COLLISIONAL-RADIATIVE MODELS FOR HYDROGEN-LIKE AND HELIUM-LIKE CARBONAND OXYGEN IONS AND APPLICATIONS TO EXPERIMENTAL-DATA FROM THE TS TOKAMAK AND THE REVERSED-FIELD PINCH RFX
L. Carraro et al., COLLISIONAL-RADIATIVE MODELS FOR HYDROGEN-LIKE AND HELIUM-LIKE CARBONAND OXYGEN IONS AND APPLICATIONS TO EXPERIMENTAL-DATA FROM THE TS TOKAMAK AND THE REVERSED-FIELD PINCH RFX, Physica scripta. T, 55(5), 1997, pp. 565-578
Collisional radiative models (CRM) are needed to simulate experimental
line brightnesses and emissivities from fusion devices. CRM are built
for H-like and He-like carbon and oxygen ions, following a detailed r
eview of the published literature on the required atomic data (includi
ng both collision rate coefficients and atomic transition probabilitie
s). The impurity ion radial distribution is obtained using a transport
code with two radius dependent transport parameters: a diffusion coef
ficient D and an inward convection velocity V. Reliable atomic data ar
e a prerequisite to these simulations, since they are supposed to be w
ell known; adjustement of the simulations to the experimental line and
/or continuum brightnesses and emissivities is done by varying only D
and V. Examples are given of the quantitative interpretation of experi
mental spectroscopic data from two fusion devices: the Tore Supra Toka
mak and the Reversed Field Pinch RFX. As a consequence of the order of
magnitude difference in the central electron temperatures in the two
devices, the sensitivity of the H-like and He-like ion emissions to th
e transport parameters is different. These differences are highlighted
in the examples given.