Speaker
Dr
Alessandro Bruschi
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Description
The Collective Thomson Scattering (CTS) diagnostic on FTU tokamak was renewed [1] for investigations on the excitation of Parametric Decay Instabilities (PDI) by Electron Cyclotron (EC) beams in presence of magnetic islands and their effects on the EC absorption.
Experiments were performed with a gyrotron probe (140 GHz, 400 kW) launched in symmetric and asymmetric configurations with respect to the equatorial plane, in different conditions of plasma density and magnetic field (with or without the EC resonance in the plasma), and with magnetic islands generated by Neon injection. The acquisition with a fast digitizer allowed observing spectral features with very high time and frequency resolution [2]. In the shots performed at 7.2 T, with the fundamental EC resonance out of the plasma region, a sequence of faint lines emitted with a fast temporal evolution have been observed in a range 0.5-1.1 GHz from the gyrotron frequency (Fig.1) while at 4.7 T, with the resonance on the high field side of the plasma column, asynchronous "bursts" of continuous emissions were observed at a microsecond time scale.
In 2015 experiments were performed at 4.7 and 3.6 T, in this last case with the plasma between the first and the second EC harmonics. Different types of spectral features with a fast evolution were observed. Their correlation with magnetic probes and fast signals from the plasma has been investigated, to characterize the observations and exclude parasitic effects, as well as breakdown phenomena in front of the antennas. The variation in the stray radiation distribution in the vessel has been studied with the aid of a diffusive model, to characterize variations on the probe beam absorption associated to the observed phenomena. Further improvements of the diagnostic both in frequency band (up to ±4.2 GHz from the probe) and with the addition of a second radiometer, will allow a clearer interpretation of the emissions.
Acknowledgement: This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 under grant agreement No 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission.
[1] W. Bin et al., Fusion Eng. Des. 96-97 (2015) 733-737
[2] A. Bruschi et al., Proc. 42nd EPS Conference on Plasma Physics (2015)
Country or International Organization | Italy |
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Paper Number | EX/P8-23 |
Primary author
Dr
Alessandro Bruschi
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Co-authors
Dr
Alessandro Moro
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
Cristian Galperti
(Swiss Plasma Center, EPFL, Lausanne, Switzerland)
Dr
Daria Ricci
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
Edoardo Alessi
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
Francesco Belli
(ENEA C.R. Frascati, Roma, Italy)
Dr
Francesco Paolo Orsitto
(CREATE, Università degli Studi, Napoli, Italy)
Dr
GUSTAVO GRANUCCI
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
Giovanni Grosso
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
Giuseppe Calabro
(ENEA C.R. Frascati, Roma, Italy)
Dr
Giuseppe Ramogida
(ENEA C.R. Frascati, Roma, Italy)
Irene Casiraghi
(Università degli Studi di Milano Bicocca, Milano, Italy)
Dr
Jesper Rasmussen
(Department of Physics, DTU, Lyngby, Denmark)
Dr
Lorenzo Figini
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
Maurizio Lontano
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
Morten Stejner Pedersen
(Department of Physics, DTU, Lyngby, Denmark)
Dr
Ocleto D'Arcangelo
(ENEA C.R. Frascati, Roma, Italy)
Dr
Saul Garavaglia
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
Stefan Kragh Nielsen
(Department of Physics, DTU, Lyngby, Denmark)
Dr
Søren Bang Korsholm
(Department of Physics, DTU, Lyngby, Denmark)
Dr
Umberto Tartari
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
Valter Cocilovo
(ENEA C.R. Frascati, Roma, Italy)
Vittoria Mellera
(Istituto di Fisica del Plasma, CNR, Milano, Italy)
Dr
William Bin
(Istituto di Fisica del Plasma, CNR, Milano, Italy)