Parker spiral geometry reduces perpendicular outer scales in reflection-driven turbulence, slowing the nonlinear turnover time growth and enabling greater heating and sustained cross-helicity imbalance compared to radial-field models.
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The influence of Parker spiral on the reflection-driven turbulence
Parker spiral geometry reduces perpendicular outer scales in reflection-driven turbulence, slowing the nonlinear turnover time growth and enabling greater heating and sustained cross-helicity imbalance compared to radial-field models.