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astro-ph.SR2023★ 1 cited
Reflection-driven turbulence in the super-Alfvénic solar wind
Romain Meyrand, Jonathan Squire, Alfred Mallet +1
In magnetized, stratified astrophysical environments such as the Sun's corona and solar wind, Alfvénic fluctuations ''reflect'' from background gradients, enabling nonlinear intera…
astro-ph.SR2023
Electron-ion heating partition in imbalanced solar-wind turbulence
Jonathan Squire, Romain Meyrand, Matthew W. Kunz
A likely candidate mechanism to heat the solar corona and solar wind is low-frequency "Alfvénic" turbulence sourced by magnetic fluctuations near the solar surface. Depending on it…