Dynamic alignment in MHD turbulence is a selective survival effect of intense small-angle events rather than a cascade-wide tendency toward collinearity.
For each 24-hour interval we compute the mean solar-wind speed Vsw =|⟨v(t)⟩ t| and an interval-level normalized cross helicity, σc = E+ −E − E+ +E − , E ± = D z±(t)− ⟨z ±⟩t 2E t
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Dynamic Alignment: A Fragile Survival Effect
Dynamic alignment in MHD turbulence is a selective survival effect of intense small-angle events rather than a cascade-wide tendency toward collinearity.