AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
BRIKEN
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<p> <table width="98%" align="center" cellspacing="1" style="border:1px solid #486090;"> <tbody> <tr> <td cellpadding="3px" style="background-color:#486090; font-weidht:bold; color:white;">Quote:</td></tr> <tr> <td cellpadding="10px" style="background-color:#FFFFB0;"><p>Altogether 16 tubes are mounted for the parasitic detector test (see the attached photos):</p> <p>- two tubes (belonging to RIKEN) are in a 10 cm x 10 cm x 30 cm polyethylene matrix inside Eurica, the distance from AIDA is about 30 cm</p> <p>- 12 tubes (belonging to RIKEN) are in a 20 xm x 30 xm x 30 cm matrix, outside (below) Eurica, at the closest possible place to AIDA, the distance is about 60 cm</p> <p>- further two tubes (ORNL) are at the bottom of the Eurica support, about 1.2 m from the AIDA Silicon.</p> <p>Furthermore, spectra measured using a 252Cf source is attached to this report, too (Jap1Cf-RIKEN tube, Us1Cf-ORNL tube). At the moment a background measurement is running.<a href="150425_082251/P1120020.JPG?lb=BRIKEN"><img border="0" alt="P1120020.JPG" src="150425_082251/P1120020.JPG?lb=BRIKEN&thumb=1" name="att0" id="att0" /></a></p></td> </tr> </tbody> </table> </p><p> </p>
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