Concept: Turbulence
Turbulent black hole coronae can produce observed X-ray spectra
How turbulent coronae around black holes accelerate particles and emit X-rays

DM Tau disk shows non-thermal line broadening
Turbulent motion detected in a young star's planet-forming disk

Structure-preserving simulations show differing turbulence behavior
Long-time behavior of magnetized fluid turbulence preserved through geometric simulation methods

Predictive gyrokinetic simulations matched TCV edge-plasma data
Simulating tokamak edge turbulence from physics alone, without fitting to experiments









