AIDA GELINA BRIKEN nToF CRIB ISOLDE CIRCE nTOFCapture DESPEC DTAS EDI_PSA 179Ta CARME StellarModelling DCF K40 MONNET
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Entry  Sun Apr 2 00:44:01 2017, ID JA GK CG VP Liu JLT, 39Al run 75 
Date: 2/04/2017 
Start: 08:42
BRIKEN run: 75
AIDA Run: R24_0
BigRIPS run: 254

DLT:170402_0842_39Al_075.dlt

BRIKEN Rate: 1 cps 
F11 Rate: 12 cps 

Date: 2/04/2017 
Stop:09:00
BRIKEN run: 75
AIDA Run: r24_4
BigRIPS run: 254

Root file:170402_0842_0900_B075_Al39.root

OBSERVATIONS:
Entry  Fri Mar 31 00:01:55 2017, ID JA DK GK Liu, Run 030 
Date: 31/03/2017
Start: 07:58
BRIKEN run: 30
AIDA Run: R16_471
BigRIPS run: 173
DLT:170331_0630_Mg40_030.dlt

BRIKEN Rate:40
F11 Rate:11


Date:  31/03/2017
Stop: 8:57
BRIKEN run: 30
AIDA Run: R16_485
BigRIPS run: 173

Root file:170331_0012_0857_B030_Mg40.root
OBSERVATIONS:
Entry  Sat Apr 1 04:03:31 2017, ID JA DK GK, Na37 Ne36 run 056 
Date: 1/04/2017
Start:12:00
BRIKEN run: 56
AIDA Run: R20_131
BigRIPS run: 209
DLT:170401_1200_Na37_056.dlt


BRIKEN Rate: 1.5 cps
F11 Rate: 8.5 cps

Date: 1/04/2017
Stop: 12:58
BRIKEN run: 56 
AIDA Run: R20_176
BigRIPS run: 0209

Root file: 170401_0157_1159_B056_Na37Ne36.root
OBSERVATIONS: spectra was NOT cleared
Entry  Sat Apr 1 00:04:10 2017, ID GK DK Liu, 37Na or 36Ne labels? 
The BigRIPS settings are all called "36Ne setting" but the night shift labels these runs in the BRIKEN DAQ as
"37Na". We are not sure why we label it with 37Na, we think this should be consistently named 36Ne like the
BigRIPS settings. (For sure the strongest component in the beam might be 37Na. In the 39Na settings before it
was 40Mg and we labelled it 40Mg...)
Entry  Sat Apr 1 01:04:31 2017, ID DK JA, Na37 Ne36 Run 54 
Date: 1/04/2017
Start: 09:03
BRIKEN run: 54
AIDA Run: R20_115903
BigRIPS run: 206
DLT: 170401_0741_Na37_053.dlt
(change name, wrong starting time) corrected to 170401_0903_Na37_054.dlt

BRIKEN Rate: 1.5 cps
F11 Rate: 8.5 cps

Date: 1/04/2017
Stop: 
BRIKEN run: 54
AIDA Run: R20_130
BigRIPS run: 206

Root file: 170401_0157_1004_B054_Na37Ne36.root

OBSERVATIONS: PPAC discharges every ~10min (got better)
Entry  Sat Apr 1 02:07:49 2017, ID DK JA, Run 55 
Date: 1/04/2017
Start:10:04
BRIKEN run: 55
AIDA Run: R20_131
BigRIPS run: 207
DLT:170401_1002_Na37_055.dlt


BRIKEN Rate: 1.5 cps
F11 Rate: 8.5 cps

Date: 1/04/2017
Stop: 11:59
BRIKEN run: 55
AIDA Run: R20_160
BigRIPS run: 208

Root file: 170401_0157_1159_B055_Na37Ne36.root
OBSERVATIONS: 10:55 Beam stop few minutes
F11_PL_R Change the range and cleared 
Two Big rips files
Entry  Sat Apr 1 05:01:24 2017, ID DK GK JLT, 36Ne 37Na run 057 
Date: 1/04/2017
Start:13:00
BRIKEN run: 57
AIDA Run: R20_176
BigRIPS run: 210
DLT:170401_1200_Na37_057.dlt
(wrong starting time, should read 1300)

BRIKEN Rate: 1.5 cps
F11 Rate: 8.5 cps

Date: 1/04/2017
Stop: 14:44
BRIKEN run:  57
AIDA Run: R20_203
BigRIPS run: 210

Root file: 
OBSERVATIONS: spectra was NOT cleared. Some time with lower rates around 14:00
Entry  Sat Nov 26 09:31:05 2016, Gabor Kiss, Ariel Tarifeno, Alvaro Tolosa, Output signals from G7Red G7red_01.svg02.svg03.svg06.svg
Preamplifier of crystal G7Red was replaced. 
Output signals from G7Red are weird.

Several screen-shots of the signal are attached. The time calibration factor is 20ns/sample. 
Entry  Mon Feb 16 00:29:00 2015, Gabor KISS, Polyethyelene bottom1.JPGsmall2.JPG

The polyethelene arrived at RIKEN. Except 4 neighboring holes (located at the inner ring) the alignment is OK.

Entry  Fri May 26 03:24:38 2017, GK,VP, AT, AA, CLOVER, 133Ba 
133Ba source efficiency calibration, no AIDA

Start: 11:23
Stop: 11:43

Files: 
170526_1123_133Ba_noAIDA_z0cm_015.dlt
170526_1123_1143_133Ba_z0cm.root
Entry  Thu Mar 30 19:16:46 2017, GK,DK,JLiu,JA,JLT, 40 Mg run 24 
Date: 31/03/2017
Start: 03:14
BRIKEN run: 24
AIDA Run: R16_402
BigRIPS run: 168
DLT: 170331_0314_Mg40_024.dlt

BRIKEN Rate: 4
F11 Rate: 13


Date:  31/03/2017
Stop: 04:10
BRIKEN run: 24
AIDA Run: R16_416
BigRIPS run: 169

Root file: 170331_0012_0409_B024_Mg40.root
OBSERVATIONS: Previous online was cleared
Entry  Sat Nov 26 20:50:13 2016, GK, AT&AT, run 16-19 161126_1823_016_019_Rates.png161126_1823_016_019_Rings.png
=======    START    =======
Date 2016/11/26
Start time	: 17:21
BRIKEN run	: 016
Daq Conf. File	: 161125Conf_BrikenFull.xlsx
DLT File name	: 161126_1721_016
AIDA run	: R9-24
AIDA start	: 16:35
BigRIPS run	: 40Mg-1009
BigRIPS start	: 
---------------------------
Shifters:  GK, AT&AT
=======    Setup    =======
Central fragment:  41Al
--- Degraders ---
 Fixed: 3mm Pb between Musics 
 Variable: 
1=(0.5mm W+1mm Al), 2=(0.3mm W+1mm Al), 3=(1mm W +1mm Al)
1. OUT
2. IN
3. IN

=======  COMMENTS   =======
High gamma counting is affecting rings 1-4. (gammas in beam!?) 

------  Rates  ------
BRIKEN	:    1.12118e+02 cps
F11R	:    6.26962 cps
Clovers	:    1.72406e+04 cps
VPLT	:    1.82165e+01 cps
VPLB	:    9.08055 cps
AIDAPL	:    7.42954 cps

=========   END   =========
Date 2016/11/26
BRIKEN run	: 019
BRIKEN stop	: 18:04
ROOT online	: 161126_1823_016_019.root
AIDA run	: R9-43
AIDA stop	: 18:12
BigRIPS RUN	: 
Entry  Sat Apr 25 08:25:42 2015, G. Kiss, J. Agramunt, BRIKEN Test setup P1120020.JPGP1120023.JPGJap1Cf.pdfUS1Cf.pdf

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.P1120020.JPG

Entry  Mon Apr 27 04:40:43 2015, G. Kiss, J. Agramunt, neutron background at Eurica 

Based on an about 8h long background measurement, the neutron background at the Eurica site was found to be about 0.006 neutron / sec (in the Riken tubes) and 0.019 neutron / sec (in the ORNL tubes). The beam was OFF.

Entry  Mon May 11 09:14:54 2015, G. Kiss, 252Cf_data_sheet 252Cf_15_05_2006_3p7MBq.jpg

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 :-(252Cf_15_05_2006_3p7MBq.jpg

Entry  Mon Nov 5 09:32:00 2018, FM, JR, PA, AT, Low threshold, 252Cf, z=0cm, Perpendicular 0deg 
252Cf at z=0cm,ie center of moderator, source axis perpendicular at 0deg (typical orientation)
Low threshold.

18/11/05 START: 18:50
18/11/05 STOP:  20:45


** Configuration file: 
181016_Conf_BrikenFull_2153_test_thr.xlsx


ROOT file: 

181105_1850_252Cf_z0cm_2045.root


DLT files:

181105_1850_252Cf_z0cm_133.dlt
181105_1850_252Cf_z0cm_134.dlt
181105_1850_252Cf_z0cm_135.dlt
181105_1850_252Cf_z0cm_136.dlt




Comment: 
- Clovers are placed inside the moderator, front face ~5mm from AIDA hole border.
- AIDA not inside the moderator.
- In beam PE shielding placed.
Entry  Mon Nov 5 12:04:08 2018, FM, PA, AT, Low threshold, 252Cf, z=15cm, Perpendicular 0deg 
252Cf at z=15cm,ie center of moderator, source axis perpendicular at 0deg (typical orientation)
Low threshold.

18/11/05 START: 21:05
18/11/05 STOP:  22.30


** Configuration file: 
181016_Conf_BrikenFull_2153_test_thr.xlsx


ROOT file: 

181105_2105_252Cf_z15cm_2230.root


DLT files:

181105_2105_252Cf_z15cm_137.dlt
181105_2105_252Cf_z15cm_138.dlt
181105_2105_252Cf_z15cm_139.dlt




Comment: 
- Clovers are placed inside the moderator, front face ~5mm from AIDA hole border.
- AIDA not inside the moderator.
- In beam PE shielding placed.
Entry  Mon Nov 5 15:10:43 2018, FM, PA,, Low threshold, 252Cf, z=15cm, Parallel downstream 
252Cf at z=15cm, i.e 15 cm from the center of the detector,  source axis parallel downstream 
Low threshold.

18/11/06 START: 00:10
18/11/06 STOP:  01:32


** Configuration file: 
181016_Conf_BrikenFull_2153_test_thr.xlsx


ROOT file: 

181106_0010_252Cf_z15cm_0132.root



DLT files:

181106_0010_252Cf_z15cm_143.dlt
181106_0010_252Cf_z15cm_144.dlt
181106_0010_252Cf_z15cm_145.dlt





Comment: 
- Clovers are placed inside the moderator, front face ~5mm from AIDA hole border.
- AIDA not inside the moderator.
- In beam PE shielding placed.
Entry  Mon Nov 5 16:43:43 2018, FM, PA,, Low threshold, 252Cf, z=25cm, Parallel downstream 
252Cf at z=25cm, i.e 25 cm from the center of the detector,  source axis parallel downstream 
Low threshold.

18/11/06 START: 01:43
18/11/06 STOP:  03:03


** Configuration file: 
181016_Conf_BrikenFull_2153_test_thr.xlsx


ROOT file: 

181106_0143_252Cf_z25cm_0303.root



DLT files:

181106_0143_252Cf_z25cm_146.dlt
181106_0143_252Cf_z25cm_147.dlt





Comment: 
- Clovers are placed inside the moderator, front face ~5mm from AIDA hole border.
- AIDA not inside the moderator.
- In beam PE shielding placed.
Entry  Mon Nov 5 13:43:57 2018, FM, PA, Low threshold, 252Cf, z=0cm, Parallel downstream 
252Cf at z=0cm,ie center of moderator, source axis parallel downstream 
Low threshold.

18/11/05 START: 22:46
18/11/05 STOP:  00:01


** Configuration file: 
181016_Conf_BrikenFull_2153_test_thr.xlsx


ROOT file: 

181105_2245_252Cf_z0cm_0001.root


DLT files:

181105_2245_252Cf_z0cm_140.dlt
181105_2245_252Cf_z0cm_141.dlt
181105_2245_252Cf_z0cm_142.dlt



Comment: 
- Clovers are placed inside the moderator, front face ~5mm from AIDA hole border.
- AIDA not inside the moderator.
- In beam PE shielding placed.
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