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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

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