Magnetic helicity and the evolution of decaying magnetohydrodynamic turbulence.
Ensemble-averaged high resolution direct numerical simulations of reverse spectral transfer are presented, extending on the many single realization numerical studies done up to now. This identifies this type of spectral transfer as a statistical property of magnetohydrodynamic turbulence and thus permits reliable numerical exploration of its dynamics. The magnetic energy decay exponent from these ensemble runs has been determined to be nE=(0.47±0.03)+(13.9±0.8)/Rλ for initially helical magnetic fields. We show that even after removing the Lorentz force term in the momentum equation, thus decoupling it from the induction equation, reverse spectral transfer still persists. The induction equation is now linear with an externally imposed velocity field, thus amenable to numerous analysis techniques. A new door has opened for analyzing reverse spectral transfer, with various ideas discussed.
SUPA, School of Physics and Astronomy, University of Edinburgh, Peter Guthrie Tait Road EH9 3FD, United Kingdom.
Arjun
A
Berera
SUPA, School of Physics and Astronomy, University of Edinburgh, Peter Guthrie Tait Road EH9 3FD, United Kingdom.
Moritz
M
Linkmann
D003198:Computer Simulation; D057446:Hydrodynamics; D060328:Magnetic Phenomena