ID |
Date |
Author |
Category |
Subject |
Text |
|
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.
|
|
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, |
|
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]
|
|
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 |
|
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
|
|
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. |
|
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 |
|
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 |
|
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.
|
|
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 |
|
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.
|
|
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.
|
|
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
|
|
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.
|
|
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. |
|
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).
|
|
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)
|
|
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 |
|
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
|
|