Study of radiation limits in fusion reactor scenarios

Radiative mantle scenarios of the ignited ITER FDR (Final Design Report) wi th argon and neon seeding are explored by self-consistent simulations with a special version of the 1.5-D BALDUR predictive transport code. The calcul ations apply empirical transport coefficients and are carried out both in t he bulk and in the SOL. Operation relevant upper limits to the radiative po wer losses from the main chamber, from closed flux surfaces and from the SO L are found. Both simulations and an analytic study of power balances show that these limits are set by the radiation profile and by the cross-field h eat conduction in the SOL. For given heating power, the conductive heat flu x across the separatrix and the energy flow to the divertor are also restri cted. With high edge density, the required thermal energy confinement times at the radiation limits are found to be 4.4 s in the argon and 4.0 s in th e neon scenario. The assumption of flat density profiles and no inward pinc h in the whole plasma is supported by simulations using a new scaling relat ion for the anomalous inward drift. The dependence of the radiation limits on the separatrix density is investigated. Formulas for relevant power limi ts are presented.