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ID |
Date |
Author |
Subject |
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32
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Sat Jul 9 21:08:08 2016 |
J.L. Tain | Neutron moderator |
Drawings of the polyethylene neutron moderator and table assembly |
| Attachment 1: Moderator-Table.pdf
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| Attachment 2: Table.pdf
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| Attachment 3: Moderator-Shielding.pdf
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31
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Sat Jul 9 21:00:54 2016 |
J.L. Tain | Hardware |
A list of the available hardware |
| Attachment 1: Hardware.xlsx
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| Attachment 2: Hardware.pdf
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30
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Sat Jul 9 20:44:31 2016 |
J.L. Tain | BRIKEN neutron detector |
START
Assembly and commissioning of BRIKEN neutron detector
The hybrid configuration of the BRIKEN neutron detector will be assembled at BF2 for the first time with 140 3He
tubes and 2 CLOVER detectors, connected to the Gasific digital data acquisition system and tested with 252Cf
sources. |
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29
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Mon May 11 09:14:54 2015 |
G. Kiss | 252Cf_data_sheet |
The activity of the 252Cf source, used for the calibration was 3.7 MBq at 15.05.2006. Unfortunately, uncertainty is missing from the data sheet :-( |
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28
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Fri May 8 03:20:48 2015 |
J.Agramunt J.L.Tain K.Gabor | BnCorrelation |
We run all the night until the end of beam time, and the Bn correlations are more clear now. |
| Attachment 1: BnCorr.pdf
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27
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Thu May 7 08:36:56 2015 |
J.L. Tain, J. Agramunt, A. Estrade, G.Kiss, T. Davinson, C.Griffin | First BRIKEN_v.0 beta-delayed neutron correlations? |
During the 98,100Kr setting run we observe
in the time correlation plot (middle right panel)
of beta signals (marked by AIDA, with amplitude larger than ch=600)
with Riken 3He tube signals (noise and pulser cleaned)
a small peak around t=0 which might be indication
of beta-delayed neutrons.
The spectrum was measured for about 2h. |
| Attachment 1: Screenshot_from_2015-05-07_16_01_27.png
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26
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Wed May 6 11:41:24 2015 |
J. Agramunt, A. Estrade | First online combined analysis |
Screen shot of the rudimentary on-line
analysis of the combined data:
BRIKEN-AIDA-BigRIPS
Top Left: dE (from MUSIC) vs. ToF (F11-F7)
Top Right: X-position (at F9) vs ToF
Middle Left: Amplitude spectrum of RIKEN tubes
Bottom Left: Energy spectrum from AIDA marked as beta-decays
Middle Right: Time correlations between betas (AIDA) and neutrons (BRIKEN)
Bottom Right: Time correlations between implants (AIDA) and neutrons (BRIKEN)
(the range of time correlated data [-1ms,+1ms]) |
| Attachment 1: Screenshot_from_2015-05-06_19_12_29.png
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25
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Wed May 6 05:10:14 2015 |
J.L. Tain, J. Agramunt, G. Kiss | 94Se setting measurement |
After the long shutdown the beam is back at 00:30 (06/05)
Intensity is slightly lower 26pnA and somewhat unstable (short time)
Measurement in the morning:
File: 150506_0846_0915_94Se.root
Average rate per tube (n/s): U=3.39 D=0.93B=0.40
Notes:
-The rate has increased by 3.5 in the detectors close to EURICA (!?)
-The rate at the detector below the MUSIC is substantial.
From the different magnitudes it is clear that neutrons are originated
both outside and inside EURICA. |
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24
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Wed May 6 04:57:24 2015 |
J.L. Tain, J. Agramunt, G. Kiss | New degrader thickness |
The Al degrader thickness was reduced to 4.8mm |
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23
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Tue May 5 05:29:26 2015 |
J.L. Tain, J. Agramunt, G. Kiss | Ambient background measurement |
Beam still down. New background measurement
with new RIKEN tube below the MUSIC chamber
(call it B)
File: 150505_0040_1130_aprox_bckg.root
Average rate per tube (n/s): U=0.0073, D=0.0065, B=0.0070 |
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22
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Tue May 5 05:17:36 2015 |
J.L. Tain, J. Agramunt, G. Kiss | Ambient background measurement |
Failure of a quadrupole triplet at BigRIPS (some time after earthquake)
We take the chance of measuring background:
File: 150504_1500_2047_bckg.root
Rate per tube (n/s): U=0.098, D=0.0062, US=0.0200
Ratio to 1st 110Zr: U=1.38, D=1.99, US=0.90
Notes:
-Compared to the 1st background measurement there are changes
larger than expected statistical fluctuations:
perhaps due to slight changes in noise
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21
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Tue May 5 05:04:00 2015 |
J.L. Tain, J. Agramunt, G. Kiss | Change of degrader thickness |
For EURICA measurements degrader thickness were increased
trying to decrease MACI and AIDA trigger rate
Before we had 5.7 mm of Al
Now we have:
Degrader: 4.0 + 1.0 + 0.6 + 0.4 +0.3 = 6.3 mm of Al
also 2x 0.8mm Al plates were added before
the MACI start detector (thus covering partially AIDA)
Trigger from AIDA will be taken from 3rd DSSSD |
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20
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Tue May 5 02:19:58 2015 |
j.Agramunt J.L.Tain K.Gabor | The Lower polyethylene pieces was swamped |
The Lower polyethylene pieces was swamped.
In the photo beam comes from the left.
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| Attachment 1: photo-4.JPG
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19
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Mon May 4 15:03:47 2015 |
J.Agramunt J.L.Tain K.Gabor | New detector placed under the beam line |
New detector placed under the beam line, below MUSIC chamber
This detector replace the USA tubes in the DACQ because we need the preamp to plug it.
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| Attachment 1: photo_2-2.JPG
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| Attachment 2: photo_1-2.JPG
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| Attachment 3: photo_3-2.JPG
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18
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Mon May 4 04:14:18 2015 |
J.Agramunt J.L.Tain K.Gabor | AIDA trigger plugged in Mod2 Ch12 |
AIDA trigger plugged in Mod2 Ch12 |
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17
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Mon May 4 03:20:00 2015 |
Shunji Nishimura | RNC New Rule |
We have some new rule about the data taken at RNC from this year.
Shunji
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| Attachment 1: kanri_e.pdf
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16
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Mon May 4 02:36:16 2015 |
J.Agramunt J.L.Tain K.Gabor | Maki trigger plugged in Mod2 Ch9 |
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15
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Mon May 4 02:26:14 2015 |
J.Agramunt J.L.Tain K.Gabor | F11 trigger plugged in Mod2 Ch16 of Briken daq |
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14
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Sun May 3 10:10:13 2015 |
J.L. Tain, J. Agramunt, G. Kiss | 94Se setting measurement |
94Se setting:
File: 150503_1500_1554_94Se.root
Rate per tube (n/s): U=0.966, D=0.263, US=0.538
Ratio to 1st 110Zr: U=2.00, D=1.89, US=1.84
Notes:
-Compared to the 1st 94Se setting measurement (12:19-13:19)
there is a drop of 25% in the rate without apparent reason |
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13
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Sun May 3 10:07:25 2015 |
J.L. Tain, J. Agramunt, G. Kiss | Photos of new PE shielding |
Photos of the general arrangement and details of the new PE blocks |
| Attachment 1: 20150502_195020.jpg
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| Attachment 2: 20150502_194340.jpg
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| Attachment 3: 20150502_192253.jpg
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