Took transfer functions for ITMY M0 and R0 now that we are in a good enough vacuum. The ones I had taken in air before doors were put on are here: 83876.
M0
Data (/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGM0/Data/)
2025-04-21_1700_H1SUSITMY_M0_Mono_WhiteNoise_{L,T,V,R,P,Y}_0p01to50Hz.xml
Results (/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGM0/Results/)
2025-04-21_1700_H1SUSITMY_M0_ALL_TFs.pdf
2025-04-21_1700_H1SUSITMY_M0_DTTTF.mat
Committed to svn as r12261 for both Data and Results
R0
Data (/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGR0/Data/)
2025-04-21_1800_H1SUSITMY_R0_WhiteNoise_{L,T,V,R,P,Y}_0p01to50Hz.xml
Committed to svn as r12259
Results (/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGR0/Results/)
2025-04-21_1800_H1SUSITMY_R0_ALL_TFs.pdf
2025-04-21_1800_H1SUSITMY_R0_DTTTF.mat
Committed to svn as r12260
I wanted to compare these measurements with old ones, and on the first try I tried comparing these measurements to the last time that ITMY measurements in vac were taken, which was a measurements set from 2018-05-22_2119 and 2018-06-08_1608 for M0 and R0 respectively. However, comparing these two measurements to the ones I just took, there are multiple differences in some of the cross-coupling traces, so I then decided to also compare my measurements to the last full set that was taken (which was in air), 2021-08-10_2115 and 2021-08-11_2242 for M0 and R0. These measurements line up well with the current measurements, so ITMY is looking good!
Comparison between May/June 2018 In-Vac vs Aug 2021 In-Air vs April 2025 In-Vac (/ligo/svncommon/SusSVN/sus/trunk/QUAD/Common/Data/)
allquads_InVacComparison_MayJun2018vAug2021vApr2025_ALLM0_TFs.pdf
allquads_InVacComparison_MayJun2018vAug2021vApr2025_ALLM0_ZOOMED_TFs.pdf
allquads_InVacComparison_MayJun2018vAug2021vApr2025_ALLR0_TFs.pdf
allquads_InVacComparison_MayJun2018vAug2021vApr2025_ALLR0_ZOOMED_TFs.pdf
allquads_InVacComparison_MayJun2018vAug2021vApr2025_ALL_TFs.pdf
allquads_InVacComparison_MayJun2018vAug2021vApr2025_ALL_ZOOMED_TFs.pdf
Committed to svn as r12263
Adding a comment to talk about the L2P coupling in page 20. It appears as if we have a non-minimum phase zero that appears and dissappears between measurements [see page 20 of the original post above].
While I don't have a full explanation for this behavior, I remember seeing these shenanigans when I was testing the ISI feedforward many years ago. I was too young to make any coherent argument about it, but I remember seeing that the state of the ISI seemed correlated with the behavior. If the ISI is ISOLATED we have normal behavior, if it is DAMPED then we have the non-minimum phase behavior.
Here is a comparison between the last few years of successful ITMY M0 to M0 transfer functions, with the ISI states retrieved from plotallquad_dtttfs.m. The color coding is selected to separate the situations with the ISI in 'ISO', and with the ISI in any other state. in pseudocode:
I got the same comparison done for ITMX and the ISI backreaction theory really does not seem to hold water.
There are two main regimes, same as ITMY. This time, the more recent ITMX TFs (after 2017-10-31) look more similar to the old (prior to 2021) ITMY TFs.
I am at a loss of what is making the change happen. Brian suggested it might be related to the vertical position of the suspension, maybe this is the next thing to test.
To back up Edgard's conclusion, I took measurments with the ISI in Fully Isolated and we didn't get the extra zero back 84083
The FMCS Reverse Osmosis (RO) system has been error free for 10 days following the water leak repair. Its alarms have been returned to the CDS cell phone alarm system.
Following the crash of h1susauxh2 over the weekend, I reviewed the alarm configuration to see if we would get cell phone alarms if something happened to h1edc which runs on h1susauxb123. To this end I have added two new alarm channels to the alarms system.
Both of these changes went into effect at 13:20 PDT when the alarms.service was restarted on cdslogin.
A Norco tech came to the site to inspect the 8 LN2 dewars that feed the cryopumps. Inspection report will be posted to Q2000008 once received.
- No major issues found, some small leaks were repaired as they were found
The vacuum jacket pressures were also measured during inspection:
The vacuum jackets were all pumped down to <10 mtorr last May (excluding CP4 which is not in use), see alog 77742
Dewar | Pressure (micron/mtorr) |
CP1 | 12 |
CP2 | 21 |
CP3 | 215 |
CP4 (not in service) | 220 |
CP5 | 12 |
CP6 | 10 |
CP7 | 16 |
CP8 | 9 |
Fil Marc Daniel
We noticed that the photodiode pins of the in-air cable that connects to RM1 and RM2 were flipped. This will flip cathode and anode which will only matter if there is a bias applied.
Going thru the schematics it seems that with 1:1 wiring the PD anode and cathode are flipped compared to what is shown in Sat Amp D080276. I assume somebody noticed this and flipped the corresponding pins of the in-air cable to correct for it back in 2013. The polarity of the PD doesn't really matter, if there is no bias. We checked the RM sat amps and they have no bias.
If the Sat Amp PDs are connected as shown om D080276, the OSEM values will be negative. Indeed, the RMs had negative OSEM values as expected. However, all ZMs have positive values, since nobody bothered to flip the pins. We propose to no longer flip the PD pins for the RMs and work with positive OSEM values in the future.
J. Kissel First, supporting Daniel's findings that the RM1 and RM2 HTTS OSEM sensor readbacks have been incorrectly negative for ages, I attach a trend of the OSEM ADC input values (and OSEMINF OFFSETS and GAINs) back to 2017. Not said explicitly in the above aLOG -- Daniel / Fil / Marc installed fresh new DB25 Sat Amp to Vac Feedthru cables (D2100464) just after this aLOG as a part of cabling up the new signal chain for PM1. These cables are one-to-one pin-for-pin cables so it *should* have played no role in the sign of the sensors or how they're connected. However, it's now obvious that RM1 and RM2 have had the ADC input voltages as negative for a *very* long time. I reviewed the signal chains for the OSEM PDs; see G2500980. The RMs are using a US 8CH satamps D1002818 / D080276. I attach a screen-cap of page 4, which highlights that - UK 4CH satamps D0900900 / D0901284 use . a negative reverse bias configuration, with . anode connected to bias and cathode connected to the negative input of the TIA, and . an inverting differential amplifier stage - US 8CH satamps D1002818 / D080276 use . a positive reverse bias configuration, with . cathode connected to the bias and anode connected to the negative input of the TIA, and [hence the apparent "pin-flip" from the other two satamp types] . a non-inverting differential amplifier stage - US 4CH satamps D1900089 / D1900217use . a negative reverse bias configuration, with . cathode connected to the bias and anode connected to the negative input of the TIA, and . a non-inverting differential amplifier stage [hence the overall "sign flip" from the other two] I disagree with Daniel that "the polarity of the PD" i.e. how the anode and cathode are connected to the transimpedance amplifier. All versions of the PD pinout + SatAmp configure the system in a reverse bias, be it negative or positive. In these configurations, even in a zero bias configuration, photocurrent always flows from from cathode to anode as light impinges on the PD. So if the anode is hooked up to the negative input of the transimpedance amp (as in D1002818), that signal will have a different sign than if the cathode is hooked up to the negative input (as in D0900900 and D1900089). The RMs should have their *positive* bias from the D080276 circuit applied. In 2011, we'd agreed in G1100856 to jumper all OSEM satamps to the "L" position, a.k.a. the LIGO OSEM a.k.a. AOSEM position, which uses a bias voltage and is thus in photo conductive or pc mode. This is mostly because we wanted to not have to think about keeping track of which satamps are jumpered and which are not, but also because the BOSEM PD didn't mind have a bias, even though it was designed to have no bias. Given the "thought of 2nd to last, last, and never" history of the RMs as they traversed subsystem from ISC to SUS circa O1, moving from the ASC front-end to a SUS front-end circa O2, then never really appearing in wiring diagrams until O3, etc. it wouldn't surprise me if the RMs didn't get the memo to put the bias jumper in the "L" position jumpering pins 2 and 3. I disagree with Daniel: only the US 4CH satamp D1900089 / D1900217 should read negative with light on it. So, my guess is that that someone "in 2013" (i.e. during aLIGO install prior to O1) didn't understand these subtleties between the UK 4CH and US 8CH satamp, saw the "different from UK 4CH satamp" and tried fixing the pins of the in-air D25 from satamp to vacuum flange. Regardless, the new cable has cleared up the issue, and ADC voltage from RM1 and RM2 is now positive.
WP12472 POP_X and LSC_REFL_B changes
Daniel, Erik, Dave:
New h1lsc and h1asc models were installed at 12:50 PDT. No DAQ restart was required.
h1lsc restart caused TIM errors in h1ioplsc0 and h1sqz.
FAMIS 31082
Generally, things are stable following the three days of work in the enclosure for the SPI pick-off path install last week, which show clearly on several trends. Most notable is the decline in PMC and RefCav transmission, which have significant misalignments as seen by the beam spot cameras. Fil and I plan to switch the connection of the picomotors to their new driver tomorrow, so after that they'll be usable again and I'll touch up the alignments.
Also, we have still not increased the pump currents for AMP1 as we noticed last week following the power outage. This should bring the power out of both amplifiers and the PMC closer to their levels pre-outage.
Mon Apr 21 10:08:36 2025 INFO: Fill completed in 8min 32secs
FAMIS 26393
Laser Status:
NPRO output power is 1.843W
AMP1 output power is 69.23W
AMP2 output power is 139.7W
NPRO watchdog is GREEN
AMP1 watchdog is GREEN
AMP2 watchdog is GREEN
PDWD watchdog is GREEN
PMC:
It has been locked 3 days, 15 hr 20 minutes
Reflected power = 23.37W
Transmitted power = 104.4W
PowerSum = 127.8W
FSS:
It has been locked for 3 days 15 hr and 20 min
TPD[V] = 0.6888V
ISS:
The diffracted power is around 4.0%
Last saturation event was 3 days 15 hours and 20 minutes ago
Possible Issues:
PMC reflected power is high
FSS TPD is low
Morning dry air skid checks, water pump, kobelco, drying towers all nominal.
Dew point measurement at HAM1 , approx. -42C
TITLE: 04/21 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
SEI_ENV state: MAINTENANCE
Wind: 3mph Gusts, 1mph 3min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.14 μm/s
QUICK SUMMARY:
VAC Team reports that the corner's pressure is currently 2e-6 Torr
I made a couple of ancilliary investigations while I was in-chamber helping adjust CPY. First, I shined a flashlight through the ITMY elliptical baffle towards the BS. Figure 1 shows that this produced a 45 degree annular beam, similar to the one observed during lock that I noted here ( 83050 ) , consistent with the hypothesis that it is a reflection from the BS cage (see linked alog).
Second, our entry through BSC8 also reminded me that LHO has some unique potential scattering sites that LLO does not have. Figure 2 shows that several of the blanked off nozzles in BSC8 act as corner retroreflectors visible to the beam spot on ITMY, and there is a reflection from the chamber, just below the beam. A look at my compilation of beam spot photos from several years ago ( 41142-Figure3 ) also shows these issues at ITMX (second page of Fig. 2). We should probably put in nozzle baffles next time we are in-chamber near BSC8 and 7.
I recently reported on multiple potential stray light issues in the vertex area, including a 45 degree conical annular beam from the beamsplitter, and a reflection of the halo of the beam passing through the ITMX elliptical baffle that is roughly directed at ITMY (83050). In a first attempt to study potential scattered light noise problems from these beams, before the break I injected 0.2 Hz X and Y motion onto the BS HEPI, with motion amplitudes of about 1e-6 m at stages, 0 and 2 (see figure). The figure demonstrates with spectrograms and spectra (second page), that there is a slight increase in DARM noise for both X and Y injections, mainly below 60 Hz. I turned the injections on and off multiple times because the noise is pretty subtle. I think we should further study these potential scattering issues after the break.
Sun Apr 20 10:09:17 2025 INFO: Fill completed in 9min 14secs
Here's a quick summary of the Estimator installation from this week (Edgard, Oli, Jeff K, Brian L)
slides with basic info: T2500082
FRS ticket 32526
Installation alogs
Infrastructure installed on HAM2/PR3 and HAM5/SR3, style updates to model, MEDM linked to sitemap - alog 83906
Tools installed in Estimator folder in the SUS SVN alog 83922
We updated the OSEM 10:0.4 calibration filters, but only on SR3 and PR3. alog 83913
Damping filters installed - alog 83926
Tested the fader switch - alog 83982
Designed and installed a blend for SR3 Yaw (DBL_notch in the first filter bank) - alog 84004
Created a new OSEM calibration script - alog 84005
(Edgard is thinking about a general version of this using Python, that is still TBD)
Fitting is well underway, but isn't done yet.
We made much more progress than we expected - thanks Oli and Jeff for all the help. It's not quite ready to go, we need to install the TF fits for the model.
We might have actually been able to test, except the temperature changes from the pumpdown were causing the SR3 optic to move, and the TFs were not very stable. Edgard is working on a log to document this. We have good fits for SR3 yaw taken Friday morning, and we might just try these remotely with Oli's help. We do plan to get a clean set of TFs in a few days when things have stabilized.
-- notes for next steps, thanks to Sheila for this --
We plan to leave the SR3 overall yaw damping gain at -0.5. This means we'll set the 'light damping' to -0.1 and the gain in the estimator to -0.4. Edgard used -0.1 for the fitting, but he notes that the Q's are pretty high so we may need to revisit this.
SR3 oplev channels are : H1:SUS-SR3_M3_OPLEV_{PIT,YAW}_OUT_DQ
Some interesting alogs about the impact of changes to SR damping: alog 72106 and 72130
Elenna's PR3 coherence plots: alog 65495
I've attached a quick spectrum of SR3 yaw and pitch on M3 as seen by the optical lever. It's odd - the yaw looks very lightly damped - but the IFO was in observe. You can not see real motion above the 3.4 ish Hz yaw mode (it should be falling faster that 1/f^6). You might be seeing real motion between the peaks though - and we can use that (peaks at 1, 2.3, 3.4).
(environment was pretty quiet - BLRMS - EQ is 40-100 nm/sec, microseism is 200-400 nm/sec, wind speed below 1 m/s, anthropogenic is 20-30 nm/sec. It's 3 pm Saturday afternoon, local time. )
I've added 2 more plots. The first is to check that the Y damping is on, and it seems to be. This is a spectrum of the Y osem signal. Ignoring seismic input (which is completely fair), the signal here should just be yaw_osem_noise * (1/1-G) (the minus sign assumes you get all the loop gain signs directly from the control). You can see dips at the resonances, so the loop is on, and has some gain, but not much at the 1 Hz mode, more at 3.4 ish Hz. I've also added my yaw noise reference from G2002065 - you can see here that the noise is a bit larger than my estimate above 1 Hz.
LDVW shows that the gain on the M1_DAMP_Y control was already turned down to -0.5 at this time.
Here is a comparison of the spectra of three channels that can be used to monitor the performance of the estimator. We compare the motion when the M0 Yaw damping loop gain is at -0.5, versus when it is at the -0.1 (which is what we are aiming for with the estimator). The equivalent estimator plots should look somewhere in between the purple and blue curves in the images attached.
- The first one is the OPLEV on SR3. If the estimator works, we should be able to see a difference on the mode Qs. The oplev should see that we are able to damp (or control) the modes to the same level as the -0.5 damping.
- The second one is the M1 OSEM spectrum. The closed loop spectrum dips at the resonances of the plant at -0.5 gain (because of the sensitivity function), so we should be able to see that the sensitivity (as seen by the OSEM) is different, but the OPLEV sees good control of the modes.
- The third one is the total drive on M1. We should see that the total drive around the resonances is similar to the drive we get with the -0.5 gain, but the total drive should decrease rapidly above 3 or so Hz. We will need a faster channel than the one shown in the last attachment.
The plan is to make a full list of channels to monitor in conversation with Oli and Jeff, then run a pilot test with the fits from 84041 later in the week.
S. Koehlenbeck, J. Freed, J. Kissel, J. Oberling, R. Short
The SPI pick-off path installation on the H1 PSL table is now complete. The beam in the new SPI path has been reduced to 20mW and is currently being dumped with a razor dump between SPI-L1 and SPI-L2. Pictures attached reflect the final installation and layout, which will be be reflected in the updated as-built layout at a later date.
Associated entries: 83925, 83933, 83956, 83961, 83978, 83983 (and more to come)
ECR E2400083 IIET 30642 WP 12453 Here's Ryan's birdseye view labeled with all the components. For details of the components, see the SPI BOM, T2300363, exported from its google sheets to -v4 as of this entry.
Tagging EPO for photos.
83996 Power In ALS / SQZ / SPI Paths Post SPI Pick-off Install
RyanC, Rahul
SUS Tip Tilt - RM1, RM2 and PM1 (picture attached) are now ready to be installed into HAM1, once the chamber is ready to accept them. The blade springs of all three suspensions have been un-muted and bosem connectors have kapton take inserted to prevent grounding issues. This morning we cleaned all three optics using First Contact - see picture for reference.
PM1 Beam Dump (rear)
Camilla, Betsy, RyanC, Rahul
SUS PM1 (Tip Tilt) has a new beam dump attached to it's rear - as shown in several pictures attached below. We had to design a new plate (D2500101_V1) to attach the beam dump. I can confirm that all the components integrates well with PM1 and there is some scope for adjustability as well.
Team SUS is now ready for HAM1 installation work.
Tagging EPO for photos.
S. Koehlenbeck, J. Freed, R. Short, J. Kissel
The mode matching of the PSL pick-off beam to the SPI fiber collimator has been implemented using two lenses. The target beam has a mode radius of 550 µm at a position 63.5 cm downstream from the SPI beamsplitter (SPI-BS).
The lens configuration that produced the closest match to the target mode used:
L1: Focal length = 100 mm
L2: Focal length = 60 mm
Attached is a beam profile fit performed using JaMMT on data acquired with a WinCamD of the beam after SPI-L2. The measured beam radii at various distances from the SPI-BS are as follows:
Distance (cm) | Horizontal Radius (µm) | Vertical Radius (µm) |
---|---|---|
70.734 | 476 | 542 |
91.054 | 470 | 543.5 |
116.454 | 558.5 | 616.5 |
Both lenses are oriented such that their planar sides face the small beam waist between the two lenses. The arrows on the lens mounts point toward the convex surfaces.
The power transmission through the fiber has been measured to be 83 %.
ECR E2400083 IIET 30642 WP 12453 Some "for the record" additional comments here: - Sina refers to the "SPI-BS" above, which is the same as what we've now officially dubbed as "SPI-BS1." - Lenses were identified to be needed after the initial measurement of the beam profile emanating from SPI-BS1. That initial beam profile measurement is cited in LHO:83956, and the lens also developed in JaMMT with the lenses that were available from the optics lab / PSL inventory. - If anyone's trying to recreate the model of the beam profile from the two measurements (LHO:83956 with no lenses, and the above LHO:83983) just note that the "zero" position is different in the quoted raw data; in LHO:83956 is the front of the rail, on Column 159 of the table, and in LHO:83983 the zero position is the SPI-BS1 reflective surface which is on Column 149 of the table, i.e. a 10 inch = 25.4 cm difference. - The real SPI-L1 installed to create this mode-shape / beam profile is labeled by its radius of curvature, which is R = 51.5 mm, and thus its focal length is more precisely f = R*2 = 103 mm. (We did find a lens that does have f = 60 mm for SPI-L2, and it's labeled by its focal length.) - "the fiber" is that which is intended for permanent use, depicted as SPI_PSL_001 in the SPI optical fiber routing diagram D2400110, a Narrow Key PM-980 Optical Fiber "patch cord" from Diamond, whose length is 30 [m]. This fiber will run all the way out to SUS-R2, eventually, to be connected as the input to the SPI Laser Prep Chassis (D2400156). - Per design, light going into this fiber is entirely p-pol, due to polarization via SPI-HWP1 and clean-up by SPI-PBS01 just upstream. We did not measure the polarization state of the light exiting the fiber. - The raw data that informs the statement that "the power transmission thru the fiber has been measured to be 83%": : We measured the input to the fiber coupler, SPI-FC1, via the S140C low-power power meter we'd been using throughout the install. The output power was measured via a fiber-coupled power meter Sina had brought with her from Stanford (dunno the make of that one). : We measured the power input to the fiber twice several hours apart (with the change in fiber input power controlled via the SPI-HWP1 / SPI-PBS01 combo)., (1) 19.9 [mW] with PMC TRANS power at 104.1 [W] at 2025-04-17 16:35 UTC (while the PMC power was in flux from enviromental controls turn on) (2) 180 [mW] with PMC TRANS power at 103.5 [W] at 2025-04-17 14:00 UTC (while the PMC power was quite stable) : We measured the output power (1') 16.6 [mW] with PMC TRANS power at 103.7 [W] at 2025-04-17 17:35 UTC (an hour later than (1)) (2') 150 [mW] with PMC TRANS power at 103.5 [W] at 2025-04-17 14:00 UTC (simultaneous to (2)) : Thus derive the transmission to be (1'') (16.6 / 19.9) * (104.1/103.7) = 0.837 = 83.7% and (2'') (150 / 180) * (103.5/103.5) = 0.833 = 83.3%
In the attachment you will find the JAMMT model for the measured beam profile of the PSL pick off with the origin a SPI-BS1, as well as the lenses used to adjust the mode of the beam for the fiber collimator FC60-SF-4-A6.2-03.
J. Kissel scribing for S. Koehlenbeck, J. Oberling, R. Short, J. Freed ECR E2400083 IIET 30642 WP 12453 Another quick summary aLOG at the end of the day, with more details to come: - With the power in the ALS/SQZ pick-off path to 10 [mW] for beam profiling, - Installed a two lens system to handle the unexpectedly different beam profile of the ALS/SQZ pick-off path - Remeasured the resulting mode after the two lens system, and we're happy enough. We're gunna call them SPI-L1 and SPI-L2. - Installed steering mirrors SPI-M1 and SPI-M2. - Rotated ALS-HWP2 to increase the s-pol light in the ALS/SQZ/SPI path to return the power transmitted through SPI-BS1 going to the ALS/SQZ fiber collimator back to 50.5 [mW]. This set the SPI path to 186 [mW] with the PMC TRANS measured at 103.5 [W]. The ALS_EXTERNAL PD in transmission of ALS-M9 measured 31 [mW] ***. - Installed SPI-HWP1 and SPI-PBS01 - Measured the power at each port of SPI-PBS01, with the intent to optimize the SPI-HWP1 position to yield maximum p-pol transmission through SPI-PBS01. *** We expect this is lower than the goal of ~45 [mW] (from LHO:83927) because we've not yet re-aligned the ALS/SQZ fiber collimator path after the install of the SPI-BS1, which translates the beam a bit due to the thickness of the beam splitter. We intend to get back to this once we're happy with the SPI path.
Small correction to above is after installing SPI-HWP1 and SPI-PBS01, we adjusted HWP1 to have 20mW in transmission of PBS1 (not maximum quite yet) to start alignment into the fiber. Using the two steering mirrors downstream of PBS1 and the collimating lens in front of the fiber, Sina maximized the transmission as measured with the output of the fiber on a spare PD. We then took power measurements of the input and output of the fiber:
This is a good start, but with a target ratio of >80%, there's still more work to be done here improving the beam into the fiber collimator. Out current mode-matching solution claims we should have 95% mode overlap into the fiber, so hopefully the issue is alignment, but it's entirely possible we'll revisit the mode-matching to see if improvements can be made there too.
The attached photo represents the optical layout as it stands as of where we stopped today, with the new SPI fiber in blue on the left (north) side of the table.
Re-post of Ryan's picture at the end of day 2, labeled with the almost entirely complete SPI pick-off path. Critically here, this shows the PSL row/column grid, confirming that this whole ECR E1900246 ALS pick-off path is 2 rows "higher" in +Y than is indicated on the current version of the as built PSL drawing D1300348-v8.
Ryan grabbed another picture I attach here. This shows the ALS pick-off path on this day in order to support the identification that the beamline between ALS-M1, through the faraday ALS-FI1 and ALS-L1, etc stopping at ALS-M2 (not pictured) is on row 25 of the PSL table *not* row 23 as drawn in D1300348-v8. I attach both the raw picture and my labeled version. So, ya, ALS-M1 should have its HR surface centered on Row 25, Col 117. Note, the grid in the picture is labeling bolt holes. Because the optical elements are all ~4 inches above the table, the beams appear offset from the way they travel on along the grid given that the photo was taken at a bit of an angle from vertical. May the future updater of D1300348 bear this in mind.
J. Kissel scribing for S. Koehlenbeck, R. Short, J. Oberling, and J. Freed ECR E2400083 IIET 30642 WP 12453 During yesterday's initial work installing the SPI pick-off path (LHO:83933), the first optic placed was SPI-BS1, the 80R/20T power beam-splitter that reflects most of the s-pol light towards the new SPI path. The pick-off is to eventually be sent into a SuK fiber collimator (60FC-SF-4-A6.2S-03), so we wanted to validate the beam profile / mode shape of this reflected beam. The without changing any power in the ALS/SQZ/SPI pick-off path, the power now reflected from newly installed SPI-BS1 measured ~40 [mW] (see LHO:83946). This is too much for the WinCam beam profiler, so they used ALS-HWP2 to rotate the polarization going into ALS-PBS01, and thus reduced the reflected s-pol light in this ALS/SQZ/SPI pick-off path to ~10 [mW]. That necessarily means there's a little more of the ~2 [W] p-pol light transmitted and going toward the HAM1 light pipe, so they placed a temporary beam dump after ALS-M2 so as to not have to think about it. The they set up a WinCam head on a rail and gathered the beam profile. With the WinCam analysis software on a computer stuck in the PSL, they simply gathered the profile information which I report here: # Distance[cm] Radius[um] Radius[um] X Y 0.0 680.5 717 17.78 465 504 25.4 389 428.5 30.48 346.5 368 38.1 281.5 300.5 where "X" is parallel to the table, and "Y" is orthogonal to the table. The "0.0" position in this measurement is the "front" of the rail (the right most position as pictured in the attachment), which is Column 159 of the PSL grid. SPI-BS1 has the center of its reflective surface is set in +/- X position in Column 149 (within the existing ALS-PBS01 to ALS-M9 beam line). It's +/- Y position is set to create a reflected beam line along Row 30 of the grid, and the WinCam head and rail are centered in +/- Y on that Row to capture that beam. Using this profile measurement, we find it to be quite different than expected from when this path was installed circa 2019 (see e.g. LHO:52381, LHO:52292, LHO:51610). Jason shared his mode matching solution from LHO:52292 with us prior to this week, and I've posted it as a comment to that aLOG, see LHO:83957. We think we can trace the issue down to an error in the as-build drawing for the PSL: - the whole beam path running in the +/-X direction from ALS-M1 to ALS-M2 is diagrammed to be on row 23 -- however, we find in reality, the path lies on row 25. That's 2 inches more between the (unlabeld) pick-off beam splitter just prior to ALS-M1 and ALS-M1 itself. Easily enough to distort a mode matching simulation. - Jason confirms that he used the *drawing* to design the lens telescope for this ALS/SQZ fiber distribution pick-off path. More on this as we work through a lens solution for the SPI path. As of this entry, we elect to NOT create a new solution for the whole ALS/SQZ fiber distribution pick-off i.e. we *won't* adjust ALS-L1 or ALS-L5 in order to fix the true problem. But, we report what we found in the event that a case is better made to help mode matching and aligning into the ALS/SQZ fiber distribution pick-off easier -- as we have verbal confirmation that it was quite a pain. For the record the fiber collimator used in the ALS/SQZ distribution pick-off is a Thor Labs F220 APC-1064.
Just a quick trend of the SM1PD1A EXTERNAL PD in transmission of ALS-M9 after they throttled the s-pol power in the ALS/SQZ/SPI path to ~10 [mW]. In that trend, you can see the different in "lights on" vs. "lights off" highlighted with the magenta vertical lines. Note, as you can see in the picture, the reflection of ALS-M9 is dumped so as to not have to think about how much power is or is not going into the ALS/SQZ fiber distribution collimator (ALS-FC2), so the INTERNAL monitor PD that's in the distribution chassis itself is "correctly" unexpectedly reading nothing, so I don't show it.
Correction to the last sentence of the main entry -- the ALS/SQZ fiber collimator is *not* an, but instead a Thorlabs Fiber Port PAF2-5A, pictured well in FinalInstall_ALSfiber.jpg from LHO:83989. I had incorrectly assumed that this collimator would be a copy of ALS-FC1, which *is* listed in E1300483 as an F220 APC-1064.
In the attachment you will find the fit with JAMMT to the measured beam profile data with offset correction:
Distance (cm) | Radius horiz. (um) | Radius vert. (um) |
17.46 | 680.5 | 717 |
35.24 | 465 | 504 |
42.86 | 389 | 428.5 |
47.94 | 346.5 | 368 |
55.56 | 281.5 | 300.5 |
Mode matching of the single bounce beam to the OMC is really bad and we don't know why. We don't even know the beam shape of the single bounce beam hitting the OMC. I constrained the beam shape by looking at the OMC scan data.
There are many OMC single bounce scans but the most recent two w/o RF SBs, one with cold and the other with hot OM2, were carefully analyzed by Jennie to resolve 02 and 20 mode as separate peaks (alogs 70502 and 71100), so I used them here.
If you just want to see the results, look at the third panel of the first attachment.
X-axis is the normalized waist position difference, Y-axis is the normalized waist radius difference. From the measured cold mode matching loss of 11.5%(!!) and hot loss of 6.2%, and the fact that the loss changed by only changing the ROC of OM2, the beam parameters hitting the OMC were constrained to two patches per each OM2 ROC. Yellow is when OM2 is cold, blue is when OM2 is hot. Arrows show how cold (yellow) patches are transformed to hot (blue) patches when OM2 ROC is changed by heating.
Note that we're talking about inconceivably huge mismatching parameters. For example, about -0.3 normalized waist position difference (left yellow patch) means that the waist of the beam is ~43cm upstream of the OMC waist. Likewise, about +0.3 normalized waist radius difference means that the beam waist radius is 690um when it should be 490um.
We cannot tell (yet) which patch is closer to reality, but in general we can say that:
There are many caveats. The first one is important. Others will have limited impact on the analysis.
Moving forward:
Here's a brief explanation of what was done.
Top left panel of the 1st attachment is the mode matching loss contour plot. loss=0 when [posDiffNormalized, sizeDiffNormalized]=[0.0]. Contours are not circular because the loss is calculated analitically, not by quadratic approximation.
Top right panel of the 1st attachment only shows the region close to the measured losses. Yelllow ring is when OM2 is cold, blue is when hot. Each and every point on these rings represent a unique waist size and waist position combination (relative to the OMC waist).
Since we are supposed to know the OMC-OM2 distance and ROC of the cold and hot OM2, you can choose any point on the yellow (cold) ring, back-propagate the beam to the upstream of OM2 (assuming the cold ROC), "heat" the OM2 by changing the ROC to the hot number, propagate it again to the OMC waist position, and see where the beam lands on the plot. If it's on the blue ring, it's consistent with the measured hot loss. If not, it's inconsistent.
Just for plotting, I chose 9 such points on the cold ring and connected them with their hot landing points on the top right panel. If you for example look at the point at ~[0, 0.4] on the plot ("beam too big but position is perfect when cold"), after heating OM2 the beam becomes smaller but the beam position doesn't change meaningfully, therefore the matching becomes better. In this case the improvement is much better than the measured (i.e the landing point is inside the blue ring), so we can conclude that this ~[0, 0.4] for cold is inconsistent with the measured hot loss.
By doing this for each and every point on the yellow ring we end up with a patch or two that are consistent with reality.
If you cannot visualize what's going on, see the 2nd attachment. Here I'm ploting the beam propagation of "beam too big but position is perfect when cold" case in the top panel. The beam between the OM2 and OMC is directly defined by the initial (cold) parameters. The beam upstream of the OM2 is back-propagation of that beam. On the bottom panel is the propagation diagram of when OM2 becomes hot. The beam upstream of OM2 is the same as the cold case. You propagate that beam to the OMC position using hot ROC. In this case the loss, which was ~12% when cold, was improved to 4.3%, that's inconsistent with the measured hot loss of (1+-0.1)*6.2%.
Further summary:
We can probably down-select the patch by 30uD single-path thermal lensing in ITM comp plate relative to the thermal lensing we had in previous scans (alogs 70502 and 71100). Start by a hot OM2. If we see a significant reduction in MM loss after ITM TCS, the actual beam parameters are on the patches in the left half plane.
Details 1:
In the 1st attachment, I took two representative points on the hot patches indicated by little green circles, which define the beam shape at the OMC waist position. I then back propagated the beam to the upstream of ITM (i.e., in this model, optics are correctly placed with correct ROC and things, but the input beam is bad). ITM is at the average ITM position. The only lensing in the ITM is the nominal diversing lens due to ITM's curvature on the HR.
Then I added the thermal lens, once to the beam impinging the ITM HR and once to the beam reflected, and see what happens to the beam parameter at the OMC waist location. These parameters are represented by tiny crosses. Blue means negative diopters (annular heating) and red means positive (central heating). I changed the thermal lensing by 10uD steps (single-path number).
As you can see, if you start from the left half plane patch, central heating will bring you close to ~(-0.04, 0) with 30uD single-path (or 60uD double-path).
OTOH if you start from the right half plane, ITM heating only makes things worse both ways.
FYI, 2nd plot shows, from the left to the right, good mode matching, hot patch in the left half plane and in the right half plane. The beam size on the ITM is ~5.3cm nominally, 5.1cm if in the left half plane (sounds plausible), 6.8cm in the right (sounds implausible). From this alone, right half plane seems almost impossible, but of course the problem might not be the bad input beam.
Details 2:
Next, I start with (almost) perfectly mode-matched beam and change the optics (either change ROC/lens or move) to see what happens. We already expect from the previous plots that ITM negative thermal lensing will bring us from perfect to the hot patch in the left half plane, but what about other optics?
3rd attachment shows twice the Gouy phase separation between ITM and other optics. Double because we're thinking about mode matching, not misalignment. As is expected, there's really no difference between ITM, SR3 and SR2. OM1 is almost the opposite of ITM (172 deg), so this is the best optic to compensate for the ITM heating, but the sign is opposite. OM2 is about -31 deg, SRM ~36 deg. From this, you can expect that SR3 and SR2 are mostly the same as ITM as actuators.
4th attachment shows a bunch of plots, each representing the change of one DOF of one optic. (One caveat is that I expected that the green circles, which repsent the beam perfectly mode matched to the arm propagated to the OMC waist position, will come very close to (0, 0) with zero MM loss, but in this model it's ~(-0.4, 0.1) with ~1.2% loss. Is this because we need a certain amount of ITM self-heating to perfectly mode match?)
Anyway, as expected, ITM, SR3, SR2 all look the same. It doesn't matter if you move the position of SR3 and SR2 or change the ROC, the trajectory of the beam parameter points on these plots are quite similar. These optics all can transform the perfectly matched system to the blue patch in the left half plane.What is kind of striking, though not surprising, is that 0.025% error in SR3 ROC seem to matter, but this also means that that particular error is easily compensated by ITM TCS.
SRM, OM1 and OM2 are different (again as expected). Somewhat interesting is that if you move OM2, the waist size only goes smaller regardless of the direction of the physical motion.
From these plot, one can conclude that if you start from perfectly matched beam, you cannot just change one optic to reach the hot patch in the right half plane. You have to make HUGE changes in multiple optics at the same time e.g. SRM ROC and ITM thermal lensing.
Both Details 1 and 2 above suggest that, regardless of what's wrong as of now (input beam or the optics ROC/position), if you apply the central heating on ITM TCS and see an improvement in the MM loss, it's more likely that the reality is more like the patches on the left, not right.
Dan pointed me to their SRC single-path Gouy phase measurement for the completely cold IFO, which was 19.5+-0.4 deg (alog 66211).
In my model, 2*Gouy(ITM-SRM single path) was ~36deg, i.e. the SRC single-path Gouy phase is about 18 degrees. Seems like they're cosistent with each other.
ITM central heating plot was updated. See attached left. Now there are four points as the "starting points" without any additional TCS corresponding to both hot and cold patches.
According to this, starting with cold OM2, if the heating diopter (single path) is [0, 10, 20, 30, 40]uD, the loss will be [11.5, 7.1, 3.5, 1.1, 0.1]% if the reality is in the left half plane (attached right, blue), or [11.5, 9.9, 10.5, 13.1, 17.3] % if in the right half plane (attached right, red).
Updated to add cold OM2, ITMY single bounce, central CO2 OFF/ON case in alog 71457.
Jennie Wright, Keita Kawabe, Sheila Dwyer
Above Keita says "I assumed that the distance between OM2 and OMC waist is as designed (~37cm). " 37 cm is a typo here, the code actually uses 97 cm, which is also the value listed for OMC waist to OM2 in T1200410