Ejection of bi-helical fields from the sun

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dc.creatorBrandenburg, A.
dc.creatorBlackman, E. G.
dc.date2003-12-19
dc.date.accessioned2026-07-07T02:11:41Z
dc.date.available2026-07-07T02:11:41Z
dc.descriptionIt 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.
dc.description4 pages, 2 figures, to appear in Magnetic field and Helicity in the Sun and the Heliosphere, eds: D. Rust & B. Schmieder, ASP Conference Series, XXV JD3 (2003)
dc.identifierhttps://arxiv.org/abs/astro-ph/0312543
dc.identifierhttp://arxiv.org/abs/astro-ph/0312543
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7181
dc.subjectAstrophysics
dc.titleEjection of bi-helical fields from the sun
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