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Influence of surface stressing on stellar coronae and winds

M Jardine,A A Vidotto,A Van Ballegooijen, J F Donati,J Morin,R Fares,Tamas I Gombosi

Monthly Notices of the Royal Astronomical Society（2013）

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Abstract
The large-scale field of the Sun is well represented by its lowest energy (or potential) state. Recent observations, by comparison, reveal that many solar-type stars show large-scale surface magnetic fields that are highly non-potential – that is, they have been stressed above their lowest energy state. This non-potential component of the surface field is neglected by current stellar wind models. ...
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Key words
magnetic fields,stars: coronae,stars: winds, outflows
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