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
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miscellaneous (cont’d.)<br />
progress report<br />
2010<br />
119<br />
been proposed. The Pd–Ag composite membranes have<br />
been produced in form of thin sheets supported over<br />
stainless steel grids and welded to stainless steel frames. The<br />
<strong>di</strong>ffusion wel<strong>di</strong>ng procedure has further been operated in<br />
order to tightly join the Pd–Ag membranes to the stainless<br />
steel frames. The resulting membrane module is very<br />
compact: as an example, a permeator of surface area of<br />
10 m 2 could be about 1000 × 120 × 180 mm in size.<br />
Modelling and testing of membrane reactors using Pd–Ag<br />
thin wall tubes have concerned the investigation of ethanol<br />
steam and oxidative reforming [9.3–9.7] and water gas shift<br />
reaction [9.8]. The tests have highlighted the complete<br />
hydrogen selectivity of the thin wall membranes and their<br />
capability of promoting the reaction conversion beyond the<br />
thermodynamic equilibrium (shift effect of the<br />
membrane) [9.9].<br />
Figure 9.3 – Hydrogen production from ethanol<br />
reforming: experimental apparatus<br />
9.3 AGILE and LOFT<br />
In 2010 the Astrorivelatore Gamma ad Immagini LEggero<br />
(AGILE), the satellite for gamma and x–ray astronomy built<br />
with the contribute of <strong>ENEA</strong>, made two interesting fin<strong>di</strong>ngs<br />
(among other results): it <strong>di</strong>scovered a possible new class of<br />
celestial gamma-ray sources [9.10], and shed new light on the<br />
nature of the terrestrial gamma ray flashes, an intriguing<br />
phenomenon which might have consequences on the safety of<br />
civil aviation [9.11].<br />
The promising performances of a new x–ray detector, designed<br />
in collaboration with <strong>ENEA</strong> Fusion Technology Unit [9.12],<br />
based on silicon drift detectors, have led to the proposal to<br />
“ESA call for a me<strong>di</strong>um–size mission opportunity for a launch<br />
in 2022” of a new satellite, called Large Observatory For x–ray<br />
Timing (LOFT) [9.13], backed by 130 scientists from 16<br />
countries. Thanks to an innovative design and the development<br />
Figure 9.4 – Pictorial view of LOFT, with the six<br />
petals of LAD deployed<br />
of large monolithic silicon drift detectors, the large area detector (LAD) on board of LOFT would achieve an<br />
effective area of ∼12 m 2 (more than one order of magnitude larger than the current spaceborne x–ray