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- W2950792922 abstract "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." @default.
- W2950792922 created "2019-06-27" @default.
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- W2950792922 date "2003-12-19" @default.
- W2950792922 modified "2023-10-16" @default.
- W2950792922 title "Ejection of bi-helical fields from the sun" @default.
- W2950792922 doi "https://doi.org/10.48550/arxiv.astro-ph/0312543" @default.
- W2950792922 hasPublicationYear "2003" @default.
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