Imbalanced turbulence throttles its cascade via the helicity barrier, yielding flat spectra (η<2) that invert minor-ion heating to Q_i ∝ Q_p A_i (A_i/Z_i)^{η-2}, with simulations across β_p0 confirming the (A_i/Z_i)^a trend and strong perpendicular heating at low β.
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2026 2representative citing papers
New ergodicity-based ACF estimator and integral timescale methodology for solar wind turbulence claimed to eliminate artificial interval-length dependence.
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Minor Ions as a Diagnostic of Solar Wind Heating: Inverted Mass-to-Charge Scaling in Imbalanced Turbulence
Imbalanced turbulence throttles its cascade via the helicity barrier, yielding flat spectra (η<2) that invert minor-ion heating to Q_i ∝ Q_p A_i (A_i/Z_i)^{η-2}, with simulations across β_p0 confirming the (A_i/Z_i)^a trend and strong perpendicular heating at low β.
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The integral and correlation scales of solar wind turbulence
New ergodicity-based ACF estimator and integral timescale methodology for solar wind turbulence claimed to eliminate artificial interval-length dependence.