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  • Operational domain for the ...
    Fonghetti, T.; Dumont, R.; Giruzzi, G.; Artaud, J.-F.; Bernard, J.-M.; Bouquey, F.; Bourdelle, C.; Delpech, L.; Hillairet, J.; Maget, P.; Manas, P.; Mollard, P.; Morales, J.; Ostuni, V.; Robinet, B.

    EPJ Web of conferences, 2023, Letnik: 277
    Journal Article

    The ECRH system formerly used in Tore Supra is being upgraded to start on WEST in 2023, at a power level of 1MW and frequency of 105 GHz. Its ultimate 3MW/1000s capability is expected to enlarge the WEST operational domain by increasing margins with respect to H-mode access, and by providing additional flexibility in terms of achievable scenarios using impurity and/or MHD control. This flexibility is made possible using an antenna based on three steerable mirrors for controlled power injection. In order to determine an appropriate range of EC wave injection angles for WEST scenarios, the fast and reliable ray-tracing code REMA has been interfaced with the WEST IMAS database. This allows the EC power damping rate to be quickly assessed, as well as deposition profiles to be predicted in realistic plasma conditions. Based on a typical WEST discharge at central magnetic field B 0 ~3.6 T, central line-averaged electron density n l ~4 × 10 19 m −3 and central electron temperature T e0 ~3keV, ray-tracing calculations have been performed. Comprehensive poloidal and toroidal angle scans, as well as variations of B t , nl and T e0 with respect to the reference parameters have allowed an adequate range of injection angles to be determined for efficient use of ECRH and/or ECCD in typical WEST scenarios, and compared with the mechanical limits set by the antenna mechanical characteristics. In order to further characterize the effect of this new power source in WEST scenarios, EC wave deposition and current profiles from ray-tracing calculations have been included in integrated simulation codes. It has been shown that this additional power source could allow central electron heating to be achieved, potentially alleviating the issue of radiative collapse caused by impurities observed in some situations.