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. 2017 Feb 22;4(2):160271. doi: 10.1098/rsos.160271

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© 2017 The Authors.

Published by the Royal Society under the terms of the Creative Commons Attribution License http://creativecommons.org/licenses/by/4.0/, which permits unrestricted use, provided the original author and source are credited.

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Figure 8. — Poloidal field configurations. (a) All field lines close outside the star, this field is unstable by an argument due to Flowers & Ruderman [78]. For the case where some field lines are closed inside the star, instability was demonstrated by Markey & Tayler [79,80] and Wright [81].