ID |
Date |
Author |
Subject |
33
|
Tue May 21 10:54:24 2019 |
A. Algora | Background |
Start: 18:55
Stop: 20:01
Lmd: Background_201905211855_068.dlt
Root:201905212001_background.root
Rates: 1.7 kHz (Dyn), 1.9 kHz (Anodes)
Comment: all measurements of today can be used to characterize the full detector.
Sources were possitioned in the center of the spectrometer, with the piece created at Ific |
83
|
Fri May 31 09:49:08 2019 |
A. Algora | Backgroun, beam on |
Start: 17:49
Stop: 22:11
Root: 201905312211_background_AIDA_in.root
Comments: |
52
|
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. |
144
|
Wed Jun 19 05:10:15 2019 |
Alvaro | Aida plastic - gain change |
TAC AIDAPL - CryA changed
After increasing the gain, x2 peaks in TAC |
Attachment 1: changeGainAPL.png
|
|
69
|
Wed May 29 09:08:11 2019 |
A. Algora | AIDA plastic setting changed |
AIDA plastic changed.
HV was at 1000 V, it was changed to 1300 V
Coarse gain was changed to x5, Fg remains as it was.
I had only two minutes to enter (it was a rush). Better to verify it again |
104
|
Sat Jun 8 04:22:39 2019 |
Jorge Alvaro | AIDA TAS correlation with 137Cs |
Files at mars /home/briken/190607AidaTasTest137Cs
For this experiment TAS Signal is stored |
Attachment 1: BetaTas137Cs.png
|
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Attachment 2: BetaGAmma137Cs.png
|
|
119
|
Fri Jun 14 16:22:25 2019 |
AT, OH, JA, CG, TD | AIDA Sync |
Problem with the sync checker appeared AIDA was not its notmal 14us out from DTAS.
Check with source shows we are in sync still
AIDA files R34_1 and R34_2 |
Attachment 1: AIDACorrelation.png
|
|
55
|
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) |
47
|
Fri May 24 10:57:37 2019 |
A. Algora | 60Co, AIDA out, possitioned 5 mm deeper |
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 |
Attachment 1: 201905242020_60Co.root
|
49
|
Sat May 25 02:11:09 2019 |
A. Algora | 60Co source, red box, no sources around, No AIDA |
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. |
Attachment 1: 201905251131_60co.root
|
Attachment 2: 20190525_Conf.xlsx
|
23
|
Mon May 20 10:02:43 2019 |
A. Algora | 60Co again, with better threshold settings |
Start: 18:06
Stop: 20:20
Rates: 14 kHz (Dynodes) 12.7 kHz (anodes)
Lmd: Co60_source_201905201806_037.dlt ...Co60_source_201905201806_045.dlt
Root: 201905202020_60Co.root |
Attachment 1: 201905202020_60Co.root
|
38
|
Wed May 22 09:01:43 2019 |
A. Algora | 60Co (source CD 395) with AIDA in |
Start: 17:00
Stop: 17:40
Lmd: Co60_source_AIDA_201905221700_072.dlt ..Co60_source_AIDA_201905221700_074.dlt
Root: 201905221740_60co_with_Aida.root
Rates: 13.2 kHz (Dyn), 12.6 kHz (Anodes)
Comments: 60Co source with AIDA in, red box, CD 395 . The source is not centered. It is positioned (the center of the source) at 14.6 cm
from the beam side external edge of the frame (lower NaI numbers). The holder is touching the nose of AIDA.
The nose of AIDA is 16 cm from the external edge of the frame (down stream). In that position Si # 3 is at the center of the DTAS according to Tom.
We have to be very careful when AIDA is moved in. Some of the AIDA flat connector cables are touching the connectors of our NaI cables.
Individual rates (kHz), remember the source is not at the center, so we expect assymetry in the counting rates):
Dy01 2.2 An01 2.27
Dy02 0.88 An02 0.91
Dy03 2.08 An03 2.20
Dy04 0.87 An04 0.86
Dy05 2.10 An05 2.17
Dy06 0.90 An06 0.89
Dy07 2.01 An07 2.13
Dy08 0.93 An08 0.93
Dy11 0.60 An11 0.68
Dy12 0.36 An12 0.33
Dy13 0.57 An13 0.62
Dy14 0.35 An14 0.33
Dy15 0.58 An15 0.65
Dy16 0.35 An16 0.33
Dy17 0.54 An17 0.62
Dy18 0.32 An18 0.31 |
Attachment 1: 201905221740_60co_with_Aida.root
|
29
|
Tue May 21 07:07:36 2019 |
A. Algora | 22Na, source 700 |
Start: 15:08
Stop: 15:42
Rates: 19 kHz (Dynodes), 16 kHz (anodes)
Lmd: Na22_source_201905211508_059.dlt ...Na22_source_201905211508_062.dlt
Root: 201905211543_22Na.root
Source details: 22Na, ID NA 401, 700, 1.038 x 105 Bq (2010/03/16), key 5,
It appears in the Sunflower home page as 09-7007 with an estimated activity of 8.9 Bq/s today
Comment; seems dynode 4 moved a little up. Most detectors keep a reasonable alignment
When overlay was marked, it did not save the root file. Root attached and tested |
Attachment 1: 201905211543_22Na.root
|
31
|
Tue May 21 08:55:20 2019 |
A. Algora | 152Eu, source ID 272 |
Start: 16:56
Stop: 17:46
Rates: 12.6 kHz (dynodes), 12 kHz (anodes)
Lmd: Eu152_201905211656_064.dlt ... Eu152_201905211656_066.dlt
Root: 201905211746_152Eu.root
Source details: 152Eu, ID: EU401, 272, 1.06x10**4 Bq (2010/03/16), key 9
Comments: |
Attachment 1: 201905211746_152Eu.root
|
46
|
Fri May 24 09:43:49 2019 |
A. Algora | 137Cs source, AIDA out, to check assymetry |
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. |
Attachment 1: 201905241851_137Cs.root
|
40
|
Thu May 23 02:48:29 2019 |
A. Algora | 137Cs short run with AIDA in |
Start: 10:48
Stop: 10:58
Root: 201905231058_137Cs_with_Aida.root
Comment: Aida in, source in the position as in the earlier entries. Just to check if there is any jump. No lmd, only root.
No large displacements. Det Dyn1 seems to have slightly larger statistics. The assymetry of the two sides is clear, as it should be.
|
Attachment 1: 201905231058_137Cs_with_Aida.root
|
54
|
Mon May 27 07:15:06 2019 |
A. Algora | 137Cs run, AIDA out, source in the center |
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.
|
Attachment 1: 201905271531_137Cs.root
|
35
|
Wed May 22 06:31:54 2019 |
A. Algora | 137Cs quick test of alignment |
Start: 14:32
Stop: 14:37
Source: 137Cs
Comments: Detectors show small drifts, of the order of the precision of the HV (we could apply 0.5 V corrections to align some of them, but I will not touch them now)
Dy16 looks quite off in the background measurement, but not with the Cs one !!!.
Calibrated spectra: Dy3 an An3 moved a little in the same direction, An12 looks also a little displaced.
Now I plan to measure some sources with AIDA in. It means that the sources will not be centered. The available distance from the oposite side to
the nose of AIDA is 16 cm. |
Attachment 1: 201905221437_137Cs.root
|
9
|
Wed May 15 11:50:04 2019 |
Algora, Nacher | 137Cs listmode, and rootfile |
137Cs source in the center of the DTAS, with the IFIC holder
list mode files: Cs137_Source_20190515_000.dlt to Cs137_Source_20190515_005.dlt
Root file: 201905151942_137Cs.root
|
Attachment 1: 201905151942_137Cs.root
|
36
|
Wed May 22 07:15:00 2019 |
A. Algora | 137Cs (4763) with AIDA in |
Start: 15:15
Stop: 15:50
Lmd: Cs137_source_AIDA_201905221515_069.dlt ..Cs137_source_AIDA_201905221515_070.dlt
Root: 201905221550_137Cs_with_Aida.root
Rates: 7.5 kHz (Dyn), 7.8 kHz (Anodes)
Comments: 137Cs source with AIDA in, Source CS401, 4763. The source is not centered. It is positioned (the center of the source) at 14.6 cm
from the beam side external edge of the frame (lower NaI numbers). The holder is touching the nose of AIDA.
The nose of AIDA is 16 cm from the external edge of the frame (down stream). In that position Si # 3 is at the center of the DTAS according to Tom.
We have to be very careful when AIDA is moved in. Some of the AIDA flat connector cables are touching the connectors of our NaI cables.
Individual rates (kHz), remember the source is not at the center, so we expect assymetry in the counting rates):
Dy01 1.1 An01 1.2
Dy02 0.35 An02 0.36
Dy03 0.97 An03 1.0
Dy04 0.34 An04 0.36
Dy05 1.1 An05 1.1
Dy06 0.4 An06 0.41
Dy07 1.0 An07 1.1
Dy08 0.37 An08 0.37
Dy11 0.27 An11 0.33
Dy12 0.15 An12 0.16
Dy13 0.25 An13 0.28
Dy14 0.15 An14 0.16
Dy15 0.28 An15 0.33
Dy16 0.15 An16 0.15
Dy17 0.25 An17 0.31
Dy18 0.16 An18 0.15
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Attachment 1: 201905221550_137Cs_with_Aida.root
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