The non-linear evolution of the tearing mode in electromagnetic turbulence using gyrokinetic simulations
William A Hornsby, Pierluigi Migliano, Rico Buchholz, Stefan, Grosshauser, Arne Weikl, David Zarzoso, Francis J Casson, Emanuele Poli,, Artur G Peeters

TL;DR
This study uses gyrokinetic simulations to analyze how electromagnetic turbulence influences the non-linear evolution of magnetic islands, revealing turbulence's role in seeding, modifying growth, and affecting rotation, especially at different plasma beta levels.
Contribution
It demonstrates the impact of electromagnetic turbulence on magnetic island evolution, including seeding, growth rates, and rotation, using self-consistent gyrokinetic simulations.
Findings
Turbulence seeds magnetic islands and bypasses linear growth.
Island growth depends on plasma beta and pressure gradients.
Turbulence alters island rotation direction and speed.
Abstract
The non-linear evolution of a magnetic island is studied using the Vlasov gyro-kinetic code GKW. The interaction of electromagnetic turbulence with a self-consistently growing magnetic island, generated by a tearing unstable current profile, is considered. The turbulence is able to seed the magnetic island and bypass the linear growth phase by generating structures that are approximately an ion gyro-radius in width. The non-linear evolution of the island width and its rotation frequency, after this seeding phase, is found to be modified and is dependent on the value of the plasma beta and equilibrium pressure gradients. At low values of beta the island evolves largely independent of the turbulence, while at higher values the interaction has a dramatic effect on island growth, causing the island to grow exponentially at the growth rate of its linear phase, even though the…
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