Revision 04302c40ef57ee57b018f37493dcd13eebe26926 (click the page title to view the current version)
Changes from 04302c40ef57ee57b018f37493dcd13eebe26926 to 5e6f4a5c038e0a59d73e8aa38f9ac090803c2b20
%info@http:://golem.fjfi.cvut.cz/wiki/root/GW4reports
\def\GWslide{\slide{Optical spectroscopy}{
\GWif{width=0.85\tw}{Diagnostics/Radiation/Minispectrometer/Slides/Naydenkova-2025-Calibration/Fig.png}{Calibration and Identified VIS lines in the tG discharge}
\begin{itemize}\footnotesize
\item Optical spectroscopy was used to study plasma composition during transport barrier formation.
\item Five compact spectrometers covered a wide spectral range from 250 to 1100\,nm.
\item Helium line emission decreases in time, while low-Z impurity lines increase.
\item Identified impurity lines indicate enhanced wall interaction and erosion of in-vessel components.
\item Spectroscopy provides indirect evidence of strong impurity influx during transport barrier phases.
\end{itemize}
}}