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  Richardson Lab Experimental Log, Page 2 of 12  Not logged in ELOG logo
Entry  Thu May 15 12:03:41 2025, Xuesi Ma, Infrastructure, Electronics, Notice 

All Sorensen power supplies are turned off. The Cymac system is down (All Chassis are down)

If you need more information or if you need to turn them back on please contact Xuesi Ma.

Entry  Tue May 13 12:41:06 2025, Tyler, Update, TCS, A# Profiles Update 
Slides on the A# ITM FROSTI profile modeling efforts can be found here.
Entry  Tue May 13 12:35:01 2025, Xuesi Ma, Update, ,  resistance_vs_voltage_all.pdfresistance_vs_voltage_overlay.pdfresistance_vs_time_all_channels_all_time_RV.pdf
 
Entry  Sun May 11 19:36:42 2025, Luke , Update, Scripts/Programs, New optimization plots 

Slides

I have re-run the optimization plots with the changes mentioned last week. 

I have added the heat maps of the HOM scattering from HR deformation and the HOM scattering due to the OPD difference as well as the curvature actuation of the surface. 

Entry  Fri May 9 20:06:27 2025, Luke , Summary, Cleanroom, Cleanroom cleaning 20250509_particalcount.png

[Luke, Mohak, Luis]

We were also able to remove the residue that has built up on the soft walls by donning a skinny bunny suit and with two wipes rubbing both sides of the soft walls at the same time. The wipes would get gummy very quickly and need to be replaced frequently.

Particle Count Measurements:

  • Pre-cleaning (1:20 pm):
    • Zone 3:
      • 0.3 µm: 3577
      • 0.5 µm: 1369
      • 1.0 µm: 485
    • Zone 4:
      • 0.3 µm: 1062
      • 0.5 µm: 442
      • 1.0 µm: 177
  • Started Cleaning (3:00 pm)
  • Finished Cleaning (4:00 pm)
  • Post-cleaning (4:22 pm):
    • Zone 3:
      • 0.3 µm: 3577
      • 0.5 µm: 618
      • 1.0 µm: 132
    • Zone 4:
      • 0.3 µm: 2031
      • 0.5 µm: 397
      • 1.0 µm: 132

 

Entry  Thu May 8 17:41:56 2025, Luis, Update, VAC, RGA Scan Post Bake  2025-4-29_HeaterElement-Bake1_ArO_overlay.png2025-4-29_HeaterElement-Bake1_ArO_overlayNormalized.png

[Ma, Luis]

After taking the RGA scans of the new system, here are the results of the raw and normalized data.We can see that in the post baked system the He peak is way lower, and the peaks around 20AMU are also significantly lower.

Entry  Tue May 6 13:19:31 2025, Xuesi Ma, Update, ,  resistance_vs_time_RV_rise_time_24.pdfresistance_vs_time_all_channels_all_time_RV.pdf
 
Entry  Tue May 6 13:07:34 2025, Michael, Update, Interferometer Simulations, Initial Convergence Plots for Toroidal Mirrors Project Convergence_Plots_5_6_25.pdfConvergence_Plots_5_6_25-1.pdfaperture_num_points_convergence.png
 
Entry  Tue May 6 12:25:03 2025, Tyler, Configuration, CDS, Cymac ADC CSD measurement cymac_adc_rin_v1.pdf
An initial measurement of the cymbal ADC CSD is attached below. As of now, it seems that the sensitivity limit is roughly the same as that of the Red Pitaya.
Entry  Sun May 4 18:17:45 2025, Luke , Update, Scripts/Programs, Ringheater modeling Update 

Slides

I have changed some properties of the thermal model and am re-running the thermal sweeping

I have also been messing around with making a logo

Entry  Fri May 2 12:34:02 2025, Xuesi Ma, Update, VAC, Stopped bake 

The vacuum chamber has stopped baking. 

Current state as of 12:30, 5/2/2025:

The gate valve is open, and the filament of the RGA is on.

The temperatures were steady at:

PID right: barrel upper: 108°C,  RGA volume: 120°C

PID left: barrel lower: 120°C, Lid: 91°C

Entry  Wed Apr 30 17:33:14 2025, Xuesi Ma, Update, VAC, Started bake 

[Luke, Ma, Tyler]

The vacuum chamber is currently baking. 

Current state as of 5:00

The gate valve is open, and the filament of the RGA is on. Argon leak is opened

The temperatures are as follows:

PID right barrel upper: 99°C,  RGA volume: 120°C

PID left barrel lower: 123°C, Lid: 92°C

Entry  Wed Apr 30 15:43:56 2025, Luis, Update, VAC, Vacuum Update 2025-4-29_HeaterElement-Bake1_ArO.png2025-2-24_HeaterElement_ArO.png

[Ma, Luke, Luis]

April 29, 2025

3:30 PM
We performed another leak test on the vacuum system, this time focusing on the welds around the main cylinder. The leaks from these junctions were in the mid 10⁻¹¹ range, but we noticed some strange behavior after completing the test. The partial pressure of He kept rising at a slow, constant rate for a while—even after stopping the test for about 15–20 minutes and restarting the measurement. We're not sure what’s causing this and wanted to check in before moving forward with the bake.

4:30 PM
We performed an RGA of the system (see below) and the findings are that there was a higher contraction of He than usual. We have attached another scan from 2/24/25 for reference.

5:00 PM
We turned off the electron multiplier and closed the RGA Program.

Entry  Wed Apr 30 13:42:45 2025, Shane, Update, CDS, UPS comms successful 
Update on UPS1 serial interfacing: communication is now successful. On 4/15/25 we connected to UPS1 via ethernet rather than USB, and manually added its static ip address (noted in lab network wiki) to the router. Able to connect and unpack all desired data nicely using telnet server connection via telnetlib. In process of finalizing code and will work next on interfacing UPS2.
Entry  Tue Apr 29 10:59:25 2025, Liu, Update, Interferometer Simulations, Test Mass Thermal State Decoder with Updated Comparison Cases  Update.pdf
 
Entry  Mon Apr 28 22:08:28 2025, Luis, Update, VAC, Vacuum Leak Test result 

[Ma, Luke, Luis]

April 24, 2025

3:00 PM
Ma and Luis attempted to connect to the RGA to initialize the leak test but encountered some difficulties.

3:20 PM
After restarting both the computer and the RGA, we realized that the DB9 cable was not connected to Spica. After connecting it, we had no further issues communicating with the RGA.

3:30 PM
Luke and Luis performed the leak test. There were no significant leaks in the vacuum system. The highest leak rates we found are listed in the table below; the rest of the entries were limited by noise, as we could not detect any change in the program after spraying the ports with He.

Connection Leak rate (torr)
ZLR(2.75"-4.5") - Reducing Cross 6.0e-12
Cross - Turbo Pump (small) 1.4e-11
Port - Pressure Sensor 8.0e-12
Entry  Fri Apr 25 19:18:10 2025, Luke , Update, Scripts/Programs, New optimization plots effective_power.pngproximity.png

I have created two more plots. One on the transmitted power for a specific configuration. This was done by taking the product of the efficiency and the power released by surface area of the source plane for a configuration assuming it is at 300C. The second is a plot of how close the reflector is to the test mass I have included a contour line at 2mm the nominal proximity constraint. Both of these plots are generated for a 2cm wide target plane.

Somethings of note: Because the proximity requires no modeling and can be determined purely mathematically it is easy to re-generate this plot of other target widths. If you increase the target width the proximity contour moves upward and downwards if reduced.

Entry  Fri Apr 25 09:09:03 2025, Luke , Update, Scripts/Programs, Update to optimization plots HOM_scattering_100kg_modified.pngcurvature_100kg.pnginitial_contour_plot_with_hom_and_curvature.pngtemp_quality_(log10_ratio).png
I have calculated the curvature of the surface plots and created a heat map out of the data. I have also created a contour plot of them together. It is very rough and the artifacts at small w make it hard to read. I am planning on excluding that data and replot them. In the meantime I have created a temporary function that balance the two values. (log_10(curvature/HOMscattering))
Entry  Tue Apr 22 13:00:04 2025, Nathan, Update, VLC Update, Photodiode signal check and additional signal check due to 20Mhz signal and amplifier thumbnail_(8)_(1).jpgvpp.jpg
In general, photodiode was able to achieve signal. Below are the voltage signals and frequency measurements of the photodiode with the dc bias and amplifier connected to the EOM (Vpp = 2mV for first and Vpp= 1 for second). Also I need assistance in using the PZT driver.
Entry  Tue Apr 22 12:08:46 2025, Xuesi Ma, Update, ,  20250415_161755.jpg20250416_174640.jpg20250422_105614.jpg

Test 7: Reconnect ribbon cables

  • Setup: Reconnect all the ribbon cables, and turned on the AI Chassis while isolated rack
  • Observation: No spike observed.

Test 8: Reconnect to rack

  • Setup: Reconnect the AI Chassis to the rack.
  • Observation: No spike observed.

Test 9: Restore to original position.

  • Setup: CLose up the AI Chassis, and put it back to its original location.
  • Observation: No spike observed.
Entry  Tue Apr 22 11:04:31 2025, Liu, Update, Interferometer Simulations, Test Mass Thermal State Decoder Update with Interferometer Operation Update.pdf
 
Entry  Tue Apr 22 08:00:39 2025, Luke , Update, Scripts/Programs, Thermal optimization modeling 40kg 40kg_into_HOM.png

I have redone the width and location optimization with a 40kg test mass. This was to see where the nominal ring heater would fall in this optimization map see attached.

There are two concerns I have with this modeling:

  1. I am using normalized power only imparting 1W, which may effect the single pass scattering used for optimization.
  2. I am only looking at the surface deformation and I believe that looking at OPD may also be something that is important to consider. 

Note z_RH is measured from the HR surface and w_RH is the half width of the target plane

Entry  Mon Apr 21 16:56:42 2025, Michael, Update, Interferometer Simulations, Fixed Observed Squeezing Curve for Toroidal Mirror Case updated_observed_squeezing_plot.png
We've resolved the issue with the observed squeezing curve for the toroidal mirror case showing worse performance at lower frequencies and better performance at higher frequencies compared to the nominal case. This issue was caused by the beam parameter at the squeezer being fixed before changing the radii of curvature of the mirrors. This has been changed to be fixed after changing the mirrors, and we see an improvement in the toroidal mirror case.
Entry  Thu Apr 17 12:12:29 2025, Liu, HowTo, Interferometer Simulations, Preventing Thread Contention in Multiprocessing with Finesse and Cython 

Avoiding Thread Contention When Using Multiprocessing with Finesse and Cython

When running Monte Carlo simulations or other computational workloads, it's common to use Python's ProcessPoolExecutor to parallelize multiple independent tasks. This approach works well—until it interacts with low-level libraries that themselves use multi-threading under the hood.

The Problem: Thread Over-Subscription

In a recent project, I ran into a significant performance issue while executing a large number of Monte Carlo trials using a process pool with 30 worker processes on Megatron (with 48 cores). Each trial ran a function that internally used cython.parallel.prange for fast, element-wise operations, which is what Finesse uses under the hood for many internal numerical calculations. Cython, via OpenMP, was configured to use all available CPU threads per process by default.

This resulted in severe thread over-subscription. With 30 parallel processes and each process attempting to use all 48 threads, the system was launching over 1,400 threads concurrently. The CPU quickly became saturated, and the tasks stalled. In some cases, the system became unresponsive, and the jobs had to be canceled repeatedly.

This happens because when the function calls into these libraries from within a Python multiprocessing context, each subprocess will attempt to use the full number of threads available to the machine.

The Solution: Limit Threads per Process

The solution is simple: explicitly limit the number of threads each subprocess is allowed to use. This can be done by setting the environment variable at the top of your script, before importing any thread-hungry libraries like Finesse.

      
import os
os.environ["OMP_NUM_THREADS"] = "1"

    

By setting OMP_NUM_THREADS to "1", we ensure that each multiprocessing worker uses only one thread internally, preventing them from overloading the system and allowing the tasks to run more efficiently.

Entry  Tue Apr 15 11:37:17 2025, Cynthia, Update, Interferometer Simulations, Finishing up mirror coating map step updates_4_15_2025.pdf
 
Entry  Tue Apr 15 11:13:43 2025, Xuesi Ma, Update, ,  20250414_120428.jpg20250414_120423.jpg20250411_163105.jpg

Test 4: AI Chassis ground isolation

  • Setup: AI Chassis isolated from the ground with readout directly connected to adapter board
  • Observation: No spike observed.

Test 5: Ribbon cable check

  • Setup: AI Chassis remains isolated from the ground. The signal is measured after the ribbon cable. (Attachment 3)
  • Observation: No spike observed.

Test 6: Single ground connection check

  • Setup: AI chassis powered on but remains isolated from the frame. The signal is measured from the output of the AI Chassis. (Attachment 1 ,2)
  • Observation: No spike observed.
Entry  Tue Apr 15 11:09:37 2025, Liu, Update, FLIR, Test Mass Thermal State Decoder Update with robustness study Update.pdfUpdate.pdf
 
Entry  Tue Apr 8 20:04:35 2025, Nathan, Update, VLC Update, PDH Lock Progress IMG_5450.jpegIMG_5449.jpeg
Connected the DC bias and mixer. Need to connect signal generator now to RF Amp and mixer, and also need to connect power supply. After that will see if I can get a detection on the oscilloscope and if so will set up the driver. [Photos attached]
Entry  Tue Apr 8 12:15:59 2025, Luke , Update, Scripts/Programs, Updated optimization plot HOM_scattering_w__nominal_and_min.png
 
Entry  Tue Apr 8 10:47:10 2025, Liu, Update, General, Test Mass Thermal State Decoder Update Update.pdf
 
Entry  Tue Apr 8 00:17:01 2025, Michael, Update, Interferometer Simulations, Squeezing Performance Graphs for Case With and Without Toroidal Mirrors in LIGO 
I've created some graphs for the frequency dependent observed squeezing level in LIGO for both the nominal case and the case where we include toroidal mirrors, giving some interesting results. https://docs.google.com/presentation/d/1RBr47hNaxFTdGrwys5ZCUEUOgVOVHmZ2B_5EQwY62IY/edit?usp=sharing
Entry  Mon Apr 7 13:28:49 2025, Xuesi Ma, Update, ,  20250403_151946.jpgELOG_Spike_adapter_filter_on.png20250404_143624.jpgELOG_Spike_adapter_isolate.png20250407_105846.jpg

Test 1: Adapter Board Connected to Filter Board

  • Setup: AI Chassis is powered on. Signal is measured directly from the adapter board. All other ports on the adapter board are connected to the filter board.
  • Observation: Two distinct spikes observed at the beginning of the measurement.

Test 2: Adapter Board Disconnected from Filter Board

  • Setup: AI Chassis remains powered on. Signal is again measured directly from the adapter board. This time, the remaining ports on the adapter board are not connected to the filter board.
  • Observation: Multiple spikes observed, distributed evenly across the entire measurement.

Test 3: Isolation Test with Spare Adapter Board (ongoing)

  • Setup: Suspecting the original adapter board may be faulty, a spare adapter board is used for comparison. Signal is measured directly from this spare board.

Update, 04/08/25, Tue 17:30

Took the old adapter board out of the AI chassis and and used it to connect DAC to AA chassis. If no spikes are seen, it means that the glitches are not originating from this board.

Also checked al the previous spikes using the raw data (65536 Hz sample rate). The duration of the glitches are ~1 second, despite the previous guess that they are happening in the Milli-second scale.

Entry  Thu Apr 3 13:23:37 2025, shane, Update, CDS, UPS interfacing 
Update on UPS serial interfacing: the driver for the UPS webcard has been installed on spica (for UPS1 in room 1119) and logrus (for UPS2 in room 1129). Static IP addresses have been assigned for both and noted on the lab wiki. Neither is yet able to connect, as the initial ip address webpage connection test failed for both. In the process of troubleshooting now.
Entry  Tue Apr 1 11:47:08 2025, Liu, Update, ,  Thermal_state_decoder_update.pdf
 
Entry  Mon Mar 31 15:41:56 2025, Xuesi Ma, Update, ,  

The result from AI Chassis bypass test showed that the AI Chassis may be the problem. There are no spikes from DAC's direct output.

All chassis except timing chassis are turned off. Power supplies for 24V, 18V, and -18V are turned off

The AI chassis has been taken out of the rack for further inspection

Refer to:

https://dcc.ligo.org/LIGO-E2300117

https://dcc.ligo.org/cgi-bin/private/DocDB/ShowDocument?.submit=Identifier&docid=D2300124&version=

Entry  Mon Mar 31 11:26:45 2025, Luke Johnson, Update, Scripts/Programs, Heatmaps of power delivery performance  temp_required.pngefficiency.png
These plots show the required temperature to release 100W of power and the efficiency of a particular configuration with half-width w and distance away from the barrel z. I want to add to these heat maps a limit line that has restricts the proximity of the reflectors from the barrel.
Entry  Tue Mar 25 12:56:47 2025, Tyler, Update, TCS, FROSTI Analysis Finalization FROSTI_OPD_profile.pdfFROSTI_temperature_profile.pdf

Upon final review of the FROSTI analysis included in the (hopefully) soon-to-be submitted instrument paper, I've made some adjustments to the reflectivity analysis that estimates the amount of power delivered to the test mass by the FROSTI. Initially, as detailed in elog 447, the delivered power was approximated to be 12.6 W (later adjusted to 12.9 W), with roughly 18% of this power being reflected by the test mass. After some final adjustments, this value now is closer to 12.0 W, with 10.2 W absorbed (15% power reflection). Below is a table showing the updated values for the FROSTI prototype tests:

Old Value New Value
Delivered Power 12.9 W 12.0 W
Absorbed Power 10.6 W (18% reflectivity) 10.2 W (15% reflectivity)
Measured Peak Temperature Difference 5.39 +/- 0.03 K 5.26 +/- 0.03 K
Model Peak Temperature Difference 5.42 K 5.21 K
Measured Peak OPD 765 +/- 9 nm 771 +/- 7 nm
Model Peak OPD 630 nm 654 nm
Entry  Sun Mar 23 15:39:06 2025, Luke Johnson, Update, Scripts/Programs, Ringheater Location optimization _4-4.png_40.png02.pngHOM_power.svg
Attached are some plots that show a new parameter sweep with a finer mesh then before. I have also been able to get a heatmap of power of HOMs in a very simple finesse model.
Entry  Tue Mar 11 11:28:52 2025, Cynthia, Update, Interferometer Simulations, flattening mirror to study power discrepency updates_3_11_(1).pdf
 
Entry  Tue Mar 11 10:43:57 2025, Xuesi Ma, Update, ,  20250310_171936.jpg

Continue investigation in the spikes

Pulsed ADC with a function generator and find no spikes. Rules out ADC for causing the spikes

Loopback test that bypasses the FROSTI Chassis shows spikes (spikes happened on all channels at the same time)

Next step is to bypass the AI Chassis to find the source of the spikes

Entry  Mon Mar 10 21:32:29 2025, Nathan, Physics, Electronics, Beam Profiling and PBS Measurements Beam_Profiling_2_20_(2).pdfbeamprfl.pngthumbnail_(6).jfif
Beam wasn't diverging, however maybe was about to diverge when measurements stopped? Will discuss the PBS measurements and how the voltage changed due to the wave plate.
Entry  Mon Mar 10 21:13:12 2025, Nathan, Update, VLC Update, PDH Lock Progress and Next Steps thumbnail_(2).jfifthumbnail_(4).jfifthumbnail_(5).jfifVisible_Light_Optical_Cavity_(2).pdf
Progress update: Photodiode is set up, need to set up DC bias tee, EOM has 400-600nm wavelength range with a resonance frequency of 0.1-100MHz. Additionally need to connect the DC bias to SR560, put it in low pass, then connect to the function generator and connect it to oscilloscope to observe. Once everything looks good and working, need to connect the driver and we can start actuating on the cavity ETM.
Entry  Mon Mar 10 17:03:52 2025, Shane, Update, CDS, Pressure Gauge successful connect 
Vac system serial interfacing update: the pressure gauge is now able to communicate successfully through the code. It's been set to a static ip of 192.168.1.30, on port 8000.
Entry  Wed Mar 5 18:13:20 2025, Shane, Update, CDS, vac system comms 

[Shane, Jon]

Update on the serial interfacing with the Inficon VGC503 pressure gauge: We began setup of the Inficon pressure gauge today. We configured the ethernet setting via USB and assigned it a static IP address of 192.168.1.30, which is listed in the network table on the lab wiki. It is showing up on the network successfully, and is responding to pings. Will attempt communication via code next.

Entry  Wed Mar 5 12:16:28 2025, Shane, Update, CDS, Vac system communications update 

[Shane, Jon]

Update on the serial interfacing with the vacuum system: both turbo pumps are now able to successfully communicate through the code. The older pump, for unknown reasons, required a newer version of the communication syntax (despite the newer, small pump being able to communicate fine with the old communication format). We have also confirmed that the newer pump works with this new format as well. Next step is interfacing the pressure gauge.

Entry  Tue Mar 4 10:47:03 2025, Shane, Update, CDS, Vac system pinouts vac_pinouts_1.jpegvac_pinouts_2.jpeg
Attached here are the pinouts, as we currently know them, for the vacuum system. The three items focused on here are the Agilent TwissTorr 74 FS turbo pump (the smaller/newer pump) and controller, the Agilent TV 551 Navigator turbo pump (the larger/older pump) and controller, and the Eight-channel Perle IOLAN SDS8 terminal server. The 'field' pinouts in the attached tables refer to the DB9 end of the RJ45F to DB9F converter.
Entry  Tue Mar 4 10:28:58 2025, Tyler, Update, TCS, RIN Plot Updates Dark_bin_veto.pdfMock_final_plot_inst.pdf
 
Entry  Tue Mar 4 10:18:43 2025, Cynthia, Update, Interferometer Simulations, attempted to remove curvature and tilt for the coating  3_4_updates.pdf
 
Entry  Tue Mar 4 03:33:18 2025, Xuesi Ma, Update, , Update 6x

Spikes Appear Again, need to address it systematically.

Power on and off before reaching steady state ✔

At 12V, the rise and fall time of heater elements are different from 24V.

Initial guess is due to temperature in the chamber. However, it does not seem to be the case, 24V with 30c have the same hall time as 24V at lower temperature.

Attached are some graphs for rise and fall time

After a weekend of powering on, the main chamber pressure stabilized in the UHV region.

Temperature in the chamber seems also not to change.

Entry  Tue Mar 4 03:05:42 2025, Xuesi Ma, Update, ELOG, LOG 

1424564097.243212 2025/02/26 00:14:39 UTC Time start

12V 2A right after start all 8 elements

1424564478.079428 2025/02/26 00:21:00 UTC Time stop

12V 1.8A right before stop all 8 elements

1424564832.211584 2025/02/26 00:26:54 UTC Time start

12V 1.9A right after start all 8 elements

1424565208.359935 2025/02/26 00:33:10 UTC Time stop

12V 1.8A right before stop all 8 elements

1424565573.565066 2025/02/26 00:39:15 UTC Time start

12V 1.8A right after start all 8 elements

1424565931.242394 2025/02/26 00:45:13 UTC Time stop

12V 1.7A right before stop all 8 elements

1424566292.67104 2025/02/26 00:51:14 UTC Time start

12V 1.8A right after start all 8 elements

1424566648.619952 2025/02/26 00:57:10 UTC Time stop

12V 1.7A right before stop all 8 elements

1424566996.312246 2025/02/26 01:02:58 UTC Time start

12V 1.8A right after start all 8 elements

1424567381.748943 2025/02/26 01:09:23 UTC Time stop

12V 1.7A right before stop all 8 elements

1424567756.528736 2025/02/26 01:15:38 UTC Time start

12V 1.7A right after start all 8 elements

0.2A right before start


spikes!?


1424643001.864687 2025/02/26 22:09:43 UTC

change c_0(VEXC0 & VCXC0) to 2V (why is it on 5V ?)


2025/02/26 22:18:51 UTC

Main chamber pressure:5.92e-9

RGA chamber pressure:1.98e-9


1424650528.240947 2025/02/27 00:15:10 UTC Time start (increase voltage)

24V 2.1A right after start all 8 elements


disconnect and reconnect (exc 1-4)(out 9-12) & (exc 5-8)(out 13-16)


2025/02/27 19:34:26 UTC

Main chamber pressure:1.34e-8

RGA chamber pressure:4.33e-9

Main chamber temp: 29

RGA chamber temp:29


2025/02/28 18:02:29 UTC

Main chamber pressure:1.05e-8

RGA chamber pressure:3.53e-9

Main chamber temp: 29

RGA chamber temp:30


1424801097.374902 2025/02/28 18:04:39 UTC Time stop

24V 1.8A right before stop all 8 elements

0.1A right after stop


1424827460.71372 2025/03/01 01:24:02 UTC Time start

24V 2.9A right after start all 8 elements

0.1A right before start


2025/03/01 01:25:34 UTC

Main chamber pressure:5.98e-9

RGA chamber pressure:2.06e-9

Main chamber temp:27

RGA chamber temp:27


2025/03/03 20:28:03 UTC

Main chamber pressure:7.8e-9

RGA chamber pressure:2.64e-9

Main chamber temp:27

RGA chamber temp:27

ELOG V3.1.3-7933898