Realization of a Gas-Puff Imaging diagnostic on W7-X
POSTER
Abstract
A Gas-Puff Imaging system designed to provide 2-d imaging of fluctuations on turbulence time-scales at the outboard edge of W7-X has been installed and is being commissioned for operation at the start of the next run campaign. The system will be used to study turbulence and filament dynamics in the SOL and in the magnetic islands, present as features of the island divertor configuration. Imaging of a ~78 x 38 mm region with 16 x 8 pixel resolution at ~1MHz framerates provides the capability to measure features with kperp in the range from ~0.04 to ~5 cm-1., with kperp ρs ~0.1.The system features high-throughput light collection by re-entrant optics imaging directly onto the camera, and a pop-up turning mirror that provides sight lines to the gas-puff region that are within ~10o of the local field lines. The novel gas-puffer features 2 vertically-stacked nozzles with “converging-diverging” cross-sections to provide improved collimation of the puffed gas. Because better collimation improves the spatial resolution and increases the chord brightnesses, careful measurements of the gas-puff cloud were made. An overview of the system, its expected capabilities, and the gas cloud measurements will be presented.
*Support for MIT participation was provided by the US Department of Energy, Fusion Energy Sciences, Award DE-SC0014251. This work has been carried out within the framework of the EUROfusion Consortium, funded by the European Union via the Euratom Research and Training Programme (Grant Agreement No 101052200 — EUROfusion). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Commission. Neither the European Union nor the European Commission can be held responsible for them.
Presenters
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James L Terry
- MIT PSFC
- Massachusetts Institute of Technology MI
- MIT-PSFC
- MIT Plasma Science Fusion Center
- Massachusetts Institute of Technology MIT