DEMO


DEMO stands for Demonstration Tokamak fusion reactor — the next-step plant, built to demonstrate actual net fusion energy production. This work is part of a EUROfusion project (Work Package Auxiliary systems, WPAUX) assigned to us; within it we develop the architecture, system design and integration of the Electron Cyclotron Emission (ECE) diagnostics for mode detection and electron-temperature measurements.
Where ECE fits in: far-infrared / submillimetre-wave plasma diagnostics for nucl
Where ECE fits in: far-infrared / submillimetre-wave plasma diagnostics for nuclear fusion.

What ECE measures

Plasma electrons radiate at harmonics of the cyclotron frequency. Where the plasma is optically thick, the emission gives a local measurement of the electron temperature along the radius, and the time/spectral analysis of the signal also lets us detect MHD modes — both essential for controlling the plasma. Turning this into a working diagnostic on DEMO is mostly a matter of architecture, waveguides and integration.

Conceptual layout of one ECE line of sight, from the front-end antennas inside t
Conceptual layout of one ECE line of sight, from the front-end antennas inside the vessel, through oversized waveguides and confinement barriers, to the back-end spectrometers in the diagnostics building.

Why DEMO is hard

Unlike present machines, DEMO combines an intense neutron/gamma environment with tight integration constraints: limited access ports, qualified materials, mirror durability, and lines shared with ECRH and reflectometry. The design answers with robust waveguides, careful front-end choices and a redundant line-of-sight layout.

The extreme conditions of DEMO: mirror durability under strong neutron/heat flux
The extreme conditions of DEMO: mirror durability under strong neutron/heat flux, and a 100% redundancy design. Photo: antenna and mirror damage on FTU (Frascati) — a far milder machine than DEMO.
Simplified 3D view of the ex-vessel arrangement of one ECE line of sight: the ro
Simplified 3D view of the ex-vessel arrangement of one ECE line of sight: the rotatable mirror switches the spectrometer input between the plasma and the hot calibration source (HS).
Detail of the DSC–waveguide interface: steerable mirrors set the toroidal (20°)
Detail of the DSC–waveguide interface: steerable mirrors set the toroidal (20°) and poloidal (4°) launch angles and ease the waveguide routing along the oblique lines of sight.

Characterizing the antennas (microwave tests)

To pin down the front-end, we characterise candidate antennas on the bench with microwave techniques — work carried out here in the DEMO context. We measure the horn pattern from near- to far-field and check the behaviour of pseudo-CPC concentrators against a 140 GHz source.

Microwave test bench: the reflectometry horn antenna and a pseudo-CPC front-end,
Microwave test bench: the reflectometry horn antenna and a pseudo-CPC front-end, characterised against a 140 GHz source with a scanning pyro-detector.
Measured horn-antenna pattern at increasing distances: the transition from near-
Measured horn-antenna pattern at increasing distances: the transition from near-field to far-field (beyond ~50 cm) and the associated drop in peak power.

Where the work stands

The current effort revises the ECE Design Description Document (DDD) against the new DEMO baseline and reports the conceptual-design studies (deliverables D001 — revised DDD, and D002 — final report). A companion, exploratory line — a multifunctional THz-TDS diagnostic tested on the WEST tokamak — feeds the same competences (see the THz and Reflectometry pages).

Key publications