900083236" @default.
• W2497729047 hasPublicationYear "1996" @default.
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