| ID |
Date |
Author |
Type |
Category |
Subject |
|
655
|
Thu Oct 23 10:07:51 2025 |
Liu | Update | Interferometer Simulations | Multi-ring FROSTI optimization for A# |
| 4D parameter space visualization and dimensionality reduction for better optimization |
| Attachment 1: loss_embedding.html
|
| Attachment 2: Update.pdf
|
|
|
658
|
Thu Oct 30 11:45:44 2025 |
Liu | Update | Interferometer Simulations | Multi-ring FROSTI optimization for A# |
| Multi-ring FROSTI optimization for A#: dimensionality reduction with PCA vs. t-SNE |
| Attachment 1: Update.pdf
|
|
|
633
|
Tue Aug 26 12:14:24 2025 |
Liu | Update | Interferometer Simulations | Multi-ring FROSTI design for A# with ring heater optimization |
| Multi-ring FROSTI design for A# with ring heater optimization |
| Attachment 1: Update_(1).pdf
|
|
|
639
|
Tue Sep 2 12:41:33 2025 |
Liu | Update | Interferometer Simulations | Multi-ring FROSTI design for A# with ring heater optimization |
| [Tyler, Liu]
Ring heater optimization, continued |
| Attachment 1: Update.pdf
|
|
|
172
|
Tue Jul 25 15:35:14 2023 |
Shane | Update | Electronics | More chassis moved |
| Finished basic assembly of binary input and output chassis today, and moved one to top shelf of work bench. The other is in corner of work bench (image attached). They are delicate, so please do not move them or place anything on top of them. |
| Attachment 1: IMG_8409.HEIC
|
|
91
|
Wed May 3 19:03:47 2023 |
Julian,Pamella and Cao | Physics | VAC | Modify vacuum asssembly and install RGA |
[Pamella, Julian, Cao]
Today we started re-configuring the vacuum chamber components.
Particle count
- 10:45 am : Starting the particle count in the clean room.
- 11:13 am : Finished the particle count in the clean room.
- Zone 3 :
- 0.3 u: 2535
- 0.5 u: 1413
- 1.0 u: 789
- Zone 4 :
- 0.3 u: 457
- 0.5 u: 290
- 1.0 u: 207
Starting the reconfiguration.
- 11:21 am: Started removing up-to-air valve
- 11:30 am: Finished removing up-to-air valve.
- 11:33 am: Started removing calibrated Ar Leak and the elbow.
- 11:35 am: Finished removing calibrated Ar Leak and started assembling the up-to-air valve.
- 11:47 am: Finished assembling up-to-air valve.
- 11:48 am: Started removing magnetron gauge.
- 11:55 am: Finished removing magnetron gauge.
- 11:57 am: Started installing the elbow and calibrated Ar Leak and started removing the RGA probe
- 12:13 pm: Finished installing the elbow and calibrated Ar Leak.
- 12:20 pm: Break for lunch.
- 01:25 pm: Come back from lunch break.
- 01:30 pm: Started removing RGA line.
- 01:39 pm: Finished removing RGA line.
- 01:39 pm: Started removing gate valve [RGA line] and finished removing gate valve.
- 02:00 pm: Started installing gate valve in the new position.
- 02:08 pm: Fished installing gate valve [RGA line].
- 02:09 pm: Checked the screws in the elbow to gate valve. [RGA line].
- 02:28 pm: Finished checking the screws in the elbow to gate valve [RGA line].
- 02:29 pm: Started installing RGA line.
- 02:39 pm: Finished installing RGA line.
- 02:50 pm: Started installing magnetron gauge.(In this part we assembled gauge with the used gasket)
- 03:02 pm: Finished installing magnetron gauge.
- 03:04 pm: Started installing RGA probe [RGA line].
- 03:13 pm: Finished installing RGA probe [RGA line].
- 03:15 pm: Connected the cables to the magnetron gauge.
- 03:20 pm: Started the testing in the vacuum chamber.
- 04:30 pm: Started installing the RGA 200 and connected the cables (power cable and DB9 cable).
- 04:52 pm: Finished installing the RGA 200 and connected the cables (power cable and DB9 cable).
- 04:53 pm: Started testing the RGA connections. Logrus is able to recognize and connect to RGA unit. We are leaving the turbo pump on for a few hours before checking back for pressure readouts.
- 05:00 pm : Starting the particle count in the clean room.
- Zone 3 :
- 0.3 u: 2244
- 0.5 u: 997
- 1.0 u: 207
- Zone 4 :
- 0.3 u: 2993
- 0.5 u: 1579
- 1.0 u: 498
- 05:30 pm : Finished the particle count in the clean room.
- 05:34 pm: Test pressure readout from the gauges.
- Channel 1 : 1.06E-5 mbar
- Channel 2 :8.89E-6 mbar
- Channel 3 :5.0E-4 mbar
- 05:59 pm: Test pressure readout from the gauges.
- Channel 1: 9.09E-6 mbar
- Channel 2: 7.75E-6 mbar
- Channel 3: 5.0E-4 mbar
|
| Attachment 1: vaccum_chamber_re-configuration.jpg
|
|
|
710
|
Tue May 5 14:13:45 2026 |
Dhatri | Summary | Interferometer Simulations | Mode mismatch |
[Pooyan, Tyler, Ceci, Dhatri]
Attached are the plots generated by running the newer code here: run.py
PRG looks good now!
| Quote: |
[Sidd, Pooyan, Dhatri] In the group meeting on 04/23/26, we discussed with Jon why we weren’t getting expected values for PRC Gain while running the current LLO model; specifically if there is mode mismatch. Worked more on this today.
- Looked at the mode mismatch using cavity_mismatch_table().
- Compared these finesse_ligo factory model mismatch values with those of the aLIGO katscript model.
- The latter does not have the cavity_mismatch_table(), looked at both models' mismatch values using cavity_mismatch().
- Ascertained that there is less mode mismatch in the katscript model (~10^-2) as compared to the factory model (~10^-6).
- Mismatch values are starkly different, not just for (PRC, XARM) but also for others like (OMC, XARM).
Is the issue with the locking procedure?
- Analysed the locking process for factory model and katscript model to find minor differences in the order.
- Tried applying the katscript locking function to the factory model and still seem to get the same results. (to recheck)
Further directions/steps:
- To compare radii of curvature of the optics in both models
- Check q parameter at PRM and assign it to the laser to run the model
- Generate powerup plots again and check against previous ones (with and without ring heater)
|
|
| Attachment 1: llo_power_up_1461976383.pdf
|
|
|
111
|
Wed May 31 16:18:41 2023 |
Aiden | Summary | General | Mock FROSTI |
| Finished assembly on the Mock FROSTI so it is ready for the fit test at LIGO lab. |
| Attachment 1: IMG_4394.jpg
|
|
|
397
|
Mon Jul 8 12:26:10 2024 |
Michael | Update | Interferometer Simulations | Minimizing Astigmatic Effects in the SRC of LIGO |
| This is the first look and analysis of the effects of astigmatism in the aLIGO optical layout which can lead to mode mismatch and therefore increased losses into higher order modes. Specifically I am currently looking at measuring the effect of changing the radii of curvature of the SRC mirrors https://docs.google.com/presentation/d/1qhIehqyNukg4g8S2fqfQZz83yr9aB76tEa6fn2J-TrM/edit?usp=sharing |
|
617
|
Tue Jul 29 11:45:19 2025 |
Maple | Update | TCS | Meeting update |
|
| Attachment 1: Maple_TCS_update_jul_29.pdf
|
|
|
339
|
Sat Feb 24 08:53:38 2024 |
Jon | Infrastructure | Computers | Matlab upgraded to 2023b on Chimay |
| I upgraded Matlab on chimay to the latest stable release, 2023b. From some quick tests, it appears to be in working order. Let me know of any issues. |
|
496
|
Thu Jan 2 17:52:58 2025 |
Luis | Update | VAC | MR Testing Continuation |
[Luis, Luke]
RGA Volume: T = 22°C, P = 2.10e-9 Torr
Main Volume: T = 21°C, P = 5.71e-9 Torr
Measurements of the current state of the vacuum systems were taken today, now that the system had reached UHV status, the results are attached bellow. The first plot overlays the data of the empty chamber taken on 12/16/24 before inserting the MR material, and the data of the system today, with the MR inside. The second plot displays the S/N Ratio of the system. The last plot displays the data of the system with the Ar leak open and closed. Notice that it is common for the Ar leak close data to fail due to the calculation of the gas flux per unit ion current, which is dependent on the Ar peak.
|
| Attachment 1: 2024-12-16_PostBake2_ArO_overlay.png
|
|
| Attachment 2: 2025-1-2_MR-Bake1_ArO.png
|
|
| Attachment 3: 2025-1-2_MR-Bake1_ArC_overlay.png
|
|
|
490
|
Mon Dec 16 21:32:21 2024 |
Luis | Update | VAC | MR Testing |
[Luis, Luke]
The MR material was placed in the vacuum chamber following standard procedures to ensure the vacuum remained as clean as possible. During this process, we only opened the main
volume while keeping the gate valve between the two volumes closed to maintain the UHV in the RGA section.
An RGA scan was taken before this process, this will be used to compare the state of the vacuum with the sample inside to determine whether the MR material is vacuum compatible. |
| Attachment 1: IMG_6011.HEIC
|
|
494
|
Sun Dec 22 20:43:35 2024 |
Luis | Update | VAC | MR Testing |
[Luis, Luke]
RGA Volume: T = 23°C, P = 3.0e-9 Torr
Main Volume: T = 22°C, P = 9.90e-9 Torr
After letting the vacuum cool down for a couple days, we reattached the magnets and sensors, then we performed a RGA scan of the vacuum system, now containing the MR sample. The results are attached below. Something to notice is that we are technically not under UHV, though Luke and I believe the reading of the sensor is not completely accurate since it was still coming to a steady state, further test will be performed when the physics building is open again.
|
| Attachment 1: 2024-12-13_PostBake2_ArO_Degas_overlay.png
|
|
| Attachment 2: 2024-12-22_MR-Bake1_ArO.png
|
|
|
467
|
Tue Nov 5 09:56:04 2024 |
Luis Martin | Update | Clean & Bake | MR Bake |
| [Luke, Luis]
On Friday, 11/1/24, the MR was unpackaged and cleaned under the flow bench. We noticed an ink stain on one of the corners of the material. After wiping it down with IPA and Vector Alpha wipes, the stain was removed. However, the material showed some wear.
After cleaning, we placed it in the bake station and applied a stainless steel baking protocol. On Tuesday, 11/4/24, the material was removed from the furnace and packaged in a static shielding bag. The MR was wrapped in Vector Alpha wipes.
|
|
329
|
Mon Feb 19 14:40:21 2024 |
Shane | Update | CDS | MEDM screen for FROSTI temp readouts |
| Here's the latest draft of the MEDM screen for the FROSTI heating elements' temperature readouts. Note that the MEDM screen isn't actually this grainy, this just happens to be a photo of the lab monitor's screen off a phone. |
| Attachment 1: IMG_6094.jpeg
|
|
| Attachment 2: IMG_6092.jpeg
|
|
|
346
|
Thu Feb 29 17:16:48 2024 |
Shane | Update | CDS | MEDM screen for FROSTI T/P readouts |
| Here's the latest draft of the MEDM screen for the FROSTI temp and power readouts, now with a button linking to the c1msc file display. Size/color/label are all changeable, if adjustment is needed. Checked in execute mode as well, and it's working correctly. Also noticed that the MEDM file name has been changed to FROSTI.adl, which I'm noting here for future reference. Still in medm_sandbox directory. |
| Attachment 1: IMG_6259.jpeg
|
|
|
593
|
Wed Jun 11 16:33:45 2025 |
Pooyan | Update | Computers | Luke's ray tracing hosting |
- Hosted Lukes model on Chimay. It's available at https://richardsonlab.ucr.edu/real-time-frosti
- The sourcecode is at Github. It is clones at
/var/www/html/real-time-frosti, and this is the block added to nginx config file at /etc/nginx/sites-available/default :
location /real-time-frosti {
root /var/www/html;
index index.html index.htm index.php;
}
- Also added this line to the crontab, so the code will be checked for updated from the sourcecode every five minutes.
*/5 * * * * cd /var/www/html/real-time-frosti/ && git pull
- TODO: Move the sourcecode from Github to git.ligo.org, and make the repository public.
|
|
334
|
Wed Feb 21 23:15:07 2024 |
Michael | Update | Interferometer Simulations | Long Shoelaces 1 Layout Created in Gtrace and Fixed Ghosting in Beamsplitter |
| I have created the long shoelaces 1 layout for cosmic explorer using gtrace, a slight modification from the shoelaces 1 layout design. I also modified the simulation code slightly to remove ghosting effects in the beamsplitter. Originally the python code specified that the HR and AR sides of the beamsplitter both have the same transmission/reflection. I modified this to the ideal case of: Refl_AR = 0, Trans_AR = 1. I have attached two images below to show the before and after effect of this modification. |
| Attachment 1: long_shoelaces1_desmos.JPG
|
|
| Attachment 2: AR_side_with_reflection.PNG
|
|
| Attachment 3: AR_side_without_reflection.PNG
|
|
|
317
|
Tue Feb 6 22:40:25 2024 |
Michael | Update | Scripts/Programs | Long Crab 1 Design Created In Gtrace |
| Worked on and completed the python code for the simulation of the Long Crab 1 layout for Cosmic Explorer basing off of Pooyan's original work with the Crab 1 layout. From here I'll look into creating the shoelaces layouts. |
| Attachment 1: Long_Crab1.png
|
|
| Attachment 2: long_crab_1_desmos.PNG
|
|
|
476
|
Wed Nov 20 12:31:24 2024 |
Luis | Update | VAC | Leak test RGA Scan after vacuum repairs |
[Luke, Luis]
After the gasket replacement performed on Monday (11/18/24) we let the vacuum pump down to UHV pressure for a couple days. Today (11/20/24) we measured the pressure to be 5.30*e^-9 with a temperature of 22C, and we performed a leak test and RGA Scan.
Here are the results:
| Connection |
Leak rate (torr) |
| Reducing Cross - TP Left |
4.5e-9 (lowish) |
| Reducing Cross - TP Right |
6.0e-9 (lowish) |
|
| Attachment 1: 2024-11-20_PostBake1_ArO.png
|
|
|
474
|
Tue Nov 19 17:10:34 2024 |
Luke | Update | VAC | Leak check |
Chamber temperature: 23C
Chamber Initial Pressure: ~1.8e-8 main, ~3.5e-8 rga
Did another leak test after monday's work to check how the seal was holding up initial leak was 5.5e-9. I then tried to tighten the bolts a bit more the leak rose to 1.9e-8 about a factor of 4 change.
I checked another flange to confirm that I was preforming the test properly. I measured the elbow to pressure sensor to be 2.2e-11 aproximatly what it was earlier in the month (1.9e-11).
I ran another isolation test. It is still exponetial. Graph attached.
Thoughts:
I belive at this point that it is a knife edge issue when replacing the gasket I checked both flanges and the new gasket. The tp knife edge seemed perfectly fine, the gasket had very minor scratches, and the reducing cross had very small imperfections on its edge.
We may want to try and use the liquid sealant or get annealed gaskets for 4.5" |
| Attachment 1: image.png
|
|
| Attachment 2: IMG_5116.jpeg
|
|
| Attachment 3: IMG_5117.jpeg
|
|
|
462
|
Wed Oct 23 11:48:06 2024 |
Luis Martin | Update | VAC | Leak Test Results |
[Luke, Luis, Mary, Ma]
On 10/22/24 Luke, Ma, Mary and myself ran a leak test, the results are displayed below. The overall pressure of the vacuum was 2.0e-8 and the temperature readings were 26C for the RGA and 25C for the main volume.
| Connection |
Leak rate (torr) |
| Tee - RGA |
9.4e-12 (very low) |
| Tee - Cal leak |
1.58e-11 (very low) |
| Tee - ZLR (2.75"-4.5") |
7.32e-12 (very low) |
| ZLR (2.75"-4.5") - Reducing Cross |
6.9e-11 (low) |
| Cross - Elbow |
2.34e-11 (very low) |
| Elbow - Pressure sensor |
1.96e-11 (very low) |
| Cross - Turbo pump (small) |
1.91e-9 (lowish) |
| Cross - Gate valve |
1.66e-10 (very low) |
| Gate valve - Port |
7.41e-10 (low) |
| Port - ZLR (6.0"-8") |
2.93e-10 (low) |
| ZLR (6.0"-8") - Turbo pump (large) |
6.15e-11 (very low) |
| Port - Pressure sensor |
2.0e-11 (very low) |
| Port - Up to air valve |
1.42e-11 (very low) |
| Port - Blank |
1.27e-11 (very low) |
| Port - Feed through port |
4.59e-12 (very low) |
| Lid - Curtain side |
3.09e-11 (very low) |
| Lid - Wall side |
4.26e-11 (very low) |
|
|
273
|
Mon Nov 20 20:45:16 2023 |
Aiden | Update | VAC | Leak Test |
[Aiden, Luis]
Tested every weld and flange to find leaks. Only found that the flange on the turbo pump and reducing nipple was still at 2e-9 torr on the leak. The chamber still rose in pressure when the two gate valves were closed but no noticeable leak could be found on the lid or welds. |
|
116
|
Tue Jun 6 16:15:09 2023 |
Peter | Update | VLC Update | Launch Optics for Visible Light Cavity |
| I assembled the first few components of the launch optics for the visible light cavity. Below is an image of the current table configuration, and the image is how the cavity will be oriented on the table. |
| Attachment 1: IMG-0882.jpg
|
|
| Attachment 2: IMG-0883.jpg
|
|
|
337
|
Fri Feb 23 15:01:48 2024 |
Shane | Update | CDS | Latest draft of MEDM screen for FROSTI readouts |
| Here's the latest draft of the MEDM screen for the FrOSTI temp and power readouts. Also, debugged the text readout boxes so they're now correctly reading out the live temperature and power values. |
| Attachment 1: IMG_6128.jpg
|
|
| Attachment 2: 23.jpg
|
|
|
495
|
Mon Dec 23 14:33:36 2024 |
Tyler | Update | TCS | Latest RIN Measurement Results |
| Attached below are the measurements I took from the FROSTI from 12/18-12/22. |
| Attachment 1: Updated_ASD_plots.pdf
|
|
| Attachment 2: Dark_Noise_Thermal_ASD_plots.pdf
|
|
| Attachment 3: DC_Voltages.pdf
|
|
| Attachment 4: RP-2.jpg
|
|
|
62
|
Tue Apr 4 09:53:37 2023 |
Peter | Update | VLC Update | Laser intensity/polarization drift measurements |
| The set up for the next round of beam characterization measurements has begun. The beam is initially passing through a half waveplate, is split at a polarizing beam splitter, and then stirring mirrors are used to properly aim the beam into photodiodes (not yet installed). This is the current configuration of the set up. |
| Attachment 1: initial_Intens_measure_set_up.jpg
|
|
|
65
|
Thu Apr 6 10:20:43 2023 |
Peter | Update | VLC Update | Laser intensity/polarization drift measurements |
| More optical components were added to the optical set up for laser intensity / polarization drift measurements. Both lenses and both PDs were added to the configuration, as seen in the image below. The beam is already well aligned into the center of both of PDs, and focused nicely by the lens.
Both PD's take BNC connecting cables, and the Red Pitaya takes SMA connecting cables. Since we are currently without a BNC to SMA cable, and we do not want to cut, strip, and crimp what we have, then measurement process cannot proceed until we get the cables. |
| Attachment 1: Optical_Setup_4-6-23.jpg
|
|
|
83
|
Fri Apr 28 11:21:01 2023 |
Peter | Update | VLC Update | Laser intensity/polarization drift measurements |
| The Digi-key cables have arrived, and I have began implementing them in the intensity drift measurements.
There was a slight problem initially in connecting the SMA to BNC cables from the photodiode to the red pitaya, since the red pitaya was way on the other side of the lab. Cao and I connected the red pitaya to a new ethernet cable that extended far enough for the red pitaya to sit comfortably on the breadboard with the optics.
Right now the PDAs are not connected to the red pitaya. I have connected them to the oscilloscope in order to read out how much voltage they produce upon incidence of 532nm laser light. This was done in order to make sure that they do not surpass the limit of the red pitaya (+-1V). I have not acquired a value for the readout voltage of the PDAs since I had to go to class. I will gather this preliminary data soon. |
| Attachment 1: IMG-0183.jpg
|
|
|
102
|
Mon May 22 16:43:28 2023 |
Peter | Update | VLC Electronics | Laser intensity/polarization drift measurements |
| In order to fully analyze the polarization data taken last Thursday, I needed to convert the signal output (which is in volts) to power (units of watts). I used the power meter to accomplish this. Keeping the exact same configuration of PD's and beam splitting, opened the red pitaya's oscilloscope package. I then took the power meter, and held it in front of the PD to measure the amount of Watts at each PD. I then wrote down the corresponding voltage being seen in the red pitaya. I took 5 sets of measurements for each PD to get experimental accuracy. I then used a simple y = mx + b fit to find out the constant m that converts the input wattage into voltage. For the s polarization, the conversion factor is 0.83. For the p polarization, the conversion factor is 1.12. I then used this data to plot polarization angle as a function of time, and the relative intensity drift as a function of time. The plots are shown below. The physical meaning of the polarization angle is shown in the unit circle diagram below, in which P is the total power. |
| Attachment 1: S-P_Polarization_Diagram.svg
|
|
| Attachment 2: Polar_angle_vs_time.png
|
|
| Attachment 3: Rel_Intens_vs_time.png
|
|
|
107
|
Wed May 24 14:28:26 2023 |
Peter | Update | VLC Electronics | Laser intensity/polarization drift measurements |
| I went in and took polarization drift data for 16 hours. The run started at 6:08pm and finished at 9:15am the next day. The four plots below are the same plots shown for the 2 hour collection and previous trials, except they extend to 16 hours. The only one that is different is the Power vs. Time graph. This is a graph of the actual incoming power of the laser (as opposed to the signal voltage that the PDA's output into the red pitaya). This was done using the calibration factors of the respective PDA's and as we can see, since there is a difference in the calibration factors between detectors, there is a difference in the power that's coupled into S and P polarization. |
| Attachment 1: Time_Series_Trial_7_16hrs.png
|
|
| Attachment 2: Power_vs_Time_16hrs.png
|
|
| Attachment 3: Polar_angle_vs_time_16hrs.png
|
|
| Attachment 4: Rel_Intens_vs_time_16hrs.png
|
|
|
21
|
Sat Feb 4 17:01:03 2023 |
Peter | Update | VLC Electronics | Laser Data |
| Peter and Ryan took laser beam data. Configuration: 100mm focal length lens is ~100mm from lens. 150mm focal length lens is ~200mm from first lens. Beam waist is ~420mm from second lens.
Beam waist is very small still. Had to input large amounts of error in data collection. Took width data successively at points near waist and at >= Rayleigh range. Plots are shown below.
Key points:
Took a while to figure out optimum configuration for lenses to be placed so that an accessible beam waist could be obtained.
Beam waist is still very small. May need to do an ABCD calculation to see if there is anything bigger that can be obtained. |
| Attachment 1: OmegaX_M2_Fit_3.png
|
|
| Attachment 2: OmegaY_M2_Fit_3.png
|
|
|
670
|
Thu Jan 22 10:10:31 2026 |
Jon | Infrastructure | General | Lab floor plans |
| Attached are the starting and final floor plans for the February 2026 expansion into the Physics 1125 lab. |
| Attachment 1: Pre-Feb-2026.png
|
|
| Attachment 2: Post-Feb-2026.png
|
|
|
672
|
Thu Jan 22 13:18:12 2026 |
Pooyan | Infrastructure | General | Lab floor plans |
The working document of tasks regarding moving the clean room is attached. Needs LIGO account to access and edit.
https://docs.google.com/document/d/14HhMYBcHmM62Hc1YJhinMsG5uPx6xoW0WEBmDcbNMMg/edit?usp=sharing
|
|
676
|
Thu Feb 5 11:42:47 2026 |
Jon | Infrastructure | General | Lab floor plans |
[Audrey, Cece, Jon, Ma, Mary, Michael, Pooyan, Tyler, Shane]
We have completed the preliminary reorganization of our Physics 1119 lab space. This includes:
- Moving all cabinets to their final positions
- Clearing out all equipment from the cleanroom in prep for HVAC work, and storing them in either the HEPA cabinet or double-bagging in regular storage.
- Moving all non-essential equipment into other lab spaces.
- Wrapping vacuum system and VLC for protection
- Removing all ceiling tiles and fans from the ceiling of the cleanroom
- Moving the cleanroom frame towards the front of the room.
Prepping the new clean-and-bake station in 1125 will begin within the next week, along with the construction of the stainless steel table planned to be put into the cleanroom.
| Quote: |
| Attached are the starting and final floor plans for the February 2026 expansion into the Physics 1125 lab. |
|
| Attachment 1: image.jpg
|
|
| Attachment 2: image_1.jpg
|
|
| Attachment 3: image_3.jpg
|
|
|
682
|
Thu Feb 12 12:25:38 2026 |
Xuesi Ma | Infrastructure | General | Lab floor plans |
[Cece, Ma, Mary, Pooyan, Tyler, Paul]
We have continued the reorganization of our Physics 1125 and 1129 lab spaces. This includes:
- Moving two workbenches from Room 1129 into Room 1125
- The workbench with the oven is still in Room 1129
- Assembling the stainless steel table
- Moving the cleanroom frame toward the whiteboard side to make room for HVAC work
The sink in Room 1125 was painted, and we stood Frosti up. |
| Attachment 1: 2563.jpg
|
|
| Attachment 2: 2567.jpg
|
|
| Attachment 3: 2570.jpg
|
|
| Attachment 4: 2569.jpg
|
|
| Attachment 5: 2564.jpg
|
|
| Attachment 6: 2565.jpg
|
|
| Attachment 7: 2568.jpg
|
|
| Attachment 8: 2566.jpg
|
|
|
46
|
Wed Mar 8 18:35:52 2023 |
Pamella | Update | | Lab cleaning |
| Today Pamella finished cleaning of the cleanroom, starting with the HEPA vacuuming, mopping and clearing all floor with IPA wipes.
Also Pamella and Julian finished cleaning of lab floor, starting with the HEPA vacuuming and mopping.
Shane and Pamella wiped down every surfaces of the laser table, computer table and the table with the vacuum pieces inside the cleanroom.
Shane, Peter, Tayler, Pamella and Julian then wiped down every surface of the laser table outside the cleanroom. We wiped the main tabletop as well as the legs and all parts for the table. We wiped the computer desk, the boxes, the cabinets and every part outside the cleanroom. For now we finished the lab cleaning. |
|
68
|
Tue Apr 11 17:56:15 2023 |
Pamella | Update | General | Lab cleaning |
| Today Pamella and Julian finished cleaning of the cleanroom, starting with the HEPA vacuuming, mopping and clearing all floor with IPA wipes. Also we wiped down some surfaces of the blue table, computer table and the top of chamber. |
|
605
|
Mon Jul 7 17:44:04 2025 |
Tyler | Update | General | Lab Organization |
| [Tyler, Pooyan, Ma, Cece, Luke, Luis, Christina, Maple]
After acquiring some new equipment for the labs, a few of us spent time on Thursday and Friday sorting through everything and storing them into their appropriate places. New vacuum parts, power supplies, cables, and much more were included. The rooms are now ready for the lab tours commencing Tuesday afternoon. |
| Attachment 1: IMG_1874.jpg
|
|
| Attachment 2: IMG_1872.jpg
|
|
| Attachment 3: IMG_1871.jpg
|
|
|
257
|
Wed Nov 8 17:55:49 2023 |
Jon | Update | General | Lab Clean-Up Day 1 |
[Jon, Tyler, Shane, Peter, Luis]
Today we completed the first phase of lab clean-up. Activities included:
- CF/KF parts stored under the cleanroom table were removed and transferred to Physics 1129
- Cleanroom workbench cleared, with all FROSTI hardware collected into one of the large SS bins
- High surfaces outside the cleanroom (lights, table enclosure frames, rack, cabinets) wiped down with IPA wipes
- Floor HEPA-vacuumed outside the cleanroom
- Sticky mats changed throughout the lab
Tomorrow, we will complete turn-over of the cleanroom (HEPA vacuuming of floors, mopping of floors, IPA wiping of softwalls and work surfaces). Shane will post a forthcoming measurement of the cleanroom particulate levels, post-turnover. |
|
528
|
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 |
|
182
|
Mon Jul 31 12:39:01 2023 |
Shane | Update | Electronics | LED cable assemblies installed |
| Today I put together the two LED cable assemblies for the CyMAC and mounted them in the anti-aliasing and anti-imaging chassis. |
| Attachment 1: IMG_8514.jpeg
|
|
| Attachment 2: IMG_8516.jpeg
|
|
|
134
|
Tue Jun 27 14:04:42 2023 |
Sophia A. | Update | Measuring Noise in Interferometer | Interferometer set up and connection to red pitaya |
| Today we (Sophia and Tyler) constructed the set-up for the electrical noise calculation that I will be conducting this summer. I have included images of the setup below. Our system is effectively a green laser, that feeds into a type of polarizer, then into a beam splitter which sends the laser light down two arms into detectors. We started by connecting the detectors to an oscilloscope to determine whether the signal will exceed 1V, as the red pitaya (our planned data collection device) cannot receive signals with a higher voltage than 1V. We spent most of our time calibrating the oscilloscope and fine-tuning the set-up so that we would have approximately equal voltages in each arm of the interferometer. Once confirming that the output voltage would not meet or exceed 1V, we switched from an oscilloscope to the red pitaya for our measurements. Now that the system is set up, we will be able to run code in the red pitaya interface that will run an FFT on the signal, and then do noise analysis from there. |
| Attachment 1: IMG_6756.jpg
|
|
| Attachment 2: IMG_6754.jpg
|
|
| Attachment 3: IMG_6755.jpg
|
|
|
81
|
Thu Apr 27 16:23:44 2023 |
Cao, Pamella and Julian | Physics | VAC | Installing vacuum system (cont.) |
[Pamella, Cao and Julian, Shane]
- Particles account
- 10:37 am: Starting the particles account
- Zone 3:
- 0.3u: 1662
- 0.5u: 872
- 1.0u: 415
- Zone 4:
- 0.3u: 831
- 0.5u: 124
- 1.0u: 0
- 11:14 am: Start removal of calibrated leak to install 45 deg elbow
- 11:21 am: Elbow installed, re-install calibrated leak back on
- 11:29 am: Finished re-install calibrated leak, start installing gate valve on pump line
- 11:47 am: Finished installing gate valve, start installing reducing cross onto gate valve
- 12:02 pm: Finished installing reducing cross, start installing 90 deg elbow to reducing cross
- 12:17 pm: Finished installing reducing cross, lunch break
- 01:24 pm: Come back to the lunch break.
- 01:26 pm: Start installing vacuum hose to elbow.
- 01:40 pm: Finished installing vacuum hose.
- 01:43 pm: Start installing turbo pump.
- 02:00 pm: finished installing turbo pump .
- 02:10 pm: Start installing standard wall hose from turbo pump to scroll pump
- 02:21 pm: finished installing hose onto scroll pump, start installing lid. Remove lid from chamber, insert viton O-ring. Place lid back
- 02:30 pm: Secure lids with screw. Start installing turbo pump controller cable: Pass cable from outside (controller) up the top of clean tent and connect to 8 pin connector on turbo pump
- 03:00 pm: Installing air cooling unit for turbo pump, found 8 M3 screws for air cooling unit in the C&B cabinet to install the fan bracket onto the back of turbo pump. Fan control cable is routed up to the top of the cleanroom to the controller
- 03:15 pm: Installing full-range gauge cable to the controller outside cleanroom. Ethernet cables 1 and 2 are used. Cable 1 is used on the RGA line gauge. Cable 2 is connected to the main body gauge. Cable1 and 2 are connected controller's channel 1 and 2 respectively.
- 04:00 pm: Finish installing gauges cables. Cables are routed up along the frame to the controller sitting outside the cleanroom
- 04:15 pm: Finished. End-of-date particle count
- Zone 3:
- 0.3u: 3699
- 0.5u: 1454
- 1.0u: 872
- Zone 4:
- 0.3u: 1662
- 0.5u: 706
- 1.0u: 290
|
| Attachment 1: IMG_0139.png
|
|
| Attachment 2: IMG_0136.png
|
|
|
87
|
Mon May 1 17:10:25 2023 |
Julian, Cao | Physics | VAC | Installing Pirani gauge and RGA probe onto to vacuum chamber |
[Julian, Cao]
- 03:00 pm: Particle count
- : Zone 3
- 0.3 um: 498
- 0.5 um: 124
- 1 um: 124
- : Zone 4
- 0.3 um: 748
- 0.5 um: 457
- 1 um: 374
- 03:32 pm: Installing Pirani gauge onto pump line
- 03:51 pm: Finish installing Pirani gauge, start installing RGA probe
- 04:03 pm: Finish installing PRGA probe, start routing cable from gauge controller to Pirani gauge
- 04:30 pm: All ethernet cables are routed and connected to gauge controllers
- 04:48 pm: Power gauge controller up, all gauges are recognised and readout shows atmospheric pressure as expected (1000 mbar)
- 04:51 pm: End-of-work particle count
- : Zone 3
- 0.3 um: 1413
- 0.5 um: 872
- 1 um: 623
- : Zone 4
- 0.3 um: 374
- 0.5 um: 166
- 1 um: 166
We also closed all the valves so we can start testing vacuum pump down of isolated volume tomorrow.
|
| Attachment 1: PXL_20230501_225241491.jpg
|
|
| Attachment 2: PXL_20230501_235854958.jpg
|
|
| Attachment 3: PXL_20230501_234750795.MP.jpg
|
|
|
11
|
Mon Oct 3 17:21:39 2022 |
Cao | Update | TCS | Inspection of macor parts |
The macor parts arrived and inspected today. These include:
- Macor spacer (drawing:
LIGO_Redesign_Macor_Spacer_Drawing_v4.pdf attached below), quantities: 40
- No defects, damages observed
- Parts are free from grease/ machining fluid
- Wall thickness of 1 mm appear to provide sufficient stiffness to part
- Images of parts:
Macor_spacer_0.jpg, Macor_spacer_1.jpg
- Macor 5-40 UNC screw (drawing:
LIGO_Redesign_Macor_Screw_Drawing_v6.pdf attached below), quantities: 20
- One screw broke, location of break: should edge between head and shaft (see image
Macor_screw_5.jpg )
- All other screws look ok, no damage observed, clean surface overall
- Images:
Macor_screw_0.jpg , Macor_screw_4.jpg
|
| Attachment 1: LIGO_Redesign_Macor_Spacer_Drawing_v4.pdf
|
|
| Attachment 2: Macor_spacer_0.jpg
|
|
| Attachment 3: Macor_spacer_1.jpg
|
|
| Attachment 4: LIGO_Redesign_Macor_Screw_Drawing_v6.pdf
|
|
| Attachment 5: Macor_screw_5.jpg
|
|
| Attachment 6: Macor_screw_0.jpg
|
|
| Attachment 7: Macor_screw_4.jpg
|
|
|
582
|
Mon May 26 23:24:33 2025 |
Michael | Update | Interferometer Simulations | Initial Monte Carlo Simulations for Toroidal Mirrors Project |
| I've run an initial Monte Carlo simulation for statistical comparison of toroidal mirrors for the dual FROSTI TCS case. Below is the link to the slides.
slideshow |
|
571
|
Tue May 6 13:07:34 2025 |
Michael | Update | Interferometer Simulations | Initial Convergence Plots for Toroidal Mirrors Project |
|
| Attachment 1: Convergence_Plots_5_6_25.pdf
|
|
| Attachment 2: Convergence_Plots_5_6_25-1.pdf
|
|
| Attachment 3: aperture_num_points_convergence.png
|
|
|
373
|
Mon Jun 3 14:14:39 2024 |
Tyler | Update | FLIR | Initial CIT FROSTI Analysis |
| [Tyler]
Attached below are the initial results of the CIT FROSTI testing analysis.
|
| Attachment 1: CIT_FROSTI_Analysis_Group_Meeting-2.pdf
|
|