Ejection of bi-helical fields from the sun

Details Ejection of bi-helical fields from the sun Ejection of bi-helical fields from the sun

2003-12-19

arxiv.org/abs/astro-ph/0312543v1

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, to appear in Magnetic field and Helicity in the Sun and the Heliosphere, eds: D. Rust & B. Schmieder, ASP

Scientific paper

It is argued that much of the observed magnetic helicity losses at the solar
surface may represent a reduction of an otherwise more dominant nonlinearity of
solar and stellar dynamos. This nonlinearity is proportional to the internal
twist (as opposed to writhe) of helical and sigmoidal surface structures.

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