Magnetic Fields Across the Hertzsprung-Russell Diagram

By G. Mathys, S. Solanki, D. Wickramasinghe. 2001

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The solar magnetic field (2006, background): “Magnetic fields have been detected on many stars of various types [201].”
Starspots: A Key to the Stellar Dynamo (2005, methodology): “Most of our current knowledge about magnetic fields on cool stars and in starspots is, however, based on Zeeman broadening measurements, which reveal the distribution of magnetic field strengths with little dependence on the unknown field geometry (Robinson Jr, 1980; Saar, 1988; Valenti and Johns-Kr”
The surprising magnetic topology of τ Sco: fossil remnant or dynamo output? (2006, background): “At some point, all theories involve the coexistence of large-scale toroidal fields in stellar interiors and possibly even close to the surface (e.g., Braithwaite & Spruit 2004; Braithwaite & Nordlund 2006), which observations of magnetic Ap and Bp stars do not yet confirm (Moss 2001).”
Sunrise/IMaX OBSERVATIONS OF CONVECTIVELY DRIVEN VORTEX FLOWS IN THE SUN (2008, background): “These durations span from 5min to 20min with a mean of τ ≃ 7.9min and a standard deviation of 3.2min.”