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physics.plasm-ph2026
Numerical simulations of shock-driven, supersonic interstellar turbulence in colliding three-temperature laboratory plasmas
Stefano Merlini, James R. Beattie, Vicente Valenzuela-Villaseca
Shock-driven turbulence is central to astrophysical plasmas in which explosions and compressive driving inject energy through shocks rather than steady stirring. We present three-d…
physics.plasm-ph2025
The universal growth of magnetic energy during the nonlinear phase of subsonic and supersonic small-scale dynamos
Neco Kriel, James R. Beattie, Mark R. Krumholz +2
Small-scale dynamos (SSDs) amplify magnetic fields in turbulent plasmas. Theory predicts nonlinear magnetic energy growth , but this scali…