Abstract
The nonlinear dynamics of kinetic-Alfvén–wave (KAW)
turbulence is studied. Weak
KAW turbulence induced by three-wave interaction among parallel-propagating
KAWs has a direct energy cascade in the wavenumber domain
ks⊥>ρ−1i
and an inverse cascade in the domain
ks⊥<ρ−1i,
resulting in Kolmogorov-type spectra,
Wk∼(kz)
−1/2(k⊥)−p,
with exponents p=4 and p=3.5 respectively. The interaction
including
antiparallel-propagating KAWs, usually most effective, results in an inverse
energy
cascade over the whole k⊥ range and p=2
(at
k⊥<ρ−1i)
and
p=3.5 (for
k⊥>ρ−1i)
spectra.
Three applications concerning KAW turbulence in flaring loops, in the Earth's
magnetosphere and in tokamaks are considered. It is suggested that turbulent
KAW spectra
are common in space plasmas.
Publisher
Cambridge University Press (CUP)
Cited by
32 articles.
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4. Turbulence in space plasmas and beyond;Journal of Physics A: Mathematical and Theoretical;2018-06-12
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