Large-scale KHI waves with vortex formation were observed from 6 to 14 solar radii in the upper corona during a fast CME, with growth rate qualitatively matching theoretical predictions.
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Turbulence from mixed-polarity magnetic carpet fields supplies enough dissipated energy to heat the solar chromosphere and lower corona, with gradual heating of spicules by entrained turbulence.
citing papers explorer
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Observation of Large-Scale Kelvin-Helmholtz Instability Wave Driven by a Coronal Mass Ejection
Large-scale KHI waves with vortex formation were observed from 6 to 14 solar radii in the upper corona during a fast CME, with growth rate qualitatively matching theoretical predictions.
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Turbulence and its Potential Impact on Solar Chromospheric and Coronal Heating
Turbulence from mixed-polarity magnetic carpet fields supplies enough dissipated energy to heat the solar chromosphere and lower corona, with gradual heating of spicules by entrained turbulence.