Not much helicity is needed to drive large-scale dynamos
Understanding the in situ amplification of large-scale magnetic fields in turbulent astrophysical rotators has been a core subject of dynamo theory. When turbulent velocities are helical, large-scale dynamos that substantially amplify fields on scales that exceed the turbulent forcing scale arise, b...
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Autores principales: | Pietarila Graham, J., Blackman, E.G., Mininni, P.D., Pouquet, A. |
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Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_15393755_v85_n6_p_PietarilaGraham |
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