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Prime pagine RA2010FUS:Copia di Layout 1 - ENEA - Fusione

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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

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