Plasma Physics & Fusion
Simulating the stars: Achieving stable plasma confinement through Magnetohydrodynamics (MHD).
Mastering 150 Million Degrees Celsius
Nuclear fusion is the ultimate challenge in fluid dynamics and electromagnetism. To realize the promise of clean, limitless energy, we provide the computational backbone for ITER and other tokamak/stellarator projects, resolving the non-linear instabilities of plasma in real-time.
ITER Fusion States
Modeling the core and edge plasma behavior in the International Thermonuclear Experimental Reactor. Resolving turbulence and heat transport across magnetic field lines.
- Gyrokinetic simulation (GKW)
- Edge Localized Mode (ELM) control modeling
Magnetohydrodynamics (MHD)
Achieving stable plasma confinement by solving the macroscopic equations of electrically conducting fluids. Critical for predicting and preventing sudden disruptions.
- Non-linear 3D MHD solvers
- Equilibrium and stability analysis
Fusion Logic: Parameter -> Computation -> Stable Burn
| Simulation Goal | Computational Action | Engineering ROI |
|---|---|---|
| Magnetic Confinement | Solving the Grad-Shafranov equation for field equilibrium. | Optimal Stellarator Geometry |
| Disruption Prediction | Real-time AI surrogates trained on multi-petabyte JET data. | Safe Reactor Shutdown Protocols |
| Wall Interactions | Kinetic modeling of neutral particle recycling at the divertor. | Extended Component Lifetime |
Institutes Defining the Fusion Future
Malgukke solutions are architected to meet the data throughput needs of the world's leading fusion centers: