Concept: Magnetic field
GVEC provides flexible 3D MHD equilibrium solutions
New solver extends plasma state exploration for fusion devices

Shock precursor type changes ion and electron acceleration
How magnetic field strength controls particle acceleration in cosmic shock waves

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

Q–Monopole–Ball soliton with unit magnetic charge exists
A new solution binding monopoles through topological and non-topological charges

Cold ions enable ion-acoustic waves in asymmetric reconnection
Electrostatic waves accelerate ions and transfer energy during magnetic reconnection in plasma








