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Electron-Cyclotron Heating and Current Drive

ECRH modeling combines ray-tracing and Fokker-Planck physics to predict the highly localized heating and current drive from electron-cyclotron waves.

Resonant electron heating

Electron-cyclotron waves are launched at the frequency where electrons gyrate, or a harmonic of it. Where that resonance occurs in the plasma, the wave transfers energy directly to electrons. Because the resonance is a narrow layer set by the magnetic field, deposition is exceptionally localized and steerable.

The modeling chain

Kronos motion — fusion

A ray-tracing code follows the launched beam to the resonance layer and computes absorption; a Fokker-Planck solver then determines how the absorbed power reshapes the electron distribution and how much current results. The combination predicts both the heating profile and the current-drive efficiency as functions of launch angle.

Why localization matters

Steering and control

Because the deposition location depends on the launch geometry and the local field, movable mirrors can steer the beam in real time. Modeling predicts the accessible deposition range and the aiming accuracy required, informing both antenna design and the control algorithms that use ECRH for stabilization.

Design integration

ECRH is valued for its flexibility: the same system can heat, drive current, and stabilize instabilities depending on where it is aimed. Modeling quantifies these trade-offs so a design carries enough power and steering to meet its stability and scenario needs.

For the Hyperion breeder, localized electron-cyclotron current drive is a candidate tool for neoclassical-tearing-mode suppression, and its modeling ties directly to the island-stabilization analysis.