| ID |
Date |
Author |
Subject |
|
308
|
Fri May 26 09:07:46 2017 |
J. Agramunt | Synchronization Monitoring |
We started the synchronization monitoring programs to check that
it is OK as can be seen in the figure below
We are using the same scheme used during Ahn parasitic run,
namely the synchronization check signal is the BigRIPS trigger
signal send by them to us (AIDA, BRIKEN).
The monitorization procedure is different from the one used
in 2016. The description to lauch the processes is described
here below and in the attached PDF.
***********
To Launch the processes:
Open 4 terminals:
Terminal 1 (DataSink) type:
>ssh aida@d05
>cd /home/aida/DataPackage/DataSink/Linux64
>DataSink -i 3
Terminal 2 (SynCheck) type:
>ssh aida@d05
>cd /home/aida/SyncCheck
>./SynCheck
Terminal 3 (BigRIPS Data Relay) type:
>ssh aida@d05
>cd /home/aida/ribfts/ribftssender
>./ribftssender_mar17ca debug
(specific for current 40Ca parasitic run because we are not sending
a pulse signal to BigRIPS as trigger but receiving triggers from
BigRIPS to create the pulses)
Terminal 4 (AIDA Data Relay) type:
>npg@aidas1
>DataRelayFilter -n 10.32.0.12 -p 10307 -I 2
"-I 2" selects ID 2 as the one for the AIDA data stream,
which must correspond to the one expected by the DataSink in the d05 PC.
The programming transmitting the data from AIDA to the DataSink includes an
intermediate filtering step. This selects only correlation scalers from one
module (and possibly ADC values from one channel in that module).
Gasific MainWindow (Briken Data Relay):
In the DAQ Control tab: Click "Start Sync Monitoring" button.
In the pop up window set server ip and port (ip:10.32.0.12, port:10305)
By default this perform a check on the differences RIBF-BRIKEN and AIDA-BRIKEN.
In case that BRIKEN is not running, the option "SynCheck -M 1" check the differences
AIDA-RIBF and BRIKEN-RIBF, while "SynCheck -M 2" checks RIBF-AIDA and BRIKEN-AIDA
To synchronize:
In the Gasific MainWindow, DAQ Control tab: Click "Send Sync Pulse" button |
|
210
|
Wed Mar 29 13:31:37 2017 |
J Agramunt, R. Caballero, T. Davinson, C. Griffin, O. Hall, D. Kahl, G. Kiss, J. Liu, S. Nishimura, V. Phong, JL Tain | Start of parasitic |
Start of parasitic Ca beam
(main experiment "New isotope search", Ahn et al.)
New directory: /data/1703Ahn/
Configuration file: 170329_Conf_BrikenFull.xlsx |
|
104
|
Thu Nov 3 05:46:48 2016 |
Iris, Ale | Background measurement |
Background measurement for threshold determination
Started at 14:45
Stopped: 16:35
Root file: 161103_1635_bck.root |
|
321
|
Mon Jun 12 02:45:44 2017 |
Iris Dillmann AT | Setup detectors. Id of Ancillary@BRIKEN |
Attachment 1: Setup detectors
Attachment 2: example of configuration file (valid only for RIBF127). The Id of the ancillary detectors are:
DTPulser 95
V_PL_T 96
V_PL_B 97
F11_PL_R_LG 98
F11_PL_L_LG 99
V_NaI_R 100
V_NaI_L 101
F11_PL_R 102
F11_PL_L 103
Si_T 104
Si_B 105
AIDA_PL 106 |
|
128
|
Mon Nov 7 09:05:09 2016 |
Iris | Draft for Run sheet |
Attached is the draft for the paper run sheet (version 2). If something is missing, please let me know. |
|
146
|
Wed Nov 9 01:02:53 2016 |
Iris | Elog |
From Nov. 9th on we use the Takechi ELOG for the run information:
http://ribf-exp.riken.jp/elog/RIBF123/ |
|
Draft
|
Wed Nov 9 01:04:35 2016 |
Iris | Drawing of present setup |
This is the setup which was used for the Ni runs (from Nov. 8th evening on).
Note (Nov. 10th): Alejandro built a U-shaped Pb wall, the degrader inside AIDA was removed and possibly a Al plate was installed. This has to be checked when access is possible again.
> Attached is the present setup including all walls, auxiliary detectors, degraders etc. and the Takechi setup.
> The lead wall will be removed for measurements (of course...).
> Not to scale! Some sizes and distances included. Pictures see Jose's entry ID 110.
>
> Note the shape of the active area of the DeltaE Silicon detector, see previous entry. |
|
148
|
Wed Nov 9 02:02:22 2016 |
Iris | Boron rubber from India |
The boron rubber from India is BR-2871, price US-$ 2700 for 2pc 1m x 2m x 3.3mm.
52% B content, density 1.61 g/cm3 |
|
247
|
Fri Mar 31 04:57:01 2017 |
ID,YS,JLT,OH | 40Mg run 35 |
Date: 31/03/2017
Start: 12:24
BRIKEN run: 035
AIDA Run: R16_536
BigRIPS run: 178
DLT: 170331_1224_Mg40_035.dlt
BRIKEN Rate: 4 cps
F11 Rate: 13 cps
Date: 31/03/2017
Stop: 1324
BRIKEN run: 035
AIDA Run: R16_551
BigRIPS run: 178
Root file: 170331_1222_1324_B035_Mg40.root
OBSERVATIONS: Online cleared |
|
273
|
Sat Apr 1 06:49:00 2017 |
ID,GK,JA,DK,SN,JLT | 37Na run 58 |
Date: 1/04/2017
Start:14:48
BRIKEN run: 58
AIDA Run: R20_203
BigRIPS run: 212
DLT:170401_1448_Na37_058.dlt
BRIKEN Rate: 1.5 cps
F11 Rate: 8.5 cps
Date: 1/04/2017
Stop: 16:37
BRIKEN run: 58
AIDA Run: R20_232
BigRIPS run: 213
Root file: 170401_0157_1637_B058_Na37Ne36.root
OBSERVATIONS:
We change in the online histograms (not on the configuration file) the range of F11_PL_R,L, _HG,LG, F11RgateSiT
and the gain of F11_PL_R,l_HG,LG
15:18 No beam. Continued running.
15:23 New BigRIPS file 213
16:14 No beam. RF problems. Continued running. |
|
243
|
Fri Mar 31 01:50:15 2017 |
ID, RCF | 40Mg Run 032 |
Date: 31/03/2017
Start: 10:01
BRIKEN run: 032
AIDA Run: R16_502
BigRIPS run: 175
DLT:170331_1001_Mg40_032.dlt
BRIKEN Rate: 4cps
F11 Rate: 11
Date: 31/03/2017
Stop: 10:22
BRIKEN run:032
AIDA Run: R16_506
BigRIPS run: 176(beginning)
Root file:170331_0012_1022_B032_Mg40.root
OBSERVATIONS: |
|
267
|
Fri Mar 31 23:41:57 2017 |
ID, LIU, DK, GK | 37Na run 53 |
Date: 1/04/2017
Start: 07:41
BRIKEN run: 53
AIDA Run: R20_94
BigRIPS run: 205
DLT: 170401_0741_Na37_053.dlt
BRIKEN Rate: 1.5 cps
F11 Rate: 8.5 cps
Date: 1/04/2017
Stop: 09:01
BRIKEN run: 53
AIDA Run: R20_115
BigRIPS run: 205
Root file: 170401_0157_0901_B053_Na37Ne36.root
OBSERVATIONS: PPAC discharges every ~10min (got better) |
|
288
|
Sat Apr 1 22:41:22 2017 |
ID, GK, SN, Liu YS JLT | 38Mg run 73 |
Date: 2/04/2017
Start: 06:37
BRIKEN run: 73
AIDA Run: R21_0
BigRIPS run: 237
DLT:170402_0637_38Mg_073.dlt
BRIKEN Rate: 5 -> 90 cps
F11 Rate: 30 -> 350 cps
Date: 2/04/2017
Stop: 08:06
BRIKEN run: 73
AIDA Run: r21_22
BigRIPS run: 251
Root file:170402_0637_0806_B073_Mg38.root
OBSERVATIONS:
Playing with degraders
Final degrader: 23mm
New BigRIPS run 238 started at 6:46 (38Mg beam attenuated by 1/8) -> very few counts in Si
New run 239-240 started at 7:03 (38Mg beam attenuated 1/2 narrow slit)-> we see more counts in the Si
run 241-242 atarted at 7:09 (38Mg 70% narrow slit)
run 243-244 at 7:16 (38Mg 5000enA)
run 245-246 at 7:23 (38Mg beam intensity 0.8)
run 247-248 at 7:32 (38Mg beam intensity 0.9)
run 249-250 at 7:38 (38Mg full beam)
run 251 at 7:41 (38Mg yield measurement) |
|
242
|
Fri Mar 31 01:01:58 2017 |
ID RCF OH | Run 031 |
Date: 31/03/2017
Start: 08:58
BRIKEN run: 31
AIDA Run: R16_485
BigRIPS run: 174
DLT:170331_0858_Mg40_031.dlt
BRIKEN Rate:3.5cps
F11 Rate:11
Date: 31/03/2017
Stop: 09:44
BRIKEN run: 31
AIDA Run: R16_498
BigRIPS run: 174
Root file:170331_0012_0944_B031_Mg40.root
OBSERVATIONS:
Beam stopped at 9:44 to change the C foil |
|
244
|
Fri Mar 31 02:26:19 2017 |
ID RCF | 40Mg Run 033 |
Date: 31/03/2017
Start: 10:23
BRIKEN run: 033
AIDA Run: R16_507
BigRIPS run: 176
DLT:170331_1023_Mg40_033.dlt
BRIKEN Rate: 4 cps
F11 Rate: 10 cps
Date: 31/03/2017
Stop: 11:22
BRIKEN run: 033
AIDA Run: R16_521
BigRIPS run: 176
Root file:170331_0012_1123_B033_Mg40.root
OBSERVATIONS: We started dividing he count rates by factor 10 (clock = 10 Hz) a few runs ago. Please check this.
Night shift has used the count rates directly from the plots. |
|
253
|
Fri Mar 31 11:46:44 2017 |
ID PV CG | 40Mg Run 041 |
Date: 31/03/2017
Start: 19:43
BRIKEN run: 41
AIDA Run: R16_647
BigRIPS run: 186
DLT: 170331_1943_Mg40_041.dlt
BRIKEN Rate: 40/ 10= 4 cps
F11 Rate: 12 cps
Date: 31/03/2017
Stop: 20:45
BRIKEN run: 41
AIDA Run: R16_662
BigRIPS run: 186
Root file: 170331_1943_2045_B040_Mg40.root
OBSERVATIONS: |
|
245
|
Fri Mar 31 03:26:53 2017 |
ID OH SN | 40Mg Run 034 |
Date: 31/03/2017
Start: 11:23
BRIKEN run: 034
AIDA Run: R16_521
BigRIPS run: 177
DLT:170331_1123_Mg40_034.dlt
BRIKEN Rate: 4 cps
F11 Rate: 13 cps
Date: 31/03/2017
Stop: 12:24
BRIKEN run: 034
AIDA Run: R16_536
BigRIPS run: 177
Root file:170331_1123_1222_B034_Mg40.root
OBSERVATIONS: We started dividing he count rates by factor 10 (clock = 10 Hz) a few runs ago. Please check this.
Night shift has used the count rates directly from the plots. |
|
274
|
Sat Apr 1 08:39:47 2017 |
ID OH JLT | 36Ne 37Na run 059 |
Date: 1/04/2017
Start:16:38
BRIKEN run: 59
AIDA Run: R20_232
BigRIPS run: 214
DLT:170401_1638_Na37_059.dlt
BRIKEN Rate: 1.5 cps
F11 Rate: 8.5 cps
Date: 1/04/2017
Stop: 17:39
BRIKEN run: 59
AIDA Run: R20_247
BigRIPS run: 0214
Root file: 170401_0157_1739_B059_Na37Ne36.root
OBSERVATIONS: |
|
246
|
Fri Mar 31 03:54:26 2017 |
ID JLT | Run 034: gamma spectra background lines |
There is a strong background line at ~1293 keV. According to the attached document this could come from the
neutron activation of 115In to 116In (14s halflife) of Indium seals. |
|
289
|
Sun Apr 2 00:19:01 2017 |
ID JA GK CG YS SN Liu VP | 39Al run 74 |
Date: 2/04/2017
Start: 08:17
BRIKEN run: 74
AIDA Run: R21_23
BigRIPS run: 252
DLT:170402_0817_39Al_074.dlt
BRIKEN Rate: 48 cps
F11 Rate: 320 cps
Date: 2/04/2017
Stop:08:20
BRIKEN run: 74
AIDA Run: r21_23
BigRIPS run: 252
Root file:170402_0817_0820_B074_Al39.root
OBSERVATIONS: |