Structure of pellet cloud emission and relation with the local ablation rate

Abstract

The experimental reproduction of the conditions of pellet injection expected in future large devices being not possible in present day machines, it is mandatory to validate as thoroughly as possible the available ablation models. Among the different points still under discussion, there is the relation between the spectroscopic measurement of the ablation clouds and the local ablation rate. This relation is investigated by coupling an emission model to the time-dependent simulation of ablation clouds with the HPI2 pellet ablation/deposition code. The simulated quantities are the time-evolution of the cloud visible spectrum ( λ = 400–700 nm) and images in different wavelength domains (e.g. $H_{\alpha}, H_{\beta}$ or the continuum centered at $\lambda = 576\,\mathrm{nm}$ ). It is found that the cloud emission is anisotropic, this is particularly the case for H _α and H _β lines, and that the relation between the cloud emission and the ablation rate depends not only on the conditions of pellet injection, but also on the direction of observation. It follows that, in general, it is not possible to estimate the ablation profile from that of an emission line $\left(H_{\alpha}\right.$ or $\left.H_{\beta}\right)$ . The code predictions are compared with corresponding measurements for a welldocumented pellet injected in LHD, showing a good agreement for global values and main trends. The reasons for observed discrepancies are discussed.

Keywords

• pellet physics
• emission spectrum
• ablation rate
• LHD