2014
DOI: 10.1017/jfm.2013.561
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Purely helical absolute equilibria and chirality of (magneto)fluid turbulence

Abstract: Purely helical absolute equilibria of incompressible neutral fluids and plasmas (electron, singlefluid and two-fluid magnetohydrodyanmics) are systematically studied with the help of helical (wave) representation and truncation, for genericities and specificities about helicity. A unique chirality selection and amplification mechanism and relevant insights, such as the one-chiralsector-dominated states, among others, about (magneto)fluid turbulence follow.

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Cited by 29 publications
(60 citation statements)
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“…Our main point is that the two extreme values ±1 for Pm found in the above are for linear waves, which themselves may not be appropriate in the case of their simulation without a guide field B0 (though large-scale magnetic fluctuations might be coarsegrained to be a local guide field, the situation would be much more complicated), and may not be appropriate for characterizing eMHD and iMHD turbulence. But, the insight that the turbulence is dominated by the iMHD and eMHD flow respectively at subsequent scale regimes, which may be termed one-flow-dominated state (OFDS), is valuable and the proper nonlinear theory may be a combination of the one-chiral-sector-dominated state (OCSDS -a state dominated by the '+' or the '-' chiral sector: Zhu, Yang & Zhu 2014) with OFDS: Having neither introduced the mean magnetic field (i.e, B may be just b), nor linearized the models, we have for uni-chiral case, σm = s = −σc, i.e.,…”
Section: Nonlinear Chirality Beyond Linear Cyclotron Wavesmentioning
confidence: 99%
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“…Our main point is that the two extreme values ±1 for Pm found in the above are for linear waves, which themselves may not be appropriate in the case of their simulation without a guide field B0 (though large-scale magnetic fluctuations might be coarsegrained to be a local guide field, the situation would be much more complicated), and may not be appropriate for characterizing eMHD and iMHD turbulence. But, the insight that the turbulence is dominated by the iMHD and eMHD flow respectively at subsequent scale regimes, which may be termed one-flow-dominated state (OFDS), is valuable and the proper nonlinear theory may be a combination of the one-chiral-sector-dominated state (OCSDS -a state dominated by the '+' or the '-' chiral sector: Zhu, Yang & Zhu 2014) with OFDS: Having neither introduced the mean magnetic field (i.e, B may be just b), nor linearized the models, we have for uni-chiral case, σm = s = −σc, i.e.,…”
Section: Nonlinear Chirality Beyond Linear Cyclotron Wavesmentioning
confidence: 99%
“…The usage of linear-wave argument is 'popular' in plasma literatures, which, in many cases are not necessary; for instance, relevant to our notion, it appears to us that the interesting hodographs of He, Tu, Marsch & Yao (2012) for chiral magnetic fluctuations (see also Telloni & Bruno 2016) may not necessarily be related to just linear waves. Note also that OCSDS requires non-vanishing (generalized) helicity (Zhu, Yang & Zhu 2014), whose origin/emergence should also be addressed.…”
Section: Nonlinear Chirality Beyond Linear Cyclotron Wavesmentioning
confidence: 99%
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