@article{ISI:000221253000044,
 abstract = {We derive relations for the decay of the kinetic and magnetic energies
and the growth of the Taylor and integral scales in unforced,
incompressible, homogeneous, and isotropic three-dimensional
magnetohydrodynamic (3DMHD) turbulence with power-law initial energy
spectra. We also derive bounds for the decay of the cross and magnetic
helicities. We then present results from systematic numerical studies of
such decay both within the context of a MHD shell model and direct
numerical simulations of 3DMHD. We show explicitly that our results
about the power-law decay of the energies hold for times t<t(*), where
t(*) is the time at which the integral scales become comparable to the
system size. For t<t(*), our numerical results are consistent with
those predicted by the principle of ``permanence of large eddies.″},
 article-number = {046304},
 author = {Kalelkar, C and Pandit, R},
 doi = {10.1103/PhysRevE.69.046304},
 eissn = {1550-2376},
 issn = {1539-3755},
 journal = {PHYSICAL REVIEW E},
 month = {APR},
 number = {4, 2},
 times-cited = {16},
 title = {Decay of magnetohydrodynamic turbulence from power-law initial
conditions},
 unique-id = {ISI:000221253000044},
 volume = {69},
 year = {2004}
}