AIDA GELINA BRIKEN nToF CRIB ISOLDE CIRCE nTOFCapture DESPEC DTAS EDI_PSA 179Ta CARME StellarModelling DCF K40
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Entry  Tue May 28 05:43:41 2019, A. Algora, 133Ba source. (IR052 from the third floor) 

Start: 13:43

Stop: 14:05

Comments: The source looks also too strong. Rates: 39 kHz (Dynodes), 40 kHz (anodes).

Source ID: IR052 from the third floor, small plastic rectangular form

Rates:

RefAn: 180 Hz

Dy01: 3.7 kHz

Dy02: 0.4 kHz

Dy11: 0.5 kHz

Dy12: 0.13 KHz

AIDA in. The source is put at the extreme of the source holder, at 16.5 cm from the edge of the detectors. Almost touching AIDA.

Lmd: 133Ba_source_AIDA_in_201905281343_227.dlt ..133Ba_source_AIDA_in_201905281343_230.dlt

Root: 201905281405_133Ba_AIDA_in.root

Entry  Tue May 28 05:30:03 2019, A. Algora, Reference detector threshold changed Screenshot_from_2019-05-28_13-29-46.png

Again the Reference detector was firing mainly in the noise. Threshold increased to 5000 !!!!

New config file was saved, rate of Ref detector now: aprox. 400 kHz

Entry  Mon May 27 13:58:03 2019, A. Algora, Background, no lmd, AIDA in, no sources around 201905281315_background_AIDA_in.root

Start: 21:59

Stop: 13:15 (next day, 28/05)

Rates: 1.9-2.3 (dynodes), 1.8-1.9 kHz (anodes)

Root: 201905281315_background_AIDA_in.root

Comments: Aida inside. No sources around

Entry  Mon May 27 13:50:54 2019, A. Algora, preparation directory moved 

The preparation directory was moved to /data/DRikenPreparation (from its first place /home/dacq/DRikenPreparation) because the lack of space.

Entry  Mon May 27 12:54:48 2019, A. Algora, Reference detector Screenshot_from_2019-05-27_20-54-21.png

The reference detector was very noisy. The threshold has been changed from 2000 to 3200. We should look at this more carefully.

The position of the fiber was also changed. It moved too close to the Cs peak. Probably it has to do with the flexibility of the plastik screw that fixes it.

 

 

Entry  Mon May 27 09:12:22 2019, A. Algora, Background, with AIDA Screenshot_from_2019-05-27_17-50-45.pngScreenshot_from_2019-05-27_17-51-02.png201905271803_background_AIDA_in.root

Start: 17:13

Stop: 18:03

Rates: 1.8 kHz (Dynodes), 1.8 kHz Anodes

Lmd: Background_AIDA_201905271711_210.dlt ... Background_AIDA_201905271711_226.dlt

Root: 201905271803_background_AIDA_in.root

Comments: AIDA in, in the same conditions as the earlier entry. Some asymetry in the spectra is seen. See EDy05 vs EDy15 and similarly EDy03 vs EDy13

Entry  Mon May 27 08:26:20 2019, A. Algora, Co source on top of Aida 201905271703_60Co_AIDA_in.root

Start: 16:28

Stop: 17:03

Rates: 14.4 kHz (Dinodes), 12.8 kHz (Anodes)

Lmd:  60Co_source_AIDA_201905271627_196.dlt .... 60Co_source_AIDA_201905271627_209.dlt

Root: 201905271703_60Co_AIDA_in.root

Comments: AIDA in, sligthly less deeper than before. It is 17 mm less deeper. So from the other side we measure 17.7 mm to the nose of AIDa.

The source is on top of AIDA with a help of a plastic ruler, that it is lying on top of it. The other extreme of the ruler is attached with tape to the edge

of the frame on the beam side. The source is positioned on top of the detectors 3, and 4, in practical terms in the geometrical center, but on top of 

AIDA. 60Co source from source box (key 3). No sources around, the sources are kept inside BELEN.

Entry  Mon May 27 07:34:58 2019, A. Algora, HV status 

EMPTY00    │   0.0 V 1500.0 uA    0.5 V    0.5 uA Off                │00.0000
DET01        │ 599.0 V 1500.0 uA  598.5 V   90.0 uA On                 │00.0001
DET02        │ 548.5 V 1500.0 uA  548.0 V   82.5 uA On                 │00.0002
DET03        │ 530.5 V 1500.0 uA  530.0 V   80.0 uA On                 │00.0003
DET04        │ 697.5 V 1500.0 uA  697.5 V  105.0 uA On                    Admi4
DET05        │ 451.5 V 1500.0 uA  451.0 V   67.5 uA On                       05
DET06        │ 820.0 V 1500.0 uA  820.5 V  123.0 uA On  Status             Ch06
DET07        │ 560.0──────────────560.0 V   84.0 uA On ────────────────┬─0.0007
DET08        │ 486.0 V 1500.0 uA  486.0 V   73.0 uA On                 │00.0008
EMPTY09    │   0.0 V 1500.0 uA    1.0 V    0.5 uA Off                │00.0009
EMPTY10    │   0.0 V 1500.0 uA    0.5 V    0.0 uA Off                │00.0010
EMPTY11    │   0.0 V 1500.0 uA    1.0 V    0.5 uA Off                │00.0011
EMPTY12    │   0.0 V 1500.0 uA    0.0 V    0.0 uA Off                │00.0000
DET11        │ 579.0 V  300.0 uA  579.5 V   86.5 uA On                 │00.0001
DET12        │ 506.0 V  300.0 uA  506.5 V   76.0 uA On                 │00.0002
DET13        │ 623.5 V  300.0 uA  623.5 V   92.5 uA On                 │00.0003
DET14        │ 649.5 V  300.0 uA  649.5 V   96.5 uA On                 │00.0004
DET15        │ 656.5 V  300.0 uA  656.5 V   97.5 uA On                 │00.0005
DET16        │ 530.5 V  300.0 uA  530.0 V   78.5 uA On                 │00.0006
EMPTY12    │   0.0 V 1500.0 uA    0.0 V    0.0 uA Off                │02.0000
DET11        │ 578.0 V  300.0 uA  578.0 V   86.5 uA On                 │02.0001
DET12        │505.5  V  300.0 uA  506.0 V   76.0 uA On                 │02.0002
DET13        │ 624.5 V  300.0 uA  624.5 V   92.5 uA On                 │02.0003
DET14        │ 650.0 V  300.0 uA  650.0 V   96.0 uA On                 │02.0004
DET15        │ 657.0 V  300.0 uA  657.0 V   98.0 uA On                 │02.0

DET16        │ 530.5 V  300.0 uA  530.0 V   78.5 uA On                 │00.0006
DET17        │ 462.0 V  300.0 uA  461.5 V   68.0 uA On                 │00.0007
DET18        │ 518.5 V  300.0 uA  518.5 V   77.5 uA On                 │00.0008
EMPTY19    │   0.0 V  300.0 uA    0.0 V    0.0 uA Off                │00.0009
EMPTY20    │   0.0 V  300.0 uA    0.0 V    0.0 uA Off                │00.0010
REF01        │ 800.0 V  300.0 uA  800.0 V  174.0 uA On                 │00.0011
EMPTY12    │   0.0 V 1500.0 uA    0.0 V    0.0 uA Off                │02.0000

 

Entry  Mon May 27 07:18:26 2019, A. Algora, AIDA Plastik 

Nishimura san found the module used for the AIDA plastik in the last BRIKEN run. We put it instead of the TFA. It was kept in the same

setting conditions as in the earlier experiment.

AIDA plastic module configuration (Ortec 671 Amplifier)

Coarse gain: 20

Fine gain: ?

Shaping time (us): 0.5

Type: Gaus

Signal pos

The configuration of the digitizer might need  to be updated (5)

Entry  Mon May 27 07:15:06 2019, A. Algora, 137Cs run, AIDA out, source in the center 201905271531_137Cs.root

Start: 15:15

Stop: 15:31

Lmd: 137Cs_source_201905271514_187.dlt .. 137Cs_source_201905271514_195.dlt

Root: 201905271531_137Cs.root

Rates: 7.9 kHz (Dynodes), 7.9 kHz (Anodes)

Comments: Aida out, source in the center. As in earlier measurements 5 mm deeper.

Reference detector might require repositioning of the optical fiber. It appears too close to the Cs peak and it is very noisy.

 

 

Entry  Mon May 27 07:11:22 2019, A. Algora, detectors realigned with Cs Screenshot_from_2019-05-27_15-13-09.png

Small alignment corrections were needed, of the order of 0.5-1V.

All detectors were realigned

Entry  Sat May 25 07:04:52 2019, A. Algora, Ancilliary card used channels until now 

For the moment there are three channels connected.

Channel 5 is AIDA plastic,

Channel 10 is the anode of the Ref detector

Channel 16 is the pulser.

Entry  Sat May 25 06:53:35 2019, A. Algora, Background, no dlt files, last config file 20190525_Conf.xlsx

Start: 14:53 (May 25)

Stop: 14: 37 (May 27)

Root: 201905271437_background.root

Comment: there is small assymetry between one side and the other. Probably it is determined by the closeness of the big wall in the direction of the beam

Entry  Sat May 25 03:42:12 2019, A. Algora, Background, no sources around, Aida out 201905251445_background.root

Start: 11:42

Stop: 14:45

Lmd: Background_201905251141_182.dlt ..Background_201905251141_186.dlt

Root: 201905251445_background.root

Comments: No sources around. All were taken back. Only doubful sources might be there, that I need to ask Nishimura san.

AIDA is out

Entry  Sat May 25 02:11:09 2019, A. Algora, 60Co source, red box, no sources around, No AIDA 201905251131_60co.root20190525_Conf.xlsx

Start: 10:27

Stop: 11:31

Root: 201905251131_60co.root

Lmd: 60Co_source_201905251027_176.dlt ...60Co_source_201905251027_181.dlt

Comments: possitioned as the measurements of yesterday. 5 mm deeper than earlier.

Red box with the other sources inside BELEN, far away from the DTAS

A few detectors have moved, but for the moment I will not correct it.

Reference detector in channel 10. It is very noisy now. I changed the threshold from 1400 to 1600 but still noisy. It requires further attention

New Config file saved.

Entry  Fri May 24 12:32:48 2019, A. Algora, Background measurement, no sources around 201905242111_background.root2019052521005_background.root

Start: 20:32

Stop: 10:05

Lmd: Background_201905242032_111.dlt ...Background_201905242032_114.dlt

removed the rest of the files. Ocupying too much space

Root: Background_201905242032_111.dlt (temporary) to play (until 21;11),

full: 2019052521005_background.root

Comment: all sources were taken back. Check for assymetry.

Entry  Fri May 24 10:57:37 2019, A. Algora, 60Co, AIDA out, possitioned 5 mm deeper 201905242020_60Co.root

Start: 18:58

Stop: 20:20

Lmd:  60Co_source_201905241858_095.dlt ...60Co_source_201905241858_106.dlt

Root: 201905242020_60Co.root

Comments: AIDA out. The source is possitioned 5 mm deeper as in the earlier Cs measurement (same position as the earlier entry)

To check asymmetry effects

Entry  Fri May 24 09:43:49 2019, A. Algora, 137Cs source, AIDA out, to check assymetry 201905241851_137Cs.root

Start: 17:43

Stop: 18:51

Root: 201905241851_137Cs.root

Lmd:  137Cs_source_201905241744_087.dlt...137Cs_source_201905241744_094.dlt

Comments: AIDA out. The source is positioned 5 mm deeper than before from the holder side (the arm is 5 mm longer).

To check if the assymetry is reduced.

Entry  Fri May 24 08:33:52 2019, A. Algora, background, AIDA is out 201905241730_background.root

Start: 16:35

Stop: 17:30

Rates: 1.5 kHz (Dynodes), 1.8 kHz (Anodes)

Listmode: Background_201905241635_082.dlt ...Background_201905241635_086.dlt

Root: 201905241730_background.root

Entry  Fri May 24 07:57:51 2019, A. Algora, Lead shielding heigth increased 

The aluminium plate of 3 cm thickness arrived and the lead shielding was dismounted and mounted again. We left a narrower hole in it.

Special thanks to Tom, who helped with the hard physical work.

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