Magnetic helicity dynamics in compressible isothermal MHD turbulence
- 1Zentrum für Astronomie und Astrophysik, TU Berlin, Germany
- 2Max-Planck/Princeton Center for Plasma Physics
Magnetic helicity dynamics are important in the context of the generation of large scale magnetic structures from small scale fluctuations. Up to the present day, these dynamics have remained largely unexplored in compressible plasmas. We present new results from direct numerical simulations of isothermal magnetohydrodynamic turbulence, with Mach numbers ranging from 0.1 to 10 by employing higher-order numerics. A mechanical driving injects kinetic energy at the largest scales, while a small scale electromotive driving injects helical magnetic fluctuations. A large-scale sink of magnetic energy leads to the formation of a turbulent statistically stationary state, which is analyzed, extending the results on nonlinear cross-scale transfer presented in doi:10.1017/jfm.2021.32 and doi:10.1017/jfm.2021.496.
How to cite: Teissier, J.-M. and Müller, W.-C.: Magnetic helicity dynamics in compressible isothermal MHD turbulence, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-15770, https://doi.org/10.5194/egusphere-egu23-15770, 2023.