ID |
Date |
Author |
Subject |
30
|
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. |
2
|
Fri Oct 31 11:36:57 2014 |
Alfredo Estrade | BRIKEN elog: take 2 |
A elog for the setup of the BRIKEN detector is now operational at https://elog.ph.ed.ac.uk/BRIKEN/
We have setup a list of emails that will receive automatic updates for each new entry to the logbook: C. Domingo, G. Lorusso, T. Davinson, A. Estrade, K. Rykaczewski, J.L. Tain, C. Griffin, S. Nishimura, I. Dillman, F. Montes, J. Agramunt, G. Cortes, F. Calvino, M. Marta
Please let us know the contact info for any other person that would like to be included in this list, or if you would like your email to be removed from it (should the new entries be too frequent for your inbox traffic!). |
1
|
Fri Oct 31 09:47:59 2014 |
Alfredo Estrade | BRIKEN elog: Hello world! |
A elog for the setup of the BRIKEN detector is now operational at https://elog.ph.ed.ac.uk/BRIKEN/
We have setup a list of emails that will receive automatic updates for each new entry to the elog:
C. Domingo, G. Lorusso, T. Davinson, A. Estrade, K. Rykaczewski, J.L. Tain, C. Griffin, S. Nishimura, I. Dillman, F. Montes, J. Agramunt, G. Cortes, F. Calvino, M. Marta
Please let us know about any other person that would like to be included in this list, or if you would like your email to be removed from it (should the new entries be too frequent for your inbox traffic!).
|
79
|
Wed Oct 12 11:30:53 2016 |
Ariel Tarifeno, Alvaro Toloza, JL Tain, J. Agramunt, et al | BRIKEN Z scan |
Scanning of the BRIKEN detector with the 252Cf source
along the longitudinal axis (Z axis)
Measurements from Z: -42.5cm to 42.5cm with steps of 2.5cm. |
7
|
Sat Apr 25 08:25:42 2015 |
G. Kiss, J. Agramunt | BRIKEN Test setup |
Altogether 16 tubes are mounted for the parasitic detector test (see the attached photos):
- 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
- 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
- further two tubes (ORNL) are at the bottom of the Eurica support, about 1.2 m from the AIDA Silicon.
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. |
150
|
Fri Nov 11 08:07:18 2016 |
BCR SG NTB | BRIKEN Hit Visualization |
These are the files used to create and visualize the hit patterns of the BRIKEN detector.
There are three files needed plus one input data file. The three files are "HybridBRIKENPhysicalHistogram.hpp", "HybridBRIKENPhysicalHistogram.cpp", and "HybryidBRIKEN_Tube_Info_1.txt". These files are attached to this eLog entry.
In order to run this type in a terminal
root -l HybidBRIKENPhysicalHistogram.cpp+
The plus is important, it tells ROOT to compile this with the gcc compiler and then run that compiled version of the code. It runs slow, if at all, in the ROOT C++ interpreter CINT.
The code has been tested with ROOT v5.32 and v5.34, not version 6.
At the bottom of the HybidBRIKENPhysicalHistogram.cpp file is the "main program". In it you can set the input data file, which should be a BRIKEN online root output file, and the 3He energy cuts. It is easiest if all the files are in the same folder. If there are any questions please feel free to email B. Charles (Charlie) Rasco. |
314
|
Sat May 27 10:36:20 2017 |
JA,AT,JLT | BRIKEN DACQ |
Manuals for BRIKEN DACQ:
GasificShort.pdf including "Run protocol"
and Gasific70Manual.pdf (long) |
310
|
Fri May 26 14:27:08 2017 |
AIM, AT | BRIKEN Configuration File |
New configuration file of BRIKEN
Changes of 26th-May-2017
Previous config file 24th-May-2017
After the 152Eu calibration, the threshold of
>> V2A7C4 was increased from 20 to 30.
>> V2A7C6 was increased from 30 to 40.
AIDA veto plastic (40cm after the stack of DSSD) and
the silicon detector (shielding hole) were calibrated
with the Compton edge of 137Cs (891keV). |
390
|
Thu Oct 25 09:07:00 2018 |
ATS & JLT | BRIKEN Calibration check |
We put the 252Cf source and check the aligment of 3He tubes gains:
File: 181025_1600_252Cf_gaincheck.root
All OK except 133, 35 and 140
He133: peak at 744keV
He135: peak at 783keV
He140: peak at 739keV
No gain correction applied at the moment but should be verified
before experiment |
107
|
Thu Nov 3 23:28:01 2016 |
A. Tolosa | BRIKEN Bkg + 152Eu |
Measurement over night with a 152Eu source inside
Start: 22:48 (03/11/2016)
Stop: 08:26
File: 161104_0826_152Eu.root
Neutron background rate: 0.82 n/s |
90
|
Sun Oct 16 12:58:34 2016 |
All | BRIKEN |
Installation of BRIKEN PE shielding for beam
related neutrons
The missing metallic pieces needed to mount
the forward PE shielding finally arrive and
we mount it with help of the crane.
The shielding (4 PE slabs + 1Cd-PE slab) has attached
the support for VETO detectors on the beam side
and for and additional ancillary detector
a large Si detector on the BRIKEN side.
See attached photos.
The distance between shielding and BRIKEN is 40 cm. |
206
|
Tue Mar 28 17:02:19 2017 |
DK | Applying Biases |
Today, Gabor and I discussed with Nathan from ORNL about the biasing system used for Ge, 3He, Plastic, and others. Phong is also a bit familiar with the system (edit also
Shintaro
Go). While there
is supposed to be a manual, Gabor and I did not find it.
In case of trouble: contact Nathan Brewer Gmail: Brewer.nathant@gmail.com Skype: nathan.t.brewer
Log in to high voltage PC:
$ ssh -Y pixie16@10.32.6.161
passwd: ************
For HV readout, run firefox in the background
$ firefox &
You can probably check the history or restore pages, but it should be pointed
at 192.168.13.239
It updates automatically every several seconds. Unless the HV monitor is
running, it may show nothing...
For temperatures:
$ cd ~/DAQ_1/kelvin
$ ./kelvin-read
(there are options to kill all temperatures)
For applying existing HVs (BE CAREFUL!)
$ cd ~/DAQ_1/hv-mpod
$ ./hvmon
If you want to change the voltages (up or down) kill this with Ctrl+C
To alter bias values or change which ones are on, you can edit the file:
$ ~/DAQ_1/include/hvmon.conf
Once the file is saved, restart hvmon.
We are running the above in a GNU screen session, with firefox on one computer. It has a note taped to it. Please don't use this computer for other purposes unless necessary!
Let me note that the PC we log in through has essentially no .screenrc file so you can barely understand you are actually using screen. If you are not very familiar with
screen, better not to touch it. I will put a better .screenrc later (but I also don't want to change the setup now).
28 Mar 2017 15:47:31
Ge voltage application
LN2 filling was done yesterday before lunch
D is the beam left side Ge
MPOD name
U300 D4K
U301 D4R
U302 D4G
U303 D4B
83.7 K, with 300 V
G is the beam right side Ge
MPOD name
U304 G7K
U305 G7R
U306 G7G
U307 G7B
79.6 K with 250 V (except G7R at 300 V)
All analog signals are seen in the oscilloscope with reasonable behavior
28 Mar 2017 15:56:03
Ramp up all Ge clovers.
D at 3000 V for all
G at 2500 V for all (except G7R is 3000)
28 Mar 2017 16:26:39
Biases are all applied (maybe several minutes earlier)
D4 temp 83.7 K
G7 temp 79.6 K
28 Mar 2017 17:51:09
Now we ramp up 3He and plastics. We keep the Ge on during this time.
D4 83.7 K
G7 79.6 K
Everything looks good! |
113
|
Sat Nov 5 03:36:34 2016 |
Tain et al | Ancillary detectors |
Some info on ancillary detector signals
Plastic veto detectors (Top and Botomm):
The dynode signal of the PMT is passed through an
ORTEC 474 TFA amplifier before going to the DACQ
TFA: Gain=6 x min(~x2), Tint=200ns,Tdif=100ns, NonInvert
DACQ channels: Top: V1A7C1, Bottom: V1A7C2
Photo of the signals of both detectors attached
with 60Co source (with gain changed to 20 x max(~x12.5))
200ns wide 70mV high signal
With this info a rough calibration was established:
for the 2V range an ADC unit is 2000mV/16384=0.122mV
the 70mV (~1MeV) correspond to 574 ADC units which
with the change of gain 6*2/20/12.5=0.048
become 27.6 ADC units. We checked with Gasific
that roughly 1 ADC unit corresponds to 2 EFIR units
thus the calibration is 1/2/27.6=0.018 MeV/unit
NOTE: the calibration in online spectra taken
before noon Sunday 6 was wrong by a factor 2
too large!!!!
Si detector (Top and Bottom halves):
Signal from preamplifier in the low gain mode for the measurement:
we see nothing on the scope with 60Co source. In the high gain mode
we saw the other day a negative 6microsec wide 1mV high
signal with a 60Co.
AIDA plastic veto:
The signal from the PMT is going through a CAEN
shaping amplifier. The signal has a bipolar shape
with a rise time of 500ns a total width of 2microsec
and a height of 100mV (60Co)
F11 ToF plastic (Left and Right):
The signals are processed in the same way that the
plastic veto detector with TFA using the same settings.
Polarity of the signal unknown.
Currently we see no signal seems its not connected.
We found later that the NIM crate where the
TFA were sitting was not on!
We just made a calibration with beam particles
LISE was used to estimate an energy loss of 65 MeV for the ions. |
333
|
Fri Oct 20 08:27:05 2017 |
BC Rasco | Analysis Slides |
Here are the ORNL/UTK BRIKEN analysis slides presented by BC Rasco on 2017/10/20.
Enjoy the fine reading.
The online seems to be missing some slides, but the pdf has all of the slides. |
22
|
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
|
23
|
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 |
401
|
Tue Oct 30 01:01:42 2018 |
JLT, AA | Adjustment of 3He thresholds |
Background with BigRIPS+ZD already working
No pulser
After adjustment of thresholds the rate of BRIKEN noise
was reduced to 4.5kHz
The corresponding configuration file is:
181030_Conf_BrikenFull_LowThrAdj_masterCLK.xlsx
To be decided if we want to reduce further the noise rate
We also changed the calibration of the F11 plastic to have it in the histogram range
F11_PL_R_LG: 2.73 -> 1.0
F11_PL_L_LG: 2.32 -> 2.0
Further adjustment of few channels: Now noise rate is 2.7kHz
(2018/10/30 15:45) |
315
|
Sat May 27 11:19:57 2017 |
AIM, AT | AIDA+BRIKEN background |
Background measurement AIDA+BRIKEN
AIDA is inside BRIKEN
AIDA was taking data.
Start: run 31 subrun 41
Stop: run 41 subrun 239
BRIKEN started later.
Start: 27th-May, 19:19
Stop: 28th-May, around 11:00
DLT File name:170527_1919_bck_AIDAinside_022.dlt
RUN numbers: 022-024
RootFile: 170527_1919_1914_bck_AIDAin.root
Comments: at 28th-May, 19:17, reset time stamp |
18
|
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 |
124
|
Mon Nov 7 04:49:57 2016 |
Tain, Ale | AIDA plastic (veto) and Si de calibration |
AIDA plastic (veto) and Si de calibration
For the calibration the Compton edge of the spectrum seen in the detectors was used.
There is a large uncertainty in that determination, since the spectra are not so clear in terms of shape.
For the spectra V1A7C13_EFIR (Si de, top) the channel position is 12900 units
For the spectra V1A7C14_EFIR (Si de, bottom) the channel position is 12950 units
For the spectra V1A7C9_EFIR (AIDA plastic) the channel position is 10425 units
These corresponds to the following calibration factors using 0.9 MeV as the Compton energy from Co source:
V1A7C13_EFIR (Si de, top): 6.976744E-5
V1A7C14_EFIR (Si de, bottom): 6.949807E-5
V1A7C9_EFIR (AIDA plastic): 8.633094E-5 |