ID |
Date |
Author |
Category |
Subject |
Text |
|
62
|
Sat Apr 2 01:27:25 2022 |
Jan Glorius | Runs | test runs 02.04.2022 | Beam settings:
primary beam
copper stripper
|
|
78
|
Sun Apr 3 12:31:10 2022 |
Rui-Jiu Chen, Yuri, Carsten, Ragan | Runs | Measurement of beam with different circles | Parameters of NTCAP:
1. IQ rate 20 MSamples/s
|
6x |
86
|
Mon Apr 4 09:10:44 2022 |
Ragan, Yuri, Rui-Jiu | Runs | Measurement | NTCAP is taking data with the beam with a
stop at manipulation 5 (taking all the fragments).
|
|
104
|
Tue Apr 5 23:55:11 2022 |
Carsten | Runs | Long time measurment with NTCAP | Settings:
Center: 2242.5MHz
RefLevel: -25dB
|
|
110
|
Wed Apr 6 14:52:29 2022 |
Rodolfo | Runs | Scraping the ion beam | We are T-scraping the ion beam. |
|
121
|
Thu Apr 7 02:32:29 2022 |
all on shift | Runs | First Scans 322-320nm | Laser scanning from 322-320 steps 0.01nm/s
DAQ1: lxg1927:/data.local2/BeamTimeTh22/
DAQ2: lxg0155:/data.local2/E142/
|
|
151
|
Fri Apr 8 06:53:29 2022 |
Ragan | Runs | NTCAP data taking | NTCAP is taking data since 07.04.2022 23:53:47
Carrier Frequency: 242.2 M
|
|
155
|
Fri Apr 8 09:32:32 2022 |
Ragan | Runs | NTCAP stopped | Since there is no beam, NTCAP is stopped.
Carrier Frequency: 242.2 M
|
|
157
|
Fri Apr 8 09:39:04 2022 |
Ragan | Runs | NTCAP started | Carrier Frequency: 242.2 M
IQ Rate (S/s): 10 M
Reference level (dBm): -30
|
|
158
|
Fri Apr 8 10:44:55 2022 |
Ragan, Yuri, Danyal, Sergey | Runs | NTCAP stopped | NTCAP is stopped. Sergey will now set an ion
bunch instead of two in the ESR.
|
|
161
|
Fri Apr 8 12:04:13 2022 |
Ragan | Runs | NTCAP started | NTCAP is started for the data taking.
Carrier Frequency: 242.02 M
|
|
166
|
Fri Apr 8 15:39:36 2022 |
all | Runs | first data after timing set up | started taking data again
started at 15:40
|
|
181
|
Sat Apr 9 06:25:22 2022 |
Max, Kristian | Runs | morning shift runs | DAQ1: lxg1927:/data.local2/BeamTimeTh22/
DAQ2: lxg0155:/data.local2/E142/
LMD file name DAQ1:229Thor
|
|
183
|
Sat Apr 9 13:45:42 2022 |
Max, Kristian | Runs | first scans with LV problem solved! | This is the first time with LV buffer problem
solved (see Elog ID: 184). Before the PMT
signals were out of sync with the wavelength |
|
185
|
Sat Apr 9 15:47:21 2022 |
Carsten, Rodolfo, Sarper, Patrick | Runs | Afternoon and night shift runs | After the morning shift, we got new increment
(nm) for the laser scanning. We are now scanning
2 nm of wavelength range in 5 big steps (5 |
|
195
|
Sun Apr 10 06:39:16 2022 |
Kristian, Marek, Max | Runs | runs morning shift 10.04. | These are the measurement runs of the morning
shift (10.04.).
|
|
200
|
Sun Apr 10 15:16:19 2022 |
Carsten, Rodolfo, Sarper | Runs | Runs afternoon shifts 10.04 | These are the measurement runs of the afternoon
shift (10.04.).
|
|
203
|
Sun Apr 10 22:47:05 2022 |
Patrick, Volker, Prannay, Danyal, Alexandre, Sebastian, Kristian | Runs | Runs night shift 10.04 + morning shift 11.04 | These are the measurement runs of the night
shift (10/11.04.).
|
|
210
|
Mon Apr 11 14:45:11 2022 |
Paul, Konstantin, Sarper, David | Runs | Afternoon shift runs 11.04 | We continue scan the new wavelength scan range
is 322.41 - 322.00 nm
|
|
215
|
Tue Apr 12 04:43:29 2022 |
Alexandre, Kristian, Sebastian | Runs | 322.01 - 321.60 nm | We scan the wavelength scan range is 322.01
- 321.60 nm
|
|
223
|
Wed Apr 13 14:29:04 2022 |
Carsten, Rodolfo, Sarper, David, Pierre-Michel, Max, Sebastian | Runs | Afternoon - morning shift runs 13.+14.04. | Changed the wavelength scan range from [B]321.62
- 321.10 nm[/B] to [B][B]321.12 - 320.60[/B]
nm[/B] after one scan.
|
|
230
|
Thu Apr 14 17:47:55 2022 |
Carsten, Rodolfo, Konstantin, Sarper | Runs | Afternoon shift runs 14.04 changing the wavelength scan range | The new scan range is changed from [B]321.12
- 320.60 nm to 320.62 - 320.10 nm[/B]
|
|
232
|
Thu Apr 14 22:44:40 2022 |
Patrick, Simon, Danyal, Max | Runs | Runs night shift 14./15.04. | Runs of the night shift. The wavelength range
is 320.62 - 320.10 nm.
|
|
236
|
Sat Apr 16 04:19:05 2022 |
Patrick, Simon, Alex, Sarper | Runs | Runs night + morning shifts 16.04. | Runs of the night shift 16.04. after changing
the wavelength range. The new range is 320.12
- 319.859 nm. The step size was decreased |
|
1
|
Mon Jul 26 17:15:47 2021 |
Rodolfo | Laser | Quanta Ray - Water leak | On Thursday afternoon (22.07.2021) a water
connector has broken and water has been spilled
in the laser head. |
|
2
|
Mon Jul 26 17:58:52 2021 |
Rodolfo | Laser | Water Filters | The water filters (deioninzing and particle)
have been replaced. |
|
4
|
Mon Aug 2 10:54:44 2021 |
Rodolfo | Laser | Quanta Ray - Water leak in the power supply | After fixing the broken water connector in
the laser head a new water leak appeared
in the Quanta-Ray power supply.
|
|
11
|
Thu Mar 3 13:50:45 2022 |
Rodolfo | Laser | Dye cell cracket | The "20 mm" dye cell used for the Oscillator
and Pramplifier got damage. I supposed it
was produced by the pump beam hitting on |
|
13
|
Thu Mar 3 17:34:42 2022 |
Rodolfo | Laser | Pump Laser | We have issues with our Pump Laser (Spectra
Physics - Quanta Ray Pro). After the service
made on mid Dezember (2021) the laser does |
|
14
|
Thu Mar 3 21:39:21 2022 |
Rodolfo | Laser | Dye solution, DCM in Ethanol and DMSO | I have prepared a new dye solution of DCM
in Ethanol and DMSO (1:1). The concentration
of the "oscillator + preamplifier" is 0,3 |
|
33
|
Thu Mar 24 16:59:35 2022 |
Rodolfo | Laser | Photodiode signal SO | Fast Photodiode signal at the "SO-Bogen" (South-east
arc).
|
|
35
|
Fri Mar 25 14:31:24 2022 |
Rodolfo | Laser | Photodiode signal SO in the Messhütte | Measured at the Panel "Messhütte - Laserhütte",
BNC "Fast PD / SO".
|
|
36
|
Tue Mar 29 12:01:08 2022 |
Rodolfo | Laser | Laser targets | I have installed two targets* (size: 2 inches)
to monitor the position of the laser beam.
|
|
38
|
Tue Mar 29 21:37:13 2022 |
Rodolfo | Laser | Pump Laser | The gold "reflectors and end plates" of our
pump laser (Quanta-Ray PRO) have been exchanged
by new ones.
|
|
80
|
Sun Apr 3 13:05:08 2022 |
Carsten | Laser | Distance of Partilce detecotrs wr.t. to electron cooler | As of Yuris post in the elog the positions
(Info from H. Weick):
|
|
82
|
Sun Apr 3 18:41:11 2022 |
Konstantin and Rodolfo | Laser | Beam Position Stabilization | We (Konstantin and I) have optimized the TEM
"laser-beam position stabilization".
|
|
101
|
Tue Apr 5 20:16:13 2022 |
Rodolfo | Laser | Discriminator for HF reference signal | For the laser trigger we need to generate
a few ns NIM-puls from the HF reference signal.
Therefore we (Wilfried, Konstantin and me) |
|
102
|
Tue Apr 5 20:58:53 2022 |
Wilfried | Laser | Trigger for Laser | Electronic for the timing of the laser puls
optimized. The problem with the broad photodiode
histograms is solved.
|
|
118
|
Thu Apr 7 00:15:11 2022 |
Patrick | Laser | Laser timing adjusted | We have adjusted the laser timing using PMT-middle.
Bunching freq. is 3.90362 MHz.
|
|
120
|
Thu Apr 7 01:19:05 2022 |
Patrick | Laser | Laser scanning | We did some laser scans. The wavemeter shows
spikes during scans. This may be just while
the frequency changes. See picture. |
|
136
|
Thu Apr 7 11:11:31 2022 |
Max, Sebastian | Laser | dye changed, pulse energy measurements | We changed the dye at 10am.
We increased the pump power for the dye Laser |
|
145
|
Fri Apr 8 00:06:37 2022 |
Patrick | Laser | Connection to the laser pc | To login to the laser pc use the command
xfreerdp -g 1920x1080 -u atplaser atppc023.campus.gsi.de |
|
148
|
Fri Apr 8 02:14:05 2022 |
Wilfried | Laser | Laser timings adjusted | Since we use the middle window as a reference
for the laser pulse timing, the fact that
the window is 2.25 m behind the target has |
|
149
|
Fri Apr 8 03:54:39 2022 |
Patrick | Laser | Q-switch window | The solution of increasing the Q-switch window
from 2us to 5us described in [I]ID:148[/I]
fulfills its purpose, but the window is unstable.
|
|
152
|
Fri Apr 8 08:17:52 2022 |
Sebastian | Laser | Laser Ext Trig is working | We (Max, Kristian, Danyal, me) fixed the "external
trigger" problem.
|
|
160
|
Fri Apr 8 11:16:57 2022 |
Kristian | Laser | Wavemeter | We changed the fiber to the wavemeter. The
third fiber worked best and we could operate
the WM at low exposure times, i.e., below |
|
180
|
Sat Apr 9 05:26:25 2022 |
Patrick | Laser | Wavemeter | The wavemeter still shows large spikes from
time to time. The exposure time is still
at 34ms. |
|
182
|
Sat Apr 9 06:42:23 2022 |
Kristian | Laser | Laser step size | We changed the laser step size to 0.002 nm
which corresponds to 5.75 GHz. |
|
186
|
Sat Apr 9 16:55:19 2022 |
Rodolfo | Laser | | 16:15 I have changed the dye (of both oscillator
and amplifier).
|
|
188
|
Sat Apr 9 19:09:57 2022 |
Rodolfo | Laser | Optimization - Resonator of dye laser | I have tuned a bit the resonator of the dye
laser.
|
|
196
|
Sun Apr 10 08:53:26 2022 |
Kristian, Max | Laser | Timing verified | timing is still good.
we checked the relative timing between laser |
|
197
|
Sun Apr 10 11:11:18 2022 |
Kristian, Max | Laser | additional WM readout | since the WM readout still does not work reliably,
I started a python script at atppc023 that
saves timestamp and wavemeter frequency. |
|
202
|
Sun Apr 10 15:29:53 2022 |
Rodolfo | Laser | Status - Laser system | We have checked the laser system.
- The pump laser has ~ 23Mio shots. The total |
|
208
|
Mon Apr 11 11:05:35 2022 |
Sebastian, Kristian | Laser | Check laser power | we checked the UV laser power at 10:15 am.
It was only 8.5 - 9 mJ. Pumping power was
460 mJ, which is the maximum output of the |
|
211
|
Mon Apr 11 18:46:31 2022 |
Rodolfo, Sarper and Konstantin | Laser | Alignment-check | We cross-checked the laser-ion alignment.
The horizontal position was optimized. However,
|
|
212
|
Mon Apr 11 18:57:18 2022 |
Rodolfo | Laser | New flashlamps | We (Sarper, Konstantin and me) have changed
the old flashlamps (with ~ 26 Mio. shots)
by new "fresh" ones. We have also exchange |
|
213
|
Mon Apr 11 22:14:51 2022 |
Konstantin, Sarper | Laser | Changing of the wavelength range | It is planned to change the scan range of
the laser wavelength from 322.41 - 322.0
nm to 322.01 - 321.6 nm @ 4 a.m. |
|
220
|
Tue Apr 12 15:05:56 2022 |
Rodolfo | Laser | Laser status | We have checked the laser power at 14:15 *
- Pump energy after Q-Ray @ 532nm: 559 mJ.
|
|
224
|
Wed Apr 13 15:41:29 2022 |
Rodolfo & Sarper | Laser | Laser status | We have checked the power of the laser and
optimized it "a bit".
|
|
231
|
Thu Apr 14 19:46:46 2022 |
Sarper & Konstantin & Rodolfo | Laser | Laser power | We checked the laser power before starting
the new scan range.
|
|
234
|
Fri Apr 15 12:53:25 2022 |
Max, Danyal | Laser | checked laser pulse energy after change in wavelength range | previous scan range:
the laser pulse energy @ 320.62 nm was ~11
mJ
|
|
235
|
Fri Apr 15 20:43:18 2022 |
Konstantin | Laser | Dye changed | Dye of the laser system has been changed.
UV laser power increased from ~8 mJ to 11
mJ pulse energy. |
|
237
|
Wed Apr 20 10:09:50 2022 |
Rodolfo | Laser | Optic with spots | The average energy produced by the laser along
the beamtime was about 10 mJ/puls. After
about two weeks of beamtime some of the optics, |
|
3
|
Wed Jul 28 13:31:22 2021 |
Rodolfo | General | Air filters | Filters (Hepa-) inside the flow boxes have
been replaced. |
|
Draft
|
Wed Sep 8 21:44:55 2021 |
Rodolfo | General | Preparation | [TABLE border="1"]
[B]Status[/B]|[B]Arbeitspaket[/B]|[COLOR=chocolate][B]Kommentare[/B][/COLOR]
|-
|
|
29
|
Wed Mar 23 15:38:15 2022 |
Carsten | General | Not all lights in the ESR can be switched off | Three of the lights in the ESR cannot be switched
off. It seems that these lights are now "emergency
lights" (with battery?). We will need to |
|
63
|
Sat Apr 2 05:08:00 2022 |
Kristian | General | Morning shift | I see no updates in the log. Is the morning
shift taking place?
|
|
64
|
Sat Apr 2 10:22:21 2022 |
Rui-Jiu Chen, Ragan | General | Beam is in the ESR | Primary beam is in the ESR now. Markus and
the team are tuning the ESR. |
|
106
|
Wed Apr 6 08:31:54 2022 |
Danyal & Regina | General | ESR had some errors | Regina noticed that the ESR was "red"
This means that there are some errors.
|
|
131
|
Thu Apr 7 08:14:03 2022 |
Yuri & Danyal | General | 229Th89+ line in Schottky | GLOBAL calculations for the "content" of the
Th line in the Schottky spectrum
(380 MeV/u exit energy, equilibrium charge |
|
138
|
Thu Apr 7 14:04:36 2022 |
Paul Indelicato | General | no beam until 17:00 | 10:10 There is a problem with the UNILAC.
The repair will take several hours. (4 hrs?) |
|
179
|
Sat Apr 9 05:00:11 2022 |
Carsten | General | Draft Docs and cheat sheet | Please check the attached files,
and correct or enhance them.
|
|
207
|
Mon Apr 11 10:31:07 2022 |
Kristian, Sebastian, Alexandre, Danyal, Paul | General | new laser wavelength scan range 322.41 - 322.00 nm | new wavelength scan range is 322.41 - 322.00
nm
|
|
214
|
Mon Apr 11 22:33:16 2022 |
Carsten | General | Backup of data to the external RAID disks | |
|
222
|
Tue Apr 12 21:56:54 2022 |
Volker, David, Pierre-Michel & Danyal, Alexandre, Sebastian | General | new laser wavelength scan range 321.62 - 321.10 nm | New wavelength scan range is [B]321.62 - 321.10
nm[/B]. Before the new scan range (compare
old scan range in [URL=https://elog.gsi.de/esr/E142/215] |
|
233
|
Fri Apr 15 12:42:18 2022 |
Max, Danyal, Carsten, Konstantin, Patrick, Simon | General | laser wavelength range changed: 320.12 - 319.60 nm |
Runs of the morning/afternoon/night shift.
The wavelength range is now 320.12 - 319.60 |
|
84
|
Mon Mar 25 06:22:12 143 |
Ken Ueberholz | Detectors | XUV-Detector Rates | Count rates were measured for the XUV-
detector for a full circle:
Cathode: -5V, shields: 0V, main coil 8A, |
|
8
|
Thu Oct 14 10:21:46 2021 |
Rodolfo | Detectors | Dismounting Cu-Mirror | We have dismounted the parabolic Cu-Mirror
at ESR on 13.10.2021 |
|
12
|
Thu Mar 3 17:21:26 2022 |
Rodolfo | Detectors | MgF2 Windows | New reentrance viewports made of MgF2 have
been installed at the ESR "Optical Detection
Region". In the middle the old window (also |
|
17
|
Wed Mar 16 12:04:40 2022 |
Kristian | Detectors | HV cable to particle detector South | Checked HV cable to particle detector south.
Label is HV2 Scraper.
|
|
28
|
Wed Mar 23 11:20:55 2022 |
Simon | Detectors | PMT operating voltages | During the testing of the PMTs the following
operating voltages were applied:
|
|
30
|
Wed Mar 23 16:16:42 2022 |
V. Hannen | Detectors | Control software for XUV and copper mirror detector | Attached you find a manual for the software
used to control the movement of the XUV detector
and the copper mirror detector.
|
|
31
|
Wed Mar 23 16:58:33 2022 |
V. Hannen | Detectors | Status copper mirror and XUV detectors | Over the past days, the parabolic copper mirror
and XUV detectors haven been prepared and
tested for the upcoming beamtime (see first |
|
40
|
Thu Mar 31 11:49:54 2022 |
Konstantin | Detectors | HV-Supply of particle detectors | We cross-checked the cabeling of the particle
detectors north and south. Particle detector
south is connected to channel [B]HV5[/B] |
|
42
|
Thu Mar 31 15:53:50 2022 |
Konstantin | Detectors | Control software for XUV and copper mirror detector | > Attached you find a manual for the software
used to control the movement of the XUV detector
and the copper mirror detector.
|
|
53
|
Fri Apr 1 15:27:00 2022 |
Rodolfo | Detectors | Nitrogen for UV-PMTs | There was a question concerning the nitrogen
we use to rinse the "Solar Blind PMTs".
|
|
54
|
Fri Apr 1 15:52:23 2022 |
Rodolfo | Detectors | UV PMT South | The "Solar Blind PMT" labeled as "PMT South"
has been installed by Simon and Max in the
gas target chamber on a CaF Viewport. The |
|
55
|
Fri Apr 1 16:46:33 2022 |
Carsten | Detectors | All pressuzied air drives are tested now and are working properly | All pressuzied air drives are tested now and
are working properly |
|
57
|
Fri Apr 1 18:30:38 2022 |
Carsten | Detectors | Positions / Voltages threshlds for particle detectors | [B]DC beam 238U92+ (205kV, e-beam)[/B]
We used the detector NA_SZ to determine the
central primary-beam (238U92+) position by |
|
58
|
Fri Apr 1 22:01:14 2022 |
Konstantin | Detectors | PMT operating voltages | > During the testing of the PMTs the following
operating voltages were applied:
>
|
|
59
|
Fri Apr 1 23:12:37 2022 |
Patrick | Detectors | Scraper positions "only primary beam" |
Scraper positions where there is only primary
beam for detector tests. Use only one outer |
|
60
|
Fri Apr 1 23:47:45 2022 |
Carsten | Detectors | PMT thresholds / PMT north does not allow voltage abow ~ -1kV | Checked thresholds of PMT with beam and without
beam.
|
|
77
|
Sun Apr 3 11:40:48 2022 |
Shahab, Yuri | Detectors | 245 MHz Resonator tuned to new frequency | resonance frequency changed from 243.2 MHz
to 244.692 MHz by reducing the value of both
of the plungers from 395 to 325. Now after |
|
97
|
Tue Apr 5 13:24:40 2022 |
Kristian | Detectors | PMT Cu | HV cable was in wrong channel in power supply.
Now it is back to the correct position. Checked
connection at the PMT. |
|
115
|
Wed Apr 6 19:39:08 2022 |
Ken Ueberholz | Detectors | LED installed | The UV-LED of Münster was connected over
channel 8 to the Messhütte. 6V are
supplied by the power supply (picture 2). |
|
116
|
Wed Apr 6 21:03:25 2022 |
Ken Ueberholz | Detectors | Xuv-Detektor, further information | Some further information regarding the
xuv-detector and its components. |
|
129
|
Thu Apr 7 05:55:17 2022 |
Ken Ueberholz | Detectors | XUV-Detector Mesytec crash | When the XUV-detector has to shut down unexpectedly,
it can happen that the Mesytek power supply
crashes and can't be
|
|
137
|
Thu Apr 7 14:01:22 2022 |
Sebastian, Max | Detectors | Mesytec reset | The Mesytec crate was turned off and on again.
It is again possible to communicate with |
|
139
|
Thu Apr 7 14:13:27 2022 |
Danyal | Detectors | new PMT south | I have replaced the PMT south (looks at the
gas target).
in the hope that this will produce less dark |
|
141
|
Thu Apr 7 16:45:10 2022 |
| Detectors | Detector distances | Relativ distances of the detector |
|
150
|
Fri Apr 8 05:46:35 2022 |
V. Hannen | Detectors | High background rate in Cu PMT points to light leak in ESR or active pressure gauge | The background rate of the Cu mirror PMT is
only about 300 cps when the mirror is in
the parking position but ca. 7000 cps when |
|
165
|
Fri Apr 8 14:46:02 2022 |
Danyal & Sebastian & Volker & Ken | Detectors | high dark countrate Cu PMT solved | The problem - "discovered" by Volker and Ken
- of the high dark countrate of the Cu PMT
has been solved.
|
|
191
|
Sun Apr 10 03:56:56 2022 |
V. Hannen | Detectors | Low rate in PMT South | PMT south shows a much lower count rate than
observed in elog entry 170.
|
|
217
|
Tue Apr 12 13:24:40 2022 |
Alexandre, Sebastian | Detectors | Sideband in Schottky | Sometimes we see a broad sideband at lesser
schottky frequencies to the high intensity
thorium beam.
|
|
218
|
Tue Apr 12 14:11:52 2022 |
Ragan | Detectors | Sideband in Schottky | > Sometimes we see a broad sideband at lesser
Schottky frequencies to the high-intensity
thorium beam.
|
|
219
|
Tue Apr 12 14:52:19 2022 |
Rodolfo | Detectors | PMT Nord, Middle. Datasheets | Attached are the datasheets for the solar-blind
PMTs.
|
|
221
|
Tue Apr 12 17:01:30 2022 |
Konstantin | Detectors | Voltage PMT North | Voltage of PMT North has been increased from
2500 V to 2600 V. Additionally the threshold
was adapted from 25 mV to 12 mV. |
|
228
|
Thu Apr 14 12:27:18 2022 |
Sebastian, Max | Detectors | Connection to XUV / Cu reestablished! | The connection to the XUV and Cu were lost
during the nightshift.
|
|
229
|
Thu Apr 14 12:38:38 2022 |
Sebastian | Detectors | XUV / Cu checkups | Check regularly if the connection to the XUV
and Cu detectors are still active and the
detectors move in (after injection) and out |
|
5
|
Fri Aug 6 10:23:00 2021 |
Rodolfo | DAQ | atplaser on r4l-41 | The user [B]atplaser[/B] is now existing on
the [B]R4L-XY[/B] nodes for the ESR group.
|
|
6
|
Fri Aug 6 10:40:54 2021 |
Rodolfo | DAQ | mbs in atplaser | The "MBS program" (data acquisition) is now
located within atplaser@r4l-41, in the folder
"th21":
|
|
9
|
Fri Nov 5 17:23:23 2021 |
Rodolfo | DAQ | Dye trigger out | The dye laser offers different scan settings
(see pages 65 - 67 of the user manual). We
are using the following setting, see attached |
|
15
|
Thu Mar 10 15:20:26 2022 |
Jan | DAQ | analog branch signal patches to Messhütte | The additional signals from PMTs and XUV detector
needed for spectroscopic analysis in the
second DAQ are patched to AP Messhütte (MH) |
|
16
|
Wed Mar 16 08:31:52 2022 |
Kristian | DAQ | Check cables and timing | Konstantin and I generated a signal in the
Messhütte and sent it to the ESR.
There, we used a 44m BNC cable that was sufficently |
|
21
|
Fri Mar 18 16:51:27 2022 |
Carsten | DAQ | Main DAQ /MBS error | MBS error "TDC data ready wait" solved. Common
stop trigger (20 kHz) was missing. (according
to Sebastian) |
|
24
|
Mon Mar 21 10:46:18 2022 |
Rodolfo | DAQ | TDC & Scaler description channels | For the First Vuprom we have the following
channel configuration (Stand:21.03.2021).
|
|
25
|
Mon Mar 21 16:33:23 2022 |
| DAQ | Changing code of go4 | We agreed to indicate changes in the go4 analysis
code according to the
following scheme
|
|
26
|
Mon Mar 21 17:03:47 2022 |
| DAQ | Changing code of go4 | Correction: Comments in C/C++ start with //
, i.e. forward slash
|
|
27
|
Mon Mar 21 21:48:46 2022 |
Jan | DAQ | MesyTec Shaper Control | The MesyTec Shaper & Constant Fraction (MSCF)
is used to process the PMT/det signals for
the ADC in the second DAQ.
|
|
32
|
Thu Mar 24 13:27:47 2022 |
Rodolfo | DAQ | Disk space - LXG1297 | In our Linux computer (LXG1297: Laser spectroscopy)
we have a Drive with 1.8 TB total disk space.
300 GB are at the moment in use, but I can |
|
34
|
Thu Mar 24 17:10:33 2022 |
Carsten | DAQ | DAQ / MBS VUPROM TDC buffer errors | VUPROM TDC buffer errors potentially due to
long TDC common Stop gate (>1ms from div
200).
|
|
41
|
Thu Mar 31 13:28:17 2022 |
Jan Glorius | DAQ | DAQ-2 cabling docu | newest version V2 - valid since Mo 04.April
2022 |
|
43
|
Thu Mar 31 17:56:32 2022 |
Konstantin | DAQ | Photodiode test signal | We used a signal generator to provide a 4MHz
dummy-RF signal. This was divided by a factor
of 2 for laser-"bunch" synchronization and |
|
44
|
Thu Mar 31 20:07:47 2022 |
Shahab | DAQ | Schottky Display in AP Messhütte (or anywhere else) | [B]UPDATE: 16.05.2022[/B]
[I]Please use ATPPC029 instead of ATPPC019 |
|
45
|
Thu Mar 31 22:19:14 2022 |
Kristian | DAQ | How To Start MBS | (MBS server should be running at the LXG1297
machine. If not you will get an error message.
Then start the server - last command in console)
|
|
49
|
Fri Apr 1 01:57:12 2022 |
Kristian | DAQ | Timing | with bunched primary beam (bunching frequency
1.94070 MHz) we have strong PMT (mid) and
particle detector signal. Time between both |
|
51
|
Fri Apr 1 11:00:41 2022 |
Rui-Jiu Chen | DAQ | Start NTCAP | Start taking data with NTCAP.
Carrier Frequency: 245MHz
IQ rate:5 MSamples/s
|
|
52
|
Fri Apr 1 11:19:57 2022 |
Rui-Jiu Chen | DAQ | S.M.A.R.T check on NTCAP | S.M.A.R.T. check has been done on NTCAP on
March 28th. All 12 hard disk drivers are
normal. |
|
79
|
Sun Apr 3 12:35:17 2022 |
Max | DAQ | Go 4 manual | How to start go4?:
- go to console
|
|
85
|
Mon Apr 4 00:19:16 2022 |
Ken Ueberholz | DAQ | FirstTests | New measurement:
Start: About 00:12
Stop: About 00:43
|
|
87
|
Mon Apr 4 15:27:31 2022 |
Sebastian | DAQ | PMT over wavelength histogram | Kristian and I tried to create a "PMT over
wavelength" histogram under step2Anl/LabView.
Unfortunately, the code ist still in progress |
|
88
|
Mon Apr 4 15:32:38 2022 |
Kristiand & Sebastian | DAQ | Go4 Backup Code | Due to some code changes (PMT over wavelength
historgram) Kristian and I backuped a working
Go4 code in the current go4 folder on the |
|
89
|
Mon Apr 4 16:26:04 2022 |
Carsten | DAQ | Backup Harddisk /External Disk | Since we cannot write on lustre, as a temproal
solution two RAID 1 (mirror) USB hard disks
with cpacity 6 TB each are installed.
|
|
90
|
Mon Apr 4 17:26:48 2022 |
Jan Glorius | DAQ | MSCF shaper settings | attached are the current shaper settings.
list of currently connected channels:
|
|
91
|
Mon Apr 4 19:05:57 2022 |
Carsten | DAQ | Cooler Frequency Signals Ion current not connected until now | Up to now the signals for
Ion Current
Cooler elctron current
|
|
92
|
Tue Apr 5 08:00:50 2022 |
Kristian & Sebastian | DAQ | MBS Channellist (so far) | MBS Channellist (time 5.4.2022)
0 Anode
|
|
95
|
Tue Apr 5 11:14:52 2022 |
Sebastian, Kristian, Pierre-Michel | DAQ | PMT over wavelength histogram v2 | Today we finalized the PMT over wavelength
histogram in:
|
|
96
|
Tue Apr 5 12:17:12 2022 |
Ragan, Rui-Jiu | DAQ | Instructions to start and stop NTCAP | Attached are the instructions to start and
stop data taking using the NTCAP. |
|
98
|
Tue Apr 5 13:28:06 2022 |
Kristian | DAQ | Spikes in PMT signal | Occasionally, we noticed a spike in the PMT
signal. No ions in the ring and at PMT Cu
was not even supplied with HV. Has to be |
|
99
|
Tue Apr 5 14:51:51 2022 |
Kristian | DAQ | dark counts | We shielded the PMTs, i.e., the N2 tube, which
improved the Cu PMT background rate.
|
|
100
|
Tue Apr 5 15:25:47 2022 |
Sebastian, Kristian, Pierre-Michel | DAQ | Go4 Conditions for "TDC_stacked_Sig/Ref" histogram | First version of TDC_stacked histograms implemented.
Under folder "Conditions" you can now integrate |
|
105
|
Wed Apr 6 08:06:02 2022 |
Danyal | DAQ | stopped NTCAP data acquisition | I stopped the NTCAP data acquisition at 8
AM.
|
|
108
|
Wed Apr 6 13:32:57 2022 |
Max, Sebastian | DAQ | LabView Cobra Channel List | channel 0: linux time (epoch time)
channel 1: ms timer
channel 2: E-Cooler Voltage(Ohmlabs)
|
|
119
|
Thu Apr 7 00:36:36 2022 |
Uwe | DAQ | Threshholds and shaping Mesytec for ADC | |
|
122
|
Thu Apr 7 03:06:15 2022 |
Patrick | DAQ | DAQ file sizes | The file sizes of DAQ1 (229Thor) and DAQ2
(229Th, "Carstens DAQ") are different.
During 20min of laser scanning DAQ1 saves |
|
123
|
Thu Apr 7 03:09:36 2022 |
Carsten | DAQ | NTCAP running since 02:40 | |
|
124
|
Thu Apr 7 03:44:21 2022 |
Patrick | DAQ | Measurement procedure | [U][B]Measurement procedure[/B][/U]
|
|
125
|
Thu Apr 7 04:10:18 2022 |
Ken Ueberholz | DAQ | Corrected cabling DAQ 2 | A lot of cables were wrongly or not
connected to the DAQ 2.
|
|
127
|
Thu Apr 7 05:23:50 2022 |
Patrick | DAQ | How To Start MBS for DAQ2 (Carstens DAQ) | (MBS server should be running at the LXG0155
machine. If not you will get an error message.
Then start the server - last command in console)
|
|
128
|
Thu Apr 7 05:44:40 2022 |
Pierre-Michel, Ragan | DAQ | NTCAP settings | Carrier Frequency: 244M
IQ Rate: 10M
reference Level: -30
|
|
130
|
Thu Apr 7 07:40:09 2022 |
Danyal, Max, Sebastian | DAQ | No beam and DAQs crashed | since shortly after 7 AM we have no beam in
the ESR
(reason unclear)
|
|
133
|
Thu Apr 7 09:23:18 2022 |
Sebastian | DAQ | DAQ1 & DAQ2 - 1kHz and delayed cs removed | Questionable 1kHz and delayed common stop
signals has been removed.
|
|
140
|
Thu Apr 7 15:18:25 2022 |
Danyal & Sebastian | DAQ | DAQ channels | We checked again the cables for both DAQs
(on Carsten's kind request)
|
|
146
|
Fri Apr 8 01:18:51 2022 |
Ken Ueberholz | DAQ | TODO: DAQ improvements | For somebody who knows the DAQ1 code: Go4
resets the histograms with each laser step.
Can there be additional histograms where |
|
147
|
Fri Apr 8 01:48:57 2022 |
Patrick | DAQ | Bugged Trending plots? | The wavelengths/frequencies shown in the graph
in the labview window do not match the wavelengths/frequencies
in go4.
|
|
153
|
Fri Apr 8 08:40:06 2022 |
Sebastian | DAQ | DAQ improvement | Concerning ID 146 a new histogram for accumulating
data (no cleaning histograms) can be found
under
|
|
162
|
Fri Apr 8 14:12:57 2022 |
morning shift | DAQ | timing for h=1 | The timing for h=1 has been set up
The time window is now twice as large as |
|
163
|
Fri Apr 8 14:14:28 2022 |
Kristian | DAQ | Delay of bunch RF | The bunch HF is now fed through a delay to
shift the stop trigger relative to the PMT
signal. The delay generator is placed directly |
|
164
|
Fri Apr 8 14:43:50 2022 |
Wilfried | DAQ | laser timing - Q-switch start | below are my notes concerning laser timing
/ Q-switch start |
|
170
|
Fri Apr 8 17:57:45 2022 |
Konstantin | DAQ | Laser scanning |
[TABLE border="1"]
|
|
171
|
Fri Apr 8 22:26:44 2022 |
Patrick | DAQ | Spike in all detectors | In the previous shift, there was a spike in
all detectors in the same scan step. Apparently,
this was NOT a resonance since in the next |
|
172
|
Fri Apr 8 23:56:07 2022 |
Patrick | DAQ | DAQ improvement | As requested in ID:146 and ID:147, the laserscan
tab was improved:
[LIST]
|
|
174
|
Sat Apr 9 03:27:47 2022 |
Patrick | DAQ | Laser scanning | DAQ1: lxg1927:/data.local2/BeamTimeTh22/
DAQ2: lxg0155:/data.local2/E142/
LMD file name DAQ1:229Thor
|
|
178
|
Sat Apr 9 04:40:01 2022 |
Patrick | DAQ | Bugged Trending plots? | The problem from yesterday (ID:147) still
persists. All the plots (not only the labview
stuff) comes in too late in go4. However, |
|
184
|
Sat Apr 9 14:15:44 2022 |
Kristian, Max, Konstantin | DAQ | Change in LV code | We changed the LV code so that the Cobra Set
Wavelength is permanently sent. Before it
was only sent once at the beginning of each |
|
190
|
Sun Apr 10 02:20:17 2022 |
Patrick | DAQ | New mbs startup guide | Connecting to the rfio server and opening
a file is included in '@startup' now. Since
mbs crashes reliably every 3 or 4 runs, it |
|
192
|
Sun Apr 10 04:07:53 2022 |
Patrick | DAQ | go4 shows wrong frequencies and wavelengths | [B]Update (ID:194):[/B] In labview "Stop All",
close labview, stop python script (ID:197),
close wavemeter. Then restart wavemeter, |
|
193
|
Sun Apr 10 04:37:29 2022 |
Patrick | DAQ | Next wavelength range | Measurements with the next wavelength scan
range should be started roughly around 12:00
noon. The plan is to go to lower wavelengths |
|
194
|
Sun Apr 10 06:34:49 2022 |
Kristian, Max | DAQ | Wavemeter Readout | Problem solved. Ignore this entry
|
|
198
|
Sun Apr 10 13:17:53 2022 |
Kristian, Max | DAQ | Wavemeter readout | We changed the Labview code in order to reduce
the amount of data that was overfilling the
WM data queue. We removed the temperature |
|
199
|
Sun Apr 10 15:08:42 2022 |
Carsten | DAQ | Backup of Data from 1rst Scanrange to extrenal RAID1 HDDs | I just performed a backup of all data (+log-Files)
that were collected until now to the two
RAID HDDs.
|
|
204
|
Mon Apr 11 04:26:53 2022 |
Patrick | DAQ | Next wavelength range | Measurements with the next wavelength scan
range should be started roughly around 10:00
am.
|
|
19
|
Thu Mar 17 17:56:33 2022 |
Kristian | Calibration | HV dividers | PTB HV dividers arrived. Divider ratios are:
PT120: 12003,341
|
|
46
|
Thu Mar 31 22:41:35 2022 |
Kristian | Calibration | HV divider | We noticed a difference in the electron cooler
high voltage:
|
|
56
|
Fri Apr 1 18:19:58 2022 |
Kristian | Calibration | HV divider | We checked the strange behavior of the HV
dividers again. The Ohmlabs and the PTB divider
are in good agreement at 120 kV and 150 kV. |
|
83
|
Sun Apr 3 18:52:30 2022 |
Konstantin | Calibration | Laser ion beam overlap | We measured vertical and horizontal ion beam
positions. Unfortunately, the horizontal
scraper positions can not be manipulated
|
|
142
|
Thu Apr 7 16:50:22 2022 |
Konstantin | Calibration | Spacial laser-ion overlap | Laser-ion-beam overlap was achieved after
measuring the ion beam positions (compare
[URL=https://elog.gsi.de/esr/E142/83]Entry |
|
143
|
Thu Apr 7 19:13:26 2022 |
Konstantin, Patrick | Calibration | How to find the correct laser position | In order to achieve the correct laser ion
beam superposition one needs to do the following
steps:
|
|
169
|
Fri Apr 8 17:44:25 2022 |
Konstantin | Calibration | Final Timing | We measured the timing for the laser bunch
synchronization. A summary is given below.
|
|
10
|
Fri Nov 19 15:50:44 2021 |
Rodolfo | Accelerator | Laser windows at E-Cooler side | New laser viewports have been installed at
the E-Cooler side of the ESR.
|
|
18
|
Thu Mar 17 17:37:49 2022 |
Rodolfo | Accelerator | High voltage dividers for E-Cooler | Two dividers, from PTB-Braunschweig, have
been deliver today. We will use them to monitor
the electron-cooler voltage in situ.
|
|
20
|
Fri Mar 18 09:18:38 2022 |
Rodolfo | Accelerator | Vacuum leak, ODR | After the beaking out process we got a vacuum
leak in one of the MgF2 windows (Referenz:
PMT South) of the optical detection region |
|
22
|
Fri Mar 18 16:58:26 2022 |
Rodolfo | Accelerator | Pressure at North-East Arc | The pressure at the north-east arc of ESR,
where the laser window is located, looks
suspicious. The sensor E01LF02 shows a value |
|
23
|
Mon Mar 21 09:18:28 2022 |
Rodolfo | Accelerator | Pressure at North-East Arc | Our vacuum expert has reply. The "IZ Pump"
in this region was off.
|
|
39
|
Wed Mar 30 09:27:15 2022 |
Rodolfo | Accelerator | Issue? Scrapers at E-Cooler | Carsten* forwarded me an E-Mail from Markus
yesterday. "Betreff: Scraper im ESR Elektronenkühler"
|
|
65
|
Sat Apr 2 15:54:32 2022 |
Carsten | Accelerator | ESR setup with primary beam and 1cm Be plate + Schottky data on NTCAP | MArkus and Bernd have setup the ESR with the
thick stripper foil and put the ion beam
(238U92+) on the central orbit.
|
|
66
|
Sat Apr 2 16:10:22 2022 |
Markus, Bernd | Accelerator | SIS setting complete, U90+ mit Be target: 2022-04-02_16-04-00_SIS18_FAST_E142_20220325_110213.C1.txt | # Version: 1.2
# Comment: ParamModi Export at 2022-04-02T16:04:10.778077+02:00[Europe/Berlin]
# Context: SIS18_FAST_E142_20220325_110213.C1
|
|
68
|
Sat Apr 2 18:17:31 2022 |
Yuri | Accelerator | Photo-Identification | Just a photo of the ID |
|
69
|
Sat Apr 2 18:19:47 2022 |
Yuri | Accelerator | Scraping | |
|
70
|
Sat Apr 2 18:28:47 2022 |
Markus/Bernd | Accelerator | SIS setting complete for fragments in ESR: 2022-04-02_18-09-10_SIS18_FAST_E142_20220325_110213.C1.txt | # Version: 1.2 # Comment: ParamModi Export
at 2022-04-02T18:09:36.402593+02:00[Europe/Berlin]
# Context: SIS18_FAST_E142_20220325_110213.C1 |
|
74
|
Sun Apr 3 10:28:25 2022 |
Yuri (Helmut Weick) | Accelerator | Distance cooler - detector | Calculation from Helmut Weick
Distance e-cooler to particle detectors chamber:
“This is half of ESR plus distance target |
|
75
|
Sun Apr 3 10:35:20 2022 |
Yuri (Sergey) | Accelerator | Dipole correction | The ramp for moving the beam to the central
orbit
To be inserted into manipulation, GE01MU1 |
|
76
|
Sun Apr 3 11:01:57 2022 |
Rodolfo | Accelerator | Scrapers @ E-Cooler | We the mid- and night shift (Wilfried, Simon,
Patrick, Ken and me) we not able to manipulate
the scrapers in the E-Cooler.
|
|
93
|
Tue Apr 5 09:39:01 2022 |
Danyal & Yuri | Accelerator | Strahl ist wieder im ESR - Schlitz war reingefahren | Der Strahl ist wieder im ESR!
Angeblich war einen Schlitz, oder sogar 2,
reingefahren worden.
|
|
94
|
Tue Apr 5 09:45:47 2022 |
Danyal & Yuri | Accelerator | beam is back in the ESR - a slit was moved in | And now also in English :)
The ion beam is back in the ESR!
|
|
103
|
Tue Apr 5 23:07:34 2022 |
Carsten | Accelerator | 229Th89+ identification after re-tuning of the ESR | The ESR was retuned this aftenoon since the
it was unclear if we still sit the 229Th89+
line.
|
|
107
|
Wed Apr 6 09:30:53 2022 |
Danyal | Accelerator | ESR is blue again - errors are fixed | The ESR is "blue" again.
The errors (scu related) have been fixed. |
|
111
|
Wed Apr 6 15:19:29 2022 |
Svea, Shahab | Accelerator | 5s delay implemented before injection | Operators have informed us that for better
stability and operation (and cooperation
with HHT), and after discussing with Sergey, |
|
112
|
Wed Apr 6 16:01:07 2022 |
BL | Accelerator | ESR settings before adjusting laser: 2022-04-06_14-37-30_ESR_EXP22_02_238U92_Brandau_30March22.C1.txt | # Version: 1.2
# Comment: ParamModi Export at 2022-04-06T14:37:35.957978+02:00[Europe/Berlin]
# Context: ESR_EXP22_02_238U92_Brandau_30March22.C1
|
|
113
|
Wed Apr 6 18:51:33 2022 |
Danyal & Carsten | Accelerator | target bump | This afternoon, we found out that Sergey has
also implemented a "target bump".
Although we do not use a target, this bump |
|
117
|
Wed Apr 6 22:29:55 2022 |
Patrick | Accelerator | ECooler voltages | ECooler voltages:
[B]06.04:[/B]
|
|
132
|
Thu Apr 7 08:43:19 2022 |
Danyal, Yuri, Ragan | Accelerator | again no injection in ESR - ESR kicker problem | we had no injections in the ESR again
it turned out that the injection kicker of |
|
134
|
Thu Apr 7 09:58:55 2022 |
Ragan, Yuri, Danyal | Accelerator | Kicker problem solved | The kicker problem is solved and the beam
is back in the ESR. |
|
135
|
Thu Apr 7 10:10:31 2022 |
Ragan, Yuri, Danyal | Accelerator | Problem in UNILAC | The power supply of the UNILAC magnet is broken.
The repair will take up to 6-7 hours. |
|
154
|
Fri Apr 8 09:13:38 2022 |
Ragan, Danyal | Accelerator | No beam | Cathode is being changed at the ion source.
So no beam for the moment.
|
|
167
|
Fri Apr 8 15:42:20 2022 |
Yuri | Accelerator | Slits in the TE line | At around 15:00, The slits in the TE line
were changed to :
TE4DS5HL -12 mm -> -20 mm
|
|
173
|
Sat Apr 9 02:55:38 2022 |
Carsten | Accelerator | Kühlerausfall und Gründe dazu | Wir hatten heute Abend eine Kühlerausfall,
der uns mehrere Stunden beschäftigt hat,
weil gem. Anzeige in Device Control kein |
|
175
|
Sat Apr 9 03:46:31 2022 |
Carsten | Accelerator | Slits in TE line | Changed GTEDSAH Rechts to 10mm |
|
176
|
Sat Apr 9 03:57:10 2022 |
Carsten | Accelerator | New Cooler voltage after the crash of the cooler | After the restart of the cooler the Ohmlabs
divider showed a voltage 16V lower than before.
This could also be seen as a slight shift |
|
201
|
Sun Apr 10 15:29:37 2022 |
Carsten,Sarper | Accelerator | Ecooler failed | Ecooler failed @15:23 Carsten is fixing it
Fixed @16:00 |
|
205
|
Mon Apr 11 07:54:37 2022 |
Danyal, Alexandre, Kristian, Sebastian | Accelerator | Jump in E-cooler voltage | We saw a jump in the E-cooler voltage at about
7:50.
jump from 209619 to 209610 V
|
|
206
|
Mon Apr 11 10:17:01 2022 |
Danyal | Accelerator | Interlock - reset | 10:17
Wie heutemorgen in der Sitzung (morning briefing)
vereinbart,
|
|
209
|
Mon Apr 11 12:50:22 2022 |
Kristian | Accelerator | Th lifetime | We used the counter to measure the lifetime.
During the 30 min scan time dropped only
slowly.
|
|
216
|
Tue Apr 12 12:41:20 2022 |
Alexandre, Sebastian | Accelerator | no beam in SIS18 | |
|
225
|
Thu Apr 14 06:29:18 2022 |
Max, Sebastian | Accelerator | lesser ESR injection intensity | We now have less ESR injection intensity (see
screenshot attached).
|
|
226
|
Thu Apr 14 08:41:42 2022 |
Carsten | Accelerator | Low intensity at the experiment after series of failures during the night | After the recovery from the failures during
the night, we see much lower intensity at
the experiment (measured with the particle |
|
227
|
Thu Apr 14 10:57:11 2022 |
Carsten | Accelerator | Maintanence UNILAC / Op training | We had no beam since about 1000. Also, we
are still trying to find out why we have
such a low intensity in the expereimnt.
|
|
37
|
Tue Mar 29 12:47:26 2022 |
Ken Ueberholz | | Parameter setting for XUV and copper mirror detector | Some Default Settings for the XUV
Detector. The copper
mirror should always move fully in.
|
|
47
|
Fri Apr 1 00:27:27 2022 |
Carsten | | Settings Particle Detectors /Tests with primary beam | All the beam settings will be given in a separate
post.
|
|
50
|
Fri Apr 1 02:29:40 2022 |
Carsten | | ESR Cooler crashed | ESR cooler crashed. We could not restart the
cooler. Since we had several other problems,
we stop now. |
|
Draft
|
Sat Apr 2 01:02:39 2022 |
Carsten | | Test measurements with two DAQs | We do two measurements:
One measurement using the |
|
67
|
Sat Apr 2 17:47:16 2022 |
Ken Ueberholz | | Telefon, Gästehaus | My guesthouse phone number: 06159-71-2957 |
|
71
|
Sat Apr 2 22:43:36 2022 |
Carsten | | Ring set-up for 229/89+, scraped and bunched, Iel=500mA at injection and 100mA during measurment | The ring SIS/ESR were set up for 229/89+.
Pölease note that this not only 1e- Th but
ponteially also the isobars of Ac (0e-1)/Pa(2e-, |
|
72
|
Sat Apr 2 23:16:55 2022 |
Carsten | | Cu mirror and CsI moved in and out of the ring | Ken tested the Cu-mirror and CsI disk Detector.
They move without a problem and don't scrape
the ion beam. |
|
73
|
Sun Apr 3 00:41:45 2022 |
Ken Ueberholz | | Xuv-Detektor Signale | The Xuv-detector cabel channels seem to be
wrongly labeled in the Messhütte (see
|
|
81
|
Sun Apr 3 15:34:34 2022 |
Ken Ueberholz | | Xuv-Detektor CFD-treshhold | I co controlled all detector signals and
adjusted the threshold to be just above
the noise. I will double check this when |
|
126
|
Thu Apr 7 04:48:58 2022 |
| | ToDo's for 07.04. | Some ToDo's for the next shift:
- Work on Laser stabilisation 2nd stage
in the ESR
|
|
144
|
Thu Apr 7 22:18:06 2022 |
Night shift 7.4-8.4 | | Next scans | DAQ1: lxg1927:/data.local2/BeamTimeTh22/
DAQ2: lxg0155:/data.local2/E142/
LMD file name DAQ1:229Thor
|
|
156
|
Fri Apr 8 09:33:52 2022 |
Dayshift 1 8.4.2022 | | Reference Measurements | DAQ1: lxg1297:/data.local2/BeamTimeTh22/
DAQ2: lxg0155:/data.local2/E142/
LMD file name DAQ1:229Thor
|
|
159
|
Fri Apr 8 11:02:04 2022 |
DW, YL, RSS, SL | | Change h=2 to h=1 | After changing to h=1
The frequency manipulation #5: f=242.021487MHz
(124th harmonic) [no bunching]
|
|
168
|
Fri Apr 8 15:45:24 2022 |
YL | | Spectrum manipulation 5 | See attached |
|
177
|
Sat Apr 9 04:01:35 2022 |
Carsten | | 2nd DAQ | Switched the CAEN TDC back on and changed
the threshoolds for the ADC to:
|
|
189
|
Sat Apr 9 19:50:40 2022 |
Carsten | | New thresholds for ADC of DAQ2 (starting with file0117) | unsigned short caen_V785AH_threshold_mod0
[32] =
{0x0100 , 0x0004 , 0x0003 |
|