Wind data over two solar cycles shows the phase lag between A_He and SSN increases monotonically with v_SW; after lag correction, A_He matches at fixed SSN across phases and speeds.
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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.
Nonlinear hybrid models of PSP-observed anisotropic hot-beam ion VDFs produce combined ion-cyclotron and magnetosonic instabilities whose nonlinear stage yields qualitative agreement with observed hammerhead distributions.
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Helium Variation Across Two Solar Cycles Reveals A Speed-Dependent Phase Lag
Wind data over two solar cycles shows the phase lag between A_He and SSN increases monotonically with v_SW; after lag correction, A_He matches at fixed SSN across phases and speeds.