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From small-scale dynamo to isotropic MHD turbulence

Abstract:

We consider the problem of incompressible, forced, nonhelical, homogeneous, isotropic MHD turbulence with no mean magnetic field. This problem is essentially different from the case with externally imposed uniform mean field. There is no scale-by-scale equipartition between magnetic and kinetic energies as would be the case for the Alfvén-wave turbulence. The isotropic MHD turbulence is the end state of the turbulent dynamo which generates folded fields with small-scale direction reversals. W...

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Publication status:
Published

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Journal:
ASTROPHYSICS AND SPACE SCIENCE
Volume:
292
Issue:
1-4
Pages:
141-146
Publication date:
2004-01-01
DOI:
ISSN:
0004-640X
URN:
uuid:57178fb3-93e1-458c-88fe-1f5b9926deac
Source identifiers:
161172
Local pid:
pubs:161172
Language:
English
Keywords:

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