Self-similar turbulent dynamo.
The amplification of magnetic fields in a highly conducting fluid is studied numerically. During growth, the magnetic field is spatially intermittent: it does not uniformly fill the volume, but is concentrated in long thin folded structures. Contrary to a commonly held view, intermittency of the fol...
Egile Nagusiak: | Schekochihin, A, Cowley, S, Maron, J, McWilliams, J |
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Formatua: | Journal article |
Hizkuntza: | English |
Argitaratua: |
2004
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Antzeko izenburuak
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Simulations of the small-scale turbulent dynamo
nork: Schekochihin, A, et al.
Argitaratua: (2004) -
Simulations of the small-scale turbulent dynamo
nork: Schekochihin, A, et al.
Argitaratua: (2004) -
Simulations of small-scale turbulent dynamo
nork: Schekochihin, A, et al.
Argitaratua: (2003) -
From small-scale dynamo to isotropic MHD turbulence
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Argitaratua: (2004) -
From Small-Scale Dynamo to Isotropic MHD Turbulence
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