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Oscillatory migrato...
Oscillatory migratory large-scale fields in mean-field and direct simulations
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Mitra, Dhrubaditya (författare)
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Tavakol, Reza (författare)
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- Brandenburg, Axel (författare)
- Stockholms universitet,Institutionen för astronomi,Nordiska institutet för teoretisk fysik (Nordita)
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Käpylä, Petri J. (författare)
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(creator_code:org_t)
- 2009
- 2009
- Engelska.
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Ingår i: Proceedings of the International Astronomical Union. - 1743-9213 .- 1743-9221. ; 5, s. 197-201
- Relaterad länk:
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https://urn.kb.se/re...
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https://doi.org/10.1...
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Abstract
Ämnesord
Stäng
- We summarise recent results form direct numerical simulations of both non-rotating helically forced and rotating convection driven MHD equations in spherical wedge-shape domains. In the former, using perfect-conductor boundary conditions along the latitudinal boundaries we observe oscillations, polarity reversals and equatorward migration of the large-scale magnetic fields. In the latter we obtain angular velocity with cylindrical contours and large-scale magnetic field which shows oscillations, polarity reversals but poleward migration. The occurrence of these behviours in direct numerical simulations is clearly of interest. However the present models as they stand are not directly applicable to the solar dynamo problem. Nevertheless, they provide general insights into the operation of turbulent dynamos.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Nyckelord
- MHD
- convection
- Sun: magnetic fields
Publikations- och innehållstyp
- ref (ämneskategori)
- art (ämneskategori)
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