“…Hence there is a need for databases of tabulated spectral emission lines that have been clearly identified in magnetically confined plasmas. At present, there exists in the literature a limited number of spectral line surveys covering different wavelength ranges [4,[9][10][11]. In most cases such data tabulate intrinsic, vacuum wall deposited elements, and/or commonly injected elements, e.g., helium, lithium, boron, carbon, nitrogen, oxygen, neon, aluminium, iron or chromium.…”