Magnetic field in a fluctuating ABC flow

Details Magnetic field in a fluctuating ABC flow Magnetic field in a fluctuating ABC flow

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009astl...35..321t&link_type=abstract

Astronomy Letters, Volume 35, Issue 5, pp.321-325

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The standard dynamo models that explain the origin of the large-scale magnetic fields of celestial bodies are related to the view of turbulent or convective flows as a locally statistically homogeneous and isotropic, but not mirror-symmetric, random field. Using an ABC flow, which is a classical example of a flow with deterministic chaos, we ascertain the extent to which the behavior of the magnetic field in such a flow is similar to the behavior of the magnetic field in mirror-asymmetric turbulence. Such a similarity has been found to be achieved if its coefficients A, B, and C are assumed to be random processes.

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