TY - JOUR
T1 - Development of the gas-puff imaging diagnostic in the TEXTOR tokamak
AU - Shesterikov, I.
AU - Xu, Y.
AU - Berte, M.
AU - Dumortier, P.
AU - Van Schoor, M.
AU - Vergote, M.
AU - Schweer, B.
AU - Van Oost, G.
PY - 2013/5
Y1 - 2013/5
N2 - Gas puff imaging (GPI) [S. J. Zweben, D. P. Stotler, Phys. Plasmas 9, 1981 (2002)10.1063/1.1445179; R. J. Maqueda, G. A. Wurden, Rev. Sci. Instrum. 74, 2020 (2003)10.1063/1.1535249] is a powerful diagnostic that permits a two-dimensional measurement of turbulence in the edge region of a fusion plasma and is based on the observation of the local emission of a neutral gas, actively puffed into the periphery of the plasma. The developed in-vessel GPI telescope observes the emission from the puffed gas along local (at the puff) magnetic field lines. The GPI telescope is specially designed to operate in severe TEXTOR conditions and can be treated as a prototype for the GPI systems on next generation machines. Also, the gas puff nozzle is designed to have a lower divergence of the gas flow than previous GPI diagnostics. The resulting images show poloidally and radially propagating structures, which are associated with plasma blobs. We demonstrate that the local gas puff does not disturb plasma properties. Our results indicate also that the neutral gas emission intensity is more sensitive to the electron density than the electron temperature. Here, we present implementation details of the GPI system on TEXTOR and discuss some design and diagnostic issues related to the development of GPI systems in general.
AB - Gas puff imaging (GPI) [S. J. Zweben, D. P. Stotler, Phys. Plasmas 9, 1981 (2002)10.1063/1.1445179; R. J. Maqueda, G. A. Wurden, Rev. Sci. Instrum. 74, 2020 (2003)10.1063/1.1535249] is a powerful diagnostic that permits a two-dimensional measurement of turbulence in the edge region of a fusion plasma and is based on the observation of the local emission of a neutral gas, actively puffed into the periphery of the plasma. The developed in-vessel GPI telescope observes the emission from the puffed gas along local (at the puff) magnetic field lines. The GPI telescope is specially designed to operate in severe TEXTOR conditions and can be treated as a prototype for the GPI systems on next generation machines. Also, the gas puff nozzle is designed to have a lower divergence of the gas flow than previous GPI diagnostics. The resulting images show poloidally and radially propagating structures, which are associated with plasma blobs. We demonstrate that the local gas puff does not disturb plasma properties. Our results indicate also that the neutral gas emission intensity is more sensitive to the electron density than the electron temperature. Here, we present implementation details of the GPI system on TEXTOR and discuss some design and diagnostic issues related to the development of GPI systems in general.
UR - http://www.scopus.com/inward/record.url?scp=84878922067&partnerID=8YFLogxK
U2 - 10.1063/1.4803934
DO - 10.1063/1.4803934
M3 - Article
AN - SCOPUS:84878922067
SN - 0034-6748
VL - 84
JO - Review of Scientific Instruments
JF - Review of Scientific Instruments
IS - 5
M1 - 053501
ER -