Prime pagine RA2010FUS:Copia di Layout 1 - ENEA - Fusione
Prime pagine RA2010FUS:Copia di Layout 1 - ENEA - Fusione
Prime pagine RA2010FUS:Copia di Layout 1 - ENEA - Fusione
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
024<br />
progress report<br />
2010<br />
New <strong>di</strong>agnostics for soft x–ray imaging and tomography. Magnetic fusion plasmas (MFP) are extended sources<br />
of x–rays and these emissions could reveal a lot of information about the processes occurring inside the<br />
plasmas.<br />
The aim of this project is the development of a 2–D detector with independent energy <strong>di</strong>scrimination<br />
capability for each pixel. Plasma <strong>di</strong>agnostics based on soft x–ray (SXR) tomography and/or imaging for<br />
magnetic confinement fusion plasmas could be greatly enhanced if <strong>di</strong>fferent energy bands (which are<br />
representative of <strong>di</strong>fferent plasma zones and their impurity content) could be selected dynamically. A gas<br />
detector with 2–D pixel read–out is being proposed for such a <strong>di</strong>agnostics.<br />
Moreover, the constraints posed by toroidal devices (highly ra<strong>di</strong>ative background, extremely high<br />
ra<strong>di</strong>ofrequency powers, high magnetic fields, optical limitations and so on) are very severe and strongly limit<br />
the possibility to install x–ray detectors <strong>di</strong>rectly into, or close to the machine. Therefore, it becomes mandatory,<br />
in particular for future burning plasma experiments, to study the possibility of transporting the SXR ra<strong>di</strong>ation<br />
far from the machine. Polycapillary lenses appear promising for these purposes and suitable to be used for<br />
x–ray imaging and tomography in MFP. All these activities have been carried out in collaboration with the<br />
National Institute of Nuclear Physics (INFN) – Frascati National Laboratory (LNF) and CEA laboratory of<br />
Cadarache, under the auspices of EFDA (Work Program 2010 (WP2010)).<br />
1) Realization and characterization of a triple GEM gas detector. A triple gas electron multiplier (GEM) detector<br />
has been designed and built by the LNF–INFN laboratory of Frascati and subsequently installed in the SXR<br />
laboratory of CEA for this preliminary characterization [1.13]. It is based on a gas detector with triple GEM<br />
as amplifying structure and with a two–<strong>di</strong>mensional read–out, coupled to the integrated front–end electronics.<br />
The energy <strong>di</strong>scrimination in bands, at the level of in<strong>di</strong>vidual pixel, has been stu<strong>di</strong>ed. The front-end<br />
electronics of the GEM detector, working in photon counting mode with a selectable threshold for pulse<br />
<strong>di</strong>scrimination, is optimized for high rates.<br />
The energy resolution of the detector has been accurately stu<strong>di</strong>ed in laboratory with continuous SXR spectra<br />
produced by an electronic tube (continuous spectra with a Moxtek 40 kV Bullet) and line emissions produced<br />
by fluorescence (K, Fe, Mo), in the range 3–17 keV (fig. 1.28). For the measurements presented, the detector<br />
has been filled with a gas mixture at atmospheric pressure with<br />
10 2 counts/s<br />
6<br />
4<br />
2<br />
K<br />
Fe<br />
Mo<br />
0<br />
0 10 20<br />
Energy (keV)<br />
Figure 1.28 – SXR fluorescence of K, Fe and Mo<br />
samples measured with the Si–PIN detector<br />
Counts (Arb. units)<br />
0.6<br />
0.4<br />
K<br />
3.3 keV<br />
6.39 keV<br />
0<br />
0 100 200 300 400<br />
Energy (mV)<br />
Figure 1.29 – Reconstructed spectra for<br />
samples of K and Fe sources<br />
Fe<br />
Ar (70%) and CO 2<br />
(30%). In order to assess the intrinsic<br />
energy resolution of the detector, the <strong>di</strong>stribution of the pulse<br />
amplitude of the signals collected on a single pixel has been<br />
in<strong>di</strong>rectly derived, for <strong>di</strong>fferent K α<br />
line ra<strong>di</strong>ations (K, Fe, Mo).<br />
The integral of all the counts whose amplitude is greater than<br />
the threshold has been measured instead of the effective<br />
<strong>di</strong>stribution of the counts as function of the peak amplitude.<br />
The <strong>di</strong>stribution of the pulse amplitude has been in<strong>di</strong>rectly<br />
derived by means of scans of the threshold and by fitting it<br />
with a guess function with three free parameters: position of<br />
maximum and half width at half maximum of the Gaussian<br />
peak and decay length of the tail (fig. 1.29). The <strong>di</strong>stribution of<br />
the pulse amplitude, in the range 3–17 keV, was found nearby<br />
a Gaussian. The best agreement is found for a total detector<br />
gain of 500 and an energy resolution of about 30% and a tail<br />
at higher energy. The pulse broadening is entirely due to the<br />
poor energy resolution of the detector. Scans in detector gain<br />
have been also performed to assess the capability of selecting<br />
<strong>di</strong>fferent energy ranges. Combining together two samples, Fe<br />
and Mo, fluorescence spectra with two lines have been<br />
generated, to investigate the sensitivity of the threshold scan to<br />
a more complex spectrum.<br />
The reconstruction, by means of a threshold scan, of the<br />
incident spectrum has been demonstrated in case of simple<br />
spectra, single or double line emissions or bell shaped features.<br />
In case of more complex spectra, with <strong>di</strong>fferent features, the<br />
only scan in threshold might be not sufficient. In this case a