Dynamo models and the flip-flop phenomenon in late-type stars

Details Dynamo models and the flip-flop phenomenon in late-type stars Dynamo models and the flip-flop phenomenon in late-type stars

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mnras.352l..17m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 352, Issue 2, pp. L17-L20.

Astronomy and Astrophysics

Astronomy

36

Magnetic Fields, Stars: Activity, Stars: Late-Type, Stars: Magnetic Fields, Stars: Spots

Scientific paper

The `flip-flop' phenomenon has now been found to occur on several late-type stars: active longitudes, associated with dark regions of the surface, are seen to jump by 180°. A simple non-linear non-axisymmetric mean field dynamo model is described, in which for the first time magnetic behaviour is found that is akin to the observed flip-flop.

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