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.
M., Nykyri, K., & Farrugia, C
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MMS observations document turbulence spectra and electron-scale reconnection signatures inside Kelvin-Helmholtz waves during a geomagnetic storm.
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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 properties and kinetic signatures of electron in Kelvin-Helmholtz waves during a geomagnetic storm
MMS observations document turbulence spectra and electron-scale reconnection signatures inside Kelvin-Helmholtz waves during a geomagnetic storm.