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  Laser Cooling Experiment 2021, all entries  Not logged in ELOG logo
ID Date Author Category Subject
  85   Tue May 31 07:29:11 2022 KenDetectorsXUV-Detektor
Rate was very low: ~ 100Hz
Adjusted Walk level and Threshold, new rate: 5kHz
Additionally, parameters of the detector were varied for optimization but were returned to default afterwards.
  84   Mon May 17 21:43:56 2021 DanyalGeneralThe test beamtime was a success.
Dear all,

The test beamtime is now over. 
We had 6 days of Li-like carbon in the ESR (122 MeV/u). 
Effectively, we could measure almost 5 days continuously.  

There were only a few interruptions, one of which was a longer power failure. 
The vacuum in the ESR was not optimal, which strongly reduced the lifetime of the stored ion beam (~30 s) 
and the electron cooler showed weird instabilities, which need to be clarified still. 

Still, we were able to cover all aspects of the program. 
Essentially everything we tried worked. 

Therefore, I conclude that it was a great success. 

Many thanks to all who have contributed to it! 
Special thanks to Sebastian and Benedikt - who worked really hard during the last months - for prepapring the laser system and the data acquisition system. 
Also special thanks to Volker and Ken for preparing the XUV detector system. 

We will start sorting/ordering & filtering the data soon and will invite for a meeting where we present the raw data so that we can discuss it. 
Then we will also discuss the next big step: data analysis. 
Of course it is our next objective (with high priority) to publish the analyzed data in foreseeable time. 

I hope to see you soon. 
Until then, take care and stay healthy,

Danyal 
  83   Mon May 17 08:05:42 2021 TeamGeneralEnd of beamtime
~ 8 a.m.
  82   Sun May 16 22:11:49 2021 TeamGeneralLaser Polarisation values
maximal transmission of PBSC (257/514 pbsc was used in combination with xlp12 detector and visual on a screen):

L/4 @ 276° & L/2 @ 348°                -->   p-polarized light


L/4 gleich auf 276° & L/2 auf ~19°     -->   s-polarized light
current position 22:15 p.m.

now we have some fun ! :D
  81   Sun May 16 21:23:02 2021 TeamGeneralESR OPEN -> preparation for Polarisation Tests
  80   Sun May 16 11:29:22 2021 BenediktGeneralAutomated laser scans working
The automated laser scans are working now.
We can now scan with the following functions: triangle, sawtooth, cosinus/sinus, arctan, min (linear scan, than stands still)

We are now testing these scan functions with coasting beams; ecooler 10 mA.
  79   Sun May 16 07:18:56 2021 Night Shift Sebastian/Max/NoahGeneralPreparation for automated laser scans
We shut the laser system down to prepare automated laser scans
  78   Sun May 16 07:03:07 2021 TeamGeneralLaser cooling with 166ps
We saw some indications of laser cooling @ 166ps pulse length
  77   Sun May 16 06:13:46 2021 TeamGeneralSwitch to 166ps
  76   Sun May 16 05:24:00 2021 TeamGeneralLaser cooling with 285ps
we also see laser cooling with 285ps pulse length
  75   Sun May 16 05:09:27 2021 TeamGeneralSwitch to 285ps
pulse length -> 285ps

minimum 62mW inside ESR (depending on laser wavelength)
  74   Sun May 16 05:09:04 2021 TeamGeneralLaser cooling with 482ps
we see laser cooling with 482ps pulse length
  73   Sun May 16 02:28:21 2021 TeamGeneral#Beam ON!
Laser specs:
pulse length -> 482ps

~75mW UV Power inside ESR (depending on laser wavelength)
  72   Sun May 16 02:22:19 2021 SebastianGeneral"Der Laser ist ok"
  Draft   Sun May 16 02:20:58 2021 SebastianGeneral"Der Laser ist (wieder) ok"
  70   Sun May 16 02:18:53 2021 SebastianGeneralUV Drop
1:25 a.m. huge drop in UV laser power
-> small crystal bump with both y screws of bbo oven
  69   Sat May 15 12:11:54 2021 BenediktGeneralLaser-bunch-timing
Optimizing the laser bunch timing.
h = 7 (9.0389145 MHz)
Reprate is already set to same frequency.


Results: For h=7:
4 ns delay results in a maximum fluorescence rate in the XUV detector
25 ns delay shows the highest intensity in the Schottky spectrum while the laser operates at 1028.940 nm.
  68   Sat May 15 11:26:44 2021 BenediktGeneralTEM parameters
We changed the horizontal position of the laser beam a bit, so that we maximized the fluorescence signal on the XUV detector (coasting beam, scanning laser (0.03 Hz)).

Old parameters: OffsetM Ax 0.00; Bx 0.00; Ay -0.08; By -0.40
New parameters: OffsetM Ax 0.00; Bx 0.35; Ay -0.08; By -0.40
  67   Sat May 15 11:06:31 2021 BenediktGeneralNew Zoom link for the moment
https://tu-darmstadt.zoom.us/j/4948400422?pwd=SEJaUzBuYXM0TTd6UWxoZTFlWEZxUT09

Meeting ID: 494 840 0422
Passcode:  215586
  66   Sat May 15 09:57:24 2021 DayshiftRunsCurrently on schedule
Enhance fluorescence rate and perform 
laser bunch timing 

Right now: Performing several detector tests with scanning laser (triangle) between 1028.930 and 1028.950 nm. Eccoler current @ 10 mA
  65   Sat May 15 09:50:31 2021 TeamRunsLaser cooling of....
H=2
H=7
H=10
H=20
H=30

We performed several scans:
Close to the bucket middle
Over the bucket
Over the bucket, jumped to the "red side" 
of the bucket and captured and cooled the 
beam again.

Laser settings:
7 times revolution frequency and 740ps 
pulses - - > 3.4 +/- 1.2 GHz

Still to do:
Switch to 240ps pulses - - > 5.8GHz 
+/-1.3 GHz

Maybe:
Switch to 117ps pulses - - > 11.0 +/- 0.8 GHz
BUT here we have less laser power (max. 50 mW right after BBO crystal, so maybe only 30 mW at the laser-ion overlap)
available. Maybe we are lucky and it is 
enough to cool also the ion beam. :) 
  64   Sat May 15 09:23:52 2021 SebastianAcceleratorEkühler
Tab "Kühler Elektronenstrahl"
An Gerät schicken
  63   Sat May 15 09:22:41 2021 Sebastian AcceleratorEkühler
Settings für Ekühler an und aus in SC4 und 
5
Attachment 1: IMG-20210515-WA0000.jpg
IMG-20210515-WA0000.jpg
Attachment 2: B5FE1031-7FFD-44D3-92B0-75E0784718D9.jpeg
B5FE1031-7FFD-44D3-92B0-75E0784718D9.jpeg
  62   Sat May 15 06:51:16 2021 Night Shift Sebastian/Max/NoahGeneralDifferent Laserscantypes
We use different scan types (manual scan) or constant laser wavelengths to check the effects of laser cooling in the Schottky diagrams (fluorescence can not be seen in the detector), for different bunching amplitudes and frequencies:
- Scan from 1028.950 -> 1028.940, stepsize 0.001 every 10 sec
- Scan from 1028.950 -> 1028.930, stepsize 0.001 every 5 sec
- Scan from 1028.950 -> 1028.940 -> 1029.950, stepsize 0.001 every 5 sec
- Scan from 1028.950 -> 1028.940, stepsize 0.0005 "as fast as possible" 
- constant wavelengths around 1028.940
- Scan to wavelengths < 1028.940 (heating) -> Jump to 1028.945 and fast scan back to 1028.940 (-> cooling)

The cooling effects of the laser can be observed well in the Schottky spectra :)
  61   Sat May 15 03:39:16 2021 TeamGeneralactual revolution frequency
frev = 1,2912735 MHz
  60   Fri May 14 22:20:37 2021 TeamAcceleratorESR Closed - BEAM #ON!
  59   Fri May 14 22:04:25 2021 TeamAcceleratorESR OPEN ; NO BEAM -> Reset cooling device
we had to open the ESR to reset a cooling device
  58   Fri May 14 21:43:40 2021 SebastianGeneral"problems accelerator"
There are cooling problems of some accelerator devices
short break, hopefully :)
Laser is switched of for some rest
  57   Fri May 14 16:37:01 2021 BenediktGeneralStatus update
Right now, we have to adjust the ion beam a bit to overlap better with the laser beam.
We keep the laser wavelength at resonance with the ions and try to optimize the fluorescence signal on the XUV detector while moving the ion beam.
  56   Fri May 14 11:01:33 2021 BenediktCalibrationLaser Beam adjusted
The laser beam was adjusted in his position to overlap better with the ions.

Ion beam is destroyed at scraper position 1VO 6 mm and 2VO 4 mm; the laser beam looses half its power at 1VO 6mm and 2VO 4 mm.

EDIT: In the Schottky spectrum, we saw a stronger "cut" from the laser beam with slightly different settings in the TEM system. Later today, we could maybe finetune the ion-laser overlap while observing this "cut".
  55   Fri May 14 09:40:04 2021 NightshiftRunsEcooling vs laser wavelength shift, coasting beam, laser stronger than Ecooling
Last three pictures where taken after 
first laser ion beam overlap adjustments

It seems to be that the interactions are 
better. We also see the laser earlier and 
stronger in the schottky 
Attachment 1: IMG-20210514-WA0017.jpg
IMG-20210514-WA0017.jpg
  54   Fri May 14 09:38:43 2021 NightshiftRunsCoasting beam, ecooler on, scanning laser
Attachment 1: IMG-20210514-WA0019.jpg
IMG-20210514-WA0019.jpg
  53   Fri May 14 09:38:04 2021 NightshiftRunsCoasting beam, scanning laser, ecooler on
Attachment 1: IMG-20210514-WA0018.jpg
IMG-20210514-WA0018.jpg
  Draft   Fri May 14 09:35:20 2021 NightshiftRunsCoasting beam, scanning laser, ecooler on
Attachment 1: IMG-20210514-WA0018.jpg
IMG-20210514-WA0018.jpg
  51   Fri May 14 09:00:55 2021 SebastianGeneralUNILAC Problems
~30 min downtime

--> LASER ADJUSTEMENTS!
  50   Fri May 14 08:55:53 2021 SebastianGeneralToDO 14.5 ...so far
1.) ion lasser overlap and scraper test

2.) change bunching frequency to middle of ecooled coasting beam

3.) long time measurements see labbook HKR
3.1) try ecooler on/off ; bunch on / off ; laser fixed on / off ; laser scanning on / off ; try different bunching amplitudes (MAX :LEV 0.25V) ; try other h = 10, 7, etc...
3.2) Dont forget to plug in the schottky trigger -> maybe change acquisition and analysis time if needed

4.) XUV detector tests
4.1.) laser - bunch timing by checking xuv anode signal
  Draft   Fri May 14 07:33:42 2021 Team #NightGeneralecooler central frequency shifted relative to bunch central frequency
  48   Fri May 14 07:20:18 2021 Team #NightGeneralactual bunching frequency
25,82556 MHz
h = 20
  47   Fri May 14 06:35:55 2021 Team #NightGeneralAdjustment of Laser
we increased the height of the laser beam

TEM Settings
OffsM Ay -0,07
OffsM By -0,35

1VO scratches 6
2VO scratches 3-4
  46   Fri May 14 06:34:45 2021 Team #NightAnalysisDSG821 IP
140.181.104.108
  45   Fri May 14 04:50:46 2021 Team #NightGeneralScraper Tests Ion / Laser Beam
laser is 4-6mm below the ion beam.
It could be that the interaction between both beams came only from the interaction between the laser halo with the ion beam ?!
  44   Fri May 14 01:34:44 2021 TeamGeneralstrange XUV Anode signal
We see a strange behavior of the anode signal when we bunch the ion beam and electron cooler is on.

peak structure... ---> we play now with the bunching amplitude 

200mV
150mV
100mV ---> Peaks higher?

see attached file
Attachment 1: Screenshot_(68).png
Screenshot_(68).png
  43   Fri May 14 01:28:04 2021 SebastianGeneral"new" laser wavelength
Minor changes in electron cooler voltage (~+13V, now 66903V measured by DMM) leads to that we had to shift the laser wavelength to:

1028,965nm 

to see an increase of the countrate of the XUV ANODE Signal.

electron cooler ON
electron cooler current (SET 120mA, HKR "measured" 102mA)
bunched beam, h=20
  42   Thu May 13 23:42:37 2021 Ken UeberholzGeneralWhat was done
In this shift a number of successful Schottky measurements were done:
With fixed laser wavelength, while varying the wavelength, with different bunching and more (see logfile 1 for more info: line 53 to at least 107).
The detector software sometimes files to change the current of the power supplies, if this happens a simple restart of the GUI fixes the problem.
Once in this shift the Mesytek in the laser lab turned itself (?) off and the background rate increased. Hopefully this was a single event.
Attachment 1: Schottky1.jpeg
Schottky1.jpeg
Attachment 2: Schottky2.jpeg
Schottky2.jpeg
Attachment 3: Schottky3.jpeg
Schottky3.jpeg
Attachment 4: Schottky4.jpeg
Schottky4.jpeg
  41   Thu May 13 21:00:48 2021 BenediktGeneralNew reprate of the UV laser
The lasersystem now operates at a reparte of 9.038946 MHz. This is 7 times f_rev (see previous post).

In the future, the laser-bunch-timing can be adjusted.
  40   Thu May 13 20:18:10 2021 BenediktGeneralNew f_rev
The ions were changed to a different speed today at 2 PM. The new revolution frequency is now 1.291278 MHz.
  39   Thu May 13 18:34:54 2021 Ken UeberholzGeneralWhat happened scince shift change at 4pm
Ion frequency shifts with laser, both manually and scanned, without bunches: successful
Bunching with 7 and 20 bunches: successful
Tried laser scans with bunches: unsuccessful
Manual laser scans with bunches: successful
  38   Thu May 13 03:35:25 2021 LarsGeneralStatus: Current schedule ... so far
1.) so far: 
h = 2, 4, 6, 7, 8, 10, 12, 14, 16, 18, 20, 30
Amplitudes: (10, 50, 100, 150, 200, 250) mV

now we will try to use the laser-toy ;-)


> 1.) check h=2,4,6,7,8,10 .... bunching frequencies with different amplitudes (signalgenerator), Ecooler ON, Laser OFF --> record schottky and "normal" DAQ
> 
> 2.) Ecooler ON, Bunching ON, Laser ON (wavelength fixed and/or scanned)
> 
> 2.1) Do we see the laser in the Schottky? (The laser has to be on the right side of the bunches and act as a barrier to damp the oscillation of the ions inside the buckets.) 
> If not change laser wavelength until we see the laser in the schottky 
> 
> 2.2) Do we see fluorescence in the XUV Detector signal? Weak fluorescence signal --> check laser-bunch timing by varying the lead delay until we see the highest fluorescence signal. 
> If we see no fluorescence signal change laser wavelength until we see fluorescence from the xuv anode signal.
> 
> 3.) Do we see that some sidebands vanish in the schottky? Does the lifetime of the ion beam increase?
> 3.1.) If not "play" with Laserparameters, scans, delays, etc...
  37   Thu May 13 02:45:29 2021 SebastianAnalysisESR pressure
Attachment 1: IMG_20210513_014506_resized_20210513_024017156.jpg
IMG_20210513_014506_resized_20210513_024017156.jpg
Attachment 2: IMG_20210513_014518_resized_20210513_024017559.jpg
IMG_20210513_014518_resized_20210513_024017559.jpg
Attachment 3: IMG_20210513_014524_resized_20210513_024017847.jpg
IMG_20210513_014524_resized_20210513_024017847.jpg
Attachment 4: IMG_20210513_014606_1_resized_20210513_024018452.jpg
IMG_20210513_014606_1_resized_20210513_024018452.jpg
Attachment 5: IMG_20210513_014606_resized_20210513_024018145.jpg
IMG_20210513_014606_resized_20210513_024018145.jpg
Attachment 6: IMG_20210513_014627_resized_20210513_024018757.jpg
IMG_20210513_014627_resized_20210513_024018757.jpg
Attachment 7: IMG_20210513_014636_resized_20210513_024019062.jpg
IMG_20210513_014636_resized_20210513_024019062.jpg
Attachment 8: IMG_20210513_014700_resized_20210513_024019366.jpg
IMG_20210513_014700_resized_20210513_024019366.jpg
  36   Thu May 13 02:42:58 2021 SebastianGeneralLasershutter ESR Entrance?!
attached should be the name of the entrance laser shutter. just in case somebody will close it ;)
Attachment 1: IMG_20210513_020027_resized_20210513_024049198.jpg
IMG_20210513_020027_resized_20210513_024049198.jpg
  35   Thu May 13 01:55:15 2021 SebastianGeneralESR amplifier reset / laser check
we had to go into the ESR because the amplifiers hooked up. both amplifiers were resetted!

we also checked why we didnt see the laser at the exit window.
Laser Shutter @ the exit is closed......................... E02VVLF2t needs to be opened!
Attachment 1: IMG_20210513_014345_resized_20210513_015540959.jpg
IMG_20210513_014345_resized_20210513_015540959.jpg
Attachment 2: IMG_20210513_014353_resized_20210513_015541291.jpg
IMG_20210513_014353_resized_20210513_015541291.jpg
  34   Thu May 13 01:21:30 2021 SebastianGeneralCurrent schedule ... so far
1.) check h=2,4,6,7,8,10 .... bunching frequencies with different amplitudes (signalgenerator), Ecooler ON, Laser OFF --> record schottky and "normal" DAQ

2.) Ecooler ON, Bunching ON, Laser ON (wavelength fixed and/or scanned)

2.1) Do we see the laser in the Schottky? (The laser has to be on the right side of the bunches and act as a barrier to damp the oscillation of the ions inside the buckets.) 
If not change laser wavelength until we see the laser in the schottky 

2.2) Do we see fluorescence in the XUV Detector signal? Weak fluorescence signal --> check laser-bunch timing by varying the lead delay until we see the highest fluorescence signal. 
If we see no fluorescence signal change laser wavelength until we see fluorescence from the xuv anode signal.

3.) Do we see that some sidebands vanish in the schottky? Does the lifetime of the ion beam increase?
3.1.) If not "play" with Laserparameters, scans, delays, etc...
  33   Thu May 13 01:13:06 2021 SebastianGeneralBunching frequencies
relating to Danyals ID 25 post are the current bunching frequencies:

h=2      -->     2,5823668 MHz
h=4      -->     5,1647336 MHz
h=6      -->     7,7471004 MHz
h=7      -->     9,0382838 MHz
h=8      -->     10,3294672 MHz
h=10     -->     12,911834 MHz
h=12     -->     15,4942008 MHz
h=14     -->     18,0765676 MHz
h=16     -->     20,6589344 MHz
h=18     -->     23,2413012 MHz
h=20     -->     25,823668 MHz
h=30     -->     38,735502 MHz
  32   Thu May 13 01:05:45 2021 DanyalDAQmore stability by bunching
Because the C3+ part of the ion beam is properly bunched, it is no longer so sensitive to the drifts caused by the e-cooler. 
In the O4+ part of the ion beam these drifts can still be seen. 
  31   Thu May 13 01:01:27 2021 DanyalDAQbunched ion beam
Attachment 1: bunched_-_signal.jpg
bunched_-_signal.jpg
Attachment 2: bunched_-_Schottky.jpg
bunched_-_Schottky.jpg
Attachment 3: zoom_bunched_-_Schottky.jpg
zoom_bunched_-_Schottky.jpg
  30   Thu May 13 00:58:53 2021 DanyalDAQunbunched ion beam
Attachment 1: not_bunched_-_signal.jpg
not_bunched_-_signal.jpg
Attachment 2: not_bunched_-_Schottky.jpg
not_bunched_-_Schottky.jpg
  29   Wed May 12 23:45:23 2021 Ken UeberholzGeneralLaser does not reach the exit window
High rates on the detector at 50mm positions, laser does not seem to reach the exit window.
  28   Wed May 12 23:36:18 2021 Ken UeberholzDAQVI change
carbon main vi - kopie is now in operation

here, in keysight.vi the input settings for the new impedence for the multimeter are now hopefully correct --> THIS SHOULD BE CHECKED IF THE RING IS OPEN 
  27   Wed May 12 22:57:41 2021 SebastianGeneralLaser Reprate
laser reprate is seven times the revoolution frequency: 9.038283 MHz
pulse length: 735ps
  26   Wed May 12 22:48:25 2021 SebastianGeneralDSG Control SCPI Commands
Open Ultra Sigma
Press LAN
Press Search, after a while the whole rigol devices are shown. Press ok
Than you see the DSG821 (140.181.104.108) as online
right click -> open SCPI Command Terminal


*IDN?                 check for remote control
:FREQ 1.291MHz        set the RF Frequency to 1.291MHz
:FREQ?                return current frequency
:LEV 0.2V             set the amplitude to 200mV
:LEV?                 return current amplitude
:OUTP ON / OFF        set RF output ON or OFF
:OUTP?                returns 0 if output is OFF, returns 1 if output is ON

after some time there is an automatic logout of the scpi command panel. Close the panel and reopen the SCPI Command Terminal again to reconnect to DSG821 Signalgenerator. 
If this does not work, close the whole ultra sigma program, also in the taskbar (right click -> exit) and execute Ultra Sigma Program again
  25   Wed May 12 22:35:33 2021 DanyalGeneralfrev and fb
Schottky frequency (189th harmonic) = 244.033662 MHz

revolution frequency  frev = 1.2911834 MHz

bunching frequency h=2  --> fb = 2.582367 MHz
bunching frequency h=10  --> fb = 12.911834 MHz
  24   Wed May 12 22:28:55 2021 Ken UeberholzGeneralBunching succesfull
Bunching with 2 and 10 bunches succesfull
  23   Wed May 12 19:48:24 2021 SebastianGeneralDSG821 Network
To implement the bunch Signal Generator (DSG821 inside ESR) you have to:

1. unplug the Ethernet cable
2. under System / io config set the ip address
3. set Sub mask
4. set DNS
5. very important: than press Apply!
6. plug in Ethernet cable
7. than a message like "successfully connected to network" should show up
8. you can crosscheck the Settings by pressing the "eye symbol"
Attachment 1: IMG_20210512_195329_resized_20210512_075346417.jpg
IMG_20210512_195329_resized_20210512_075346417.jpg
  22   Wed May 12 18:59:15 2021 Ken UeberholzGeneralPower is back
Power is back and most things are running again
  21   Wed May 12 15:36:04 2021 DanyalAcceleratorgeneral power failure in ESR! (everything is off)
The power in the ESR is off. 
(also on the gas-target area on top of ESR)
Electrical engineers are trying to find and fix the problem. 
  20   Wed May 12 13:11:58 2021 DanyalAcceleratorshort break between 13:30 and 15:30
There will be a short break (2 hours) this afternoon. Between 13:30 and 15:30. 
The so-calles "super lense" in the UNILAC needs to be cleaned (rinsed). 
After that operation should continue as usual. 
  19   Wed May 12 10:15:47 2021 Volker HannenDAQUnplugged TDC inputs for MCP front and back
To reduce the load on the VUPROM TDC, we unplugged the TDC inputs for the front and back signals of the MCP of the XUV detector.
The Anode signal is still plugged in and should be sufficient for the analysis.
  18   Wed May 12 10:14:18 2021 LarsAcceleratorE-Cooler
M.Steck et al. discussed about the E-Cooler and found a possible issue. They asked for enterance to the ESR. Since nobody else was in the HKR and anyway nothing was running because of some other issues, I told, the experiment would not be disturbed and they could enter and do things. (Sth. like putting some repeller electrodes onto hand and other magical things).
It should take about 10 Minutes and might be already finished by now.
  17   Wed May 12 09:59:08 2021 BenediktGeneralRigol DSG821 signal generator settings
Attachment 1: CF7701F6-86BE-406C-8FAD-F3161463181C.jpeg
CF7701F6-86BE-406C-8FAD-F3161463181C.jpeg
  16   Wed May 12 09:09:15 2021 SebastianDAQFluorescence
fluorescence with detector in parking position
fixed laser wavelength
electron cooling ON, 
BUT we saw strange drifts in the Schottky spectra. It seems to be that these drifts come from the electron cooler! are the drift tubes grounded?

the drifts shift the ion beam over the transition which result in an increase of the XUV anode signal
Attachment 1: 1029967nm.png
1029967nm.png
  Draft   Wed May 12 09:05:48 2021 Keysight SettingsDAQ 
  14   Wed May 12 09:04:48 2021 SebastianDAQKeysight AUtoCal
Attachment 1: IMG_20210510_143940_resized_20210512_090353546.jpg
IMG_20210510_143940_resized_20210512_090353546.jpg
  13   Wed May 12 08:42:49 2021 SebastianAnalysisLaser scans / coastig beam / no ecooler
Attached you'll see a first laser scan of ~100GHz in the UV.
Attachment 1: Screenshot_(156).png
Screenshot_(156).png
  12   Wed May 12 08:41:36 2021 SebastianAnalysisLaser stability
During night shift the laser was very stable! Only minor fluctuations occured in the UV
  11   Wed May 12 08:32:04 2021 SebastianAnalysisfluorescence & energetic overlap
During the night shift we saw several rises of the fluorescence (see another entry) and also energetic overlap in coasting beam modus.
Here the laser wavelength was stabilized @ 1028,967nm and electron cooler was switched off because of some fluctuations which we saw in the schottky.
Left part of the schottky picture shows the c3+ beam, the right part is the o4+ contamination.
Attachment 1: Screenshot_(154).png
Screenshot_(154).png
  10   Wed May 12 08:10:17 2021 LarsGeneralinstabilities in ion frequency
looks like the E-Cooler is responsible for this. If one turns off the electron current, the beam stays stable. 
M.Steck is informed.

> The ion beam moves around, pretty arbitrary. See picture. 
> ESR crew believes that it is not due to fluctuations in the HV of the E-Cooler. 
  8   Wed May 12 02:34:29 2021 DanyalGeneralinstabilities in ion frequency
The ion beam moves around, pretty arbitrary. See picture. 
ESR crew believes that it is not due to fluctuations in the HV of the E-Cooler. 
Attachment 1: fluctuations.jpg
fluctuations.jpg
  Draft   Wed May 12 02:16:25 2021 Danyal, LarsAcceleratorIon beam position
Laser Position with scrapers verified. 
1HA: impossible to scratch laser beam, still there at -1.0 mm
2HA: +3mm --> half the laser power on detector; +4.5mm --> gone

2VO: interlock, impossible to move (beam diagnostics is informed and will check)
1VO: +0.2mm --> half laser power, +1.2: laser gone (-1.0mm: also gone)

Ion beam adapted to measured laser beam, Target bump position: -22mm (was -18mm before)
Ion beam position verified with scrapers:
1HA: -1.0mm --> still there
2HA: +4.0mm --> beam gone
Target bump angle: unchanged (+1.2 mrad)
  6   Tue May 11 20:14:43 2021 DanyalGeneralbad ESR vacuum
I just heard that the ESR vacuum is quite bad. 
There was a small vacuum problem a while ago, it was sealed, but apparently the pressure is not as low as usual.

Markus Steck said that the beam lifetime is only 15 - 20 seconds !!! 

This will seriously complicate some of our test experiments :( 
  5   Tue May 11 18:29:35 2021 DanyalGeneralfirst ions in the ESR
Attachment 1: first_ions_are_injected.jpg
first_ions_are_injected.jpg
  4   Tue May 11 16:33:31 2021 Ken UeberholzDetectorsDetector control manual
Attached to this elog entry is a short manual for the xuv-detector control. If anything is missing or not understandable I can change anything.
Attachment 1: Manual.pdf
Manual.pdf Manual.pdf Manual.pdf Manual.pdf
  3   Tue May 11 16:07:59 2021 SebastianDAQDAQ Manual
Attached you'll find a short manual for operating the whole DAQ system
Attachment 1: DAQ_Manual.pdf
DAQ_Manual.pdf DAQ_Manual.pdf DAQ_Manual.pdf
  2   Tue May 11 15:49:30 2021 DanyalGeneralsetting up ESR
The operators are still busy extracting the beam from the SIS18 towards the ESR and injecting it into the ESR. 
  1   Mon May 10 07:58:13 2021 DanyalGeneralTelephone numbers and Zoom link
Telephone numbers:

ESR laser lab: +49 (0)6159 71 - 2882
ESR measurement hut: +49 (0)6159 71 - 2880
HKR (main control room): +49 (0)6159 71 - 2317 or 2245

here is the zoom information:

https://tu-darmstadt.zoom.us/j/2183997317?pwd=WGc2TEkxYlEyNFhMWm02bFhqRnRVUT09

Meeting-ID: 218 399 7317
Passwort: 481607
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