Fri Apr 18 10:09:22 2025 INFO: Fill completed in 9min 18secs
I confirmed a good fill curbside.
J. Kissel scribe for S. Koehlenbeck, J. Freed, R. Short, and guest star J. Oberling ECR E2400083 IIET 30642 WP 12453 Toward the end of day two of install (LHO:83961), the team set the power at the input of the ALS-FC2 by rotating ALS-HWP2, to be 50.5 [mW] (with PMC TRANS at 103.5 [W]). The reported power for the on-table ThorLabs SM1PD1A, however, measured consistently lower at "31 [mW]," lower than the goal for this PD, a reported power of "45 [mw]" (LHO:83927), when the power of the beam between ALS-M9 and ALS-FC2 was physically measured at 48.7 [mW] (with PMC TRANS at 103.0). We think lower reported power on the PD is related to (1) The slight translation of the what-used-to-be ALS-L5 to ALS-M9 beam, because of the thickness of the SPI-BS1 that was inserted into that path, and (2) a change in the amount of s- and p- polarization in reflection of the ALS-PBS01 after rotating ALS-HWP2 to increase the power in the ALS/SQZ/SPI path, because the polarization state of the reflection of a PBS can be power dependent. To support (2), we measured the polarization today between ALS-M9 and ALS-FC2 with a temporary PBS and power meter. On 2025-04-17 at 19:02 UTC with PMC power at 103.7 [W], we measure s-pol = 49.7 [mW] p-pol = 1.8 [mW] (total = 49.7 + 1.8 = 51.5 [mW]) Regrettably, we did not measure this polarization state prior to changing anything. However, because we've *measured* equal total power at ALS-FC2 before vs. after, we're confident that at least the total power going into ALS-FC2 is the same. As such, we called in Jason to help couple the beam into ALS-FC2 using ALS-M9 and what alignment screws are on ALS-FC2 itself. Attached is the trend of that process, where we used the SPI distribution chassis PD in two forms: H1:ALS-C_FIBR_INTERNAL_DC_POWER never calibrated version, used to be 0.1 [cts] H1:ALS-C_FIBR_INTERNAL_DC_POWERMON version we'd been using, calibrated into [mW] In the end, we landed with the values of these channels at H1:ALS-C_FIBR_INTERNAL_DC_POWER 0.1 [cts] H1:ALS-C_FIBR_INTERNAL_DC_POWERMON 31.4 [mW] which matches our goals from LHO:83927. The team also adjusted the position of the SM1PD1A in transmission of ALS-M9 to account for (1). However, even after moving the PD out of maximum and back, they were not able to find any position where the PD readout exceeded H1:ALS-C_FIBR_EXTERNAL_DC_POWERMON 31.0 [mW] This why we expect that something more like (2) is going on. Though we looked through - E1300483 (doesn't list ALS-M9), - E1900246 (calls the optic ALS-M6, which is not for 1064 nm in E1300483), - E0900325 (isn't new enough to have this mirror), - Peter King's purchase orders circa 2019 (Req 122638553 for the fiber collimator parts, and Req 122583017 for the SM1PD1A parts) we couldn't find anything that was clearly and obviously the ALS-M9 optic, so we can't validate or reconstruction the reflectivity in each polarization to model the factor of 31 [mW] / 45 [mW] = 0.7x (or 30% drop) reported value change. In any event, this EXTERNAL PD channel will need to be recalibrated to better reflect the real power in this path. Also, when we re-start up anything that uses the output of the ALS / SQZ fiber distribution, it may need to be adjusted to account for the polarization change described in (2)
TITLE: 04/18 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: 5mph Gusts, 2mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.17 μm/s
QUICK SUMMARY:
The Vacuum team had pumped down to about 2 .7 torr.
There is some effort to clean up staging areas and put some things back into storage.
Sounds like it will be a quiet day around here.
Roughing pumps are being turned back on to get us down to 1 torr so we can get the Turbo pumps running!
4-17 (Thursday) activities: - The corner pumpdown continued, we are at ~3 Torr now, today the pumping was on for 12 hours. The pumping speed is still at (~1900 l/min). Tomorrow 5-6 more hours are needed before switching on the turbos - A wide-range gauge (compatible with the supersucker cart) on a tee and along with a pumpdown port was installed on the freshly installed HAM6 turbo - The HAM6 turbo was then started up - as it was its initial test -, and keeps running, ready to be valved in tomorrow - The BSC8 annulus Ion pump is still suffering (~8E-6 Torr), but the pressure is slowly coming down - The HAM4 annulus system has been taken care of, after switching off the Ion pump last week, now the volume is being pumped with an aux cart - The GV5 annulus system is still being pumped by an aux cart, with the Ion pump switched off - The leak checking was continued, all the CF flanges on the Y-manifold were leak checked: Y+ side (6 pcs.); Turbo flange (1 pc.); vent valve (1 pc.); Varian valve (1 pc., see more info at aLog 83951 - after all, it seems that it is only an internal leak). All flanges were found leak-tight.
M. Todd, C. Compton, S. Dwyer
Over the past few weeks I've been trying to understand what we can learn from some of the ETMY ring heater power changes that we've made over the past 9 months or so. By looking at the Higher Order Mode spacing from OMC data as well as substrate lensing from the HWS data, we hope to be able to make some models or estimates of the coupling factors of the different actuators to substrate and surface defocus.
In particular, we want to use the HOM spacing to estimate how much of the surface defocus comes from self heating.
This derivation is better illustrated in the attachment below, which has a neater write up of the following logic:
1) Known values : HOM spacing, FSR, Cold-State Surface Curvature, Ring Heater Power, Coupling Factor of Ring Heater Power to Surface Defocus, g-factor of the ITM and ETM
2) Desired values: Surface Defocus from Self-heating (coupling * absorbed power)
Through solving some of the equations relating these values, with the assumption that our coupling factors are correct, we estimate the self-heating to change the surface curvature by about 13%.
TITLE: 04/17 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
The Vacuum team has been hard as work removing the air from the corner station. We seem to be below 20 torr.
The SPI team has Finished putting in their pickoff inside the PSL.
The SEI team workin on HAM1 still has more work to do.
SUS team has been cleaning optics in the Mega chamber as well
Also:
19:30 Hanford site called the LHO control room to let us know that they were performing a Take Cover Drill. The Operator Core decided to go over the protocol for shutting off the HVAC system in the case that this was not a drill.
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
14:45 | FAC | Nellie & Kim | LVEA | NO | Technical Cleaning | 16:45 |
15:27 | VAC | Jordan | LVEA | N | Resuming pumpdown | 16:03 |
15:35 | FAC | Tyler | LVEA | N | Putting compass stickers on cranes | 16:47 |
15:44 | Plant Study | H Miss. cont | Mid X | N | Studying plants? | 17:11 |
15:47 | PCAL | Tony | PCAL | Yes | Transfer standard PCAL measurement | 15:57 |
15:58 | SEI | Jim | LVEA Racks | n | checking ADC cabling | 19:28 |
16:01 | FAC | Randy & Mitchel | LVEA | N | Moving equipment & machines Started ~16:09 | 18:35 |
16:10 | CDS | Dave B | Remote | N | Model & DAQ restart | 16:19 |
16:12 | SPI | Sina & Ryan S | LVEA | Yes | Installing SPI Pickoff | 19:16 |
16:13 | EE | Daniel | LVEA racks | N | Running Cabling | 21:01 |
16:14 | EE | Marc | LVEA | N | Running Cables with Daniel | 23:24 |
16:17 | SEI | Jim | LVEA HAM1 | N | Working on in air side feed throughs on HAM1 | 16:20 |
16:19 | SPI | Josh | Optics Lab & PSL | Yes | Working on Optics for SPI With Escort Jeff. | 19:16 |
16:48 | EE | Fil | LVEA | N | Cabling for HAM1 with Daniel & Marc | 23:24 |
17:02 | FAC | Kim | LVEA | n | Vacuuming in MSR | 17:32 |
17:04 | PSL | Jason | PSL | Yes | Helping out with SPI | 18:56 |
17:22 | SUS | Rahul & Ryan C | LVEA HAM6-7 | N | First contact of triple suspensions. | 18:14 |
18:09 | VAC | Janos & Jordan | HAM6 area | N | Checking Guages and Valves | 20:24 |
18:42 | Sun | Ryan C | Y arm | n | Taking a walk down Y arm. | 19:15 |
18:46 | HAM1 | Camilla | LVEA | N | Retreiving Parts. | 18:53 |
19:38 | OPS | Tony, Ibrahim, Ryan C, Oli, TJ, Ryan S, Eric | Mechanical Room | N | Hanford Radiation Emergency Drill Respons | 19:39 |
20:25 | VAC | Jordan | LVEA HAM4 | N | Setting up pump on HAM4 Annulus & Cap Inventory Checks | 22:28 |
20:39 | SPI | Ryan S, Sina, Josh | PSL | Yes | Installing SPI Pickoff | 22:00 |
20:54 | VAC | Travis & Janos | HAM4 Area | N | Vacuum pump activities | 21:59 |
21:02 | SUS | Rahul, Ryan C | LVEA HAM6 | N | cleaning Tripple SUS optics. | 22:14 |
21:07 | Saftey | Richard | LVEA | N | Safety checks | 21:24 |
21:29 | SEI | Jim | LVEA HAM1 | N | Restarting HAM 1 SEI Systems | 22:28 |
22:00 | Prop | Travis | End X &Y | N | Property inventory | 22:37 |
22:14 | SEI | Jim | CER | N | Checking SEI Config | 00:14 |
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
Still on schedule! Currently in the Stand-down in HAM1 such that the corner pump down can get to a more exercised safe state. Attached is a snapshot of what is planned for the next few days. (Things un-checked on today's list are expected to continue early next week per plan.)
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.
FAMIS 27813
HEPI trends for the last month.
The sudden drop in the HEPI trends happened on the same day at the same time as the Power outage .
The last week can be see here and looks good except for today which show multiple DAQ restarts.
Brian, Oli, Edgard
Testing the implementation of the OSEM estimator installed on SR3. The models were installed on Monday. We don't have the model transfer functions yet. We were testing the basic OSEM path and the switch. We were testing SR3 YAW. It all looks good so far - the OSEM signal is getting to where it should be, and fader-switch is working correctly.
-- detailed testing notes --
ISI is damped. vacuum is still pumping pressure is ~16 torr. Looks like the suspension is still moving because of temperature changes so we can't do useful TFs yet.
GPS time 14289 57082
Look at the drive level of the classic damper, the pk-pk with normal damping is about -0.04 to +0.04
channels all start with H1:SUS-SR3_
Look at channels: M1_YAW_DAMP_EST_OUTPUT, M1_YAM_DAMP_OSEM_OUTPUT, M1_YAW_DAMP_SIGMON, M1_DAMP_Y_OUTPUT, M1_DAMP_Y_IN1
Y osem damper gain is -0.5 instead of -1.0. Gabriele changed this.
Test 1 - are the OSEM signals getting to the OSEM path, and is the damper control set correctly? - YES!
Set the YAW_DAMP_OSEM filter bank to be the same at the DAMP_Y bank
The output switch for the estimator is OFF - so the OUTPUT signal from the YAW_DAMP_OSEM filter does not get to the osem drives
Output signals of the 2 damping controllers should be the same - and they do look the same. Put them on top of each other and they seem identical
Test 2 - use the classic damping and the YAW_OSEM path, does it work? - Yes!
1. set the YAM_DAMP_OSEM gain to -0.4 (from -0.5)
2. set the classic damping gain to -0.1 (from -0.5) (so 20% of the gain is in the classic path, 80% in the estimator path)
gps time ~...58716, Turn on the estimator. This should recover the previous normal damping.
Switch looks smooth - no glitching, no drama. comes on well
The drive levels look like 4 to 1 by eye (correct). total drive looks about the same as before.
Turn off estim path at ...58900 ish. OSEM input signal doesn't look any different (gah, really?!, of course not, it's all sensor noise)
Test 2 successful - switch seems smooth, damping paths look good
Test 3 - test the switch between OSEM path and Estimator path - is it smooth and well behaved? - YES!
Set Estim damping control to be the same as the OSEM damping control.
Set the OSEM Bandpass to 1 so OSEM_DAMPER and ESTIM_DAMPER inputs should match (they do) and the outputs should match (they do).
these three signals should all be the same now during the switch from OSEM to Estim
M1_YAW_DAMP_SIGMON (this is the switch output)
M1_YAW_DAMP_OSEM_OUTPUT (first input)
M1_YAW_DAMP_EST_OUTPUT (second input)
start around 59720 -
then switch back and forth several times - these signals all stay on top of each other and are indistinguishable.
GPS is about ...60100
Zoom in for a close look at the start and stop of the fade to look for glitching - I don't see any, see plot in comment.
Test3 - success - by eye we can no see any difference in the 3 channels.
In 82097 we got some constraint on the circulating power in the arm from the squeezer data set. I'm working on looking at the data that Camilla took in 83660, and realize that with the higher nonlinear gain the frequency independent squeezing gives us a better constraint on the arm power.
Using known injection losses of 8.2%(google sheet), and 6% extra HAM7 losses from 83070 gives 13.7% minimum injection losses for squeezing, and our known readout losses are 8.4%. Based on 16.1dB of anti squeezing (for NLG of 19 as reported by Camilla) and -4.97 dB squeezing, the infered NLG is 18.7 and the total sqz efficiency is 0.694 (with 0 phase noise). This means that in addition to the 6% extra losses measured on the homodyne, we have another 12% unknown squeezer losses. We can assign those 12.2% losses to either injection losses (unlikely since there isn't much between homodyne pick off point and injection into the OFI), readout losses that also impact the IFO readout, or squeezer readout losses that don't impact the IFO (SQZ to OMC mode matching).
If the only IFO readout losses are the known losses, the IFO readout efficiency is 91.6%, and we can use the shot noise level without squeezing injected to estimate that the minimum arm power is 310kW. Using the total squeezer efficiency and the known losses, we can place bounds on the readout efficiency between 80.4% and 91.6%. The level of shot noise measured without squeezing mostly depends on arm power and readout efficiency, so this maximum readout efficiency gives us a minimum arm power of 310kW (all squeezer losses are injection losses, readout efficiency is 91.6% and arm power is minimum), while the minimum readout efficiency gives us 353kW (all unknown squeezer losses are common to IFO, which probably wouldn't be the case for mode mismatches).
Ryan C, Rahul
L1BHDM1 which is the suspended configuration of HRTS (HAM Relay Triple Suspension) for O5 is now ready to be shipped to LLO (using ground freight). The suspension (all stages locked with EQ stops, torqued double nuts and tension removed from wires ) has been wrapped in several layers of clean foil/clean cloth and clean bag as shown here.
This shipment is expected to reach LLO sometime at the end of next week (25th April), if it leaves LHO today. The details of the shipment are given below,
Tracking Site Link: https://www.shipdbi.com/ HWB Number for TRK: 139289
FRS ticket - https://services1.ligo-la.caltech.edu/FRS/show_bug.cgi?id=33849
ICS (assembly record) - https://ics.ligo-la.caltech.edu/JIRA/browse/ASSY-D1900449-L1BHDM1
ICS (shipment load) - https://ics.ligo-la.caltech.edu/JIRA/browse/Shipment-13842
This is first of the total six HRTS which will be transported to LLO.
Jim, Tony, Dave:
We restarted h1isiham1 model four times and the DAQ twice:
1. Internal wiring change to model, no DAQ retstart for that but new common part with "missing ADC chans" fix was included which did require a DAQ restart. No issues with DAQ restart other than gds0 needed a second restart.
2. A copy-paste binary parts issue was found, HAM6 parts were included in HAM1. BIO parts were renamed, no DAQ restart was neeed.
3. HAM1 differs from HAM6 in BIO inputs in that it reads 64 input channels instead of just 32. Upper32 channel BIO part was added, which added slow channels, so DAQ restart was required. No issues with DAQ restart other than gds0 second restart.
4. To minimize binary chassis hardware, HAM1 and HAM6 share the first BIO card's binary output chassis, HAM6 uses lower 32 chans, HAM1 uses upper 32 chans. h1isimodel was changed to use BIO-0 U32 for outputs. No DAQ restart was required.
Current BIO hardware as see by models:
wiring | input block | model | model | output block | wiring | |
from ham6 | BIO-0 low 32 | h1isiham6 | h1isiham6 | BIO-0 low 32 | to ham6 | |
not connected | BIO-0 high 32 | none | h1isiham1 | BIO-0 high 32 | to ham1 | |
from ham1 | BIO-1 low 32 | h1isiham1 | none | BIO-1 low 32 | no chassis | |
from ham1 | BIO-1 high 32 | h1isiham1 | none | BIO-1 high 32 | no chassis |
DAQ Changes
1st DAQ restart (correct missing ADC chans)
++: slow channel H1:ISI-HAM1_PMON_GS13_P3_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_GS13_P2_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_GS13_P1_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_GS13_D3_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_GS13_D2_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_GS13_D1_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_FF_L4C_P3_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_FF_L4C_P2_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_FF_L4C_P1_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_FF_L4C_D3_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_FF_L4C_D2_CTS added to the DAQ
++: slow channel H1:ISI-HAM1_PMON_FF_L4C_D1_CTS added to the DAQ
2nd DAQ restart (read H32 BIO-1 channels)
++: slow channel H1:ISI-HAM1_BIO_IN_GAIN_L4C_H1_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_GAIN_L4C_H2_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_GAIN_L4C_H3_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_GAIN_L4C_V1_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_GAIN_L4C_V2_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_GAIN_L4C_V3_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_INMON2 added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_TEST2 added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_TESTMON2 added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_WHT_L4C_H1_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_WHT_L4C_H2_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_WHT_L4C_H3_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_WHT_L4C_V1_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_WHT_L4C_V2_RB added to the DAQ
++: slow channel H1:ISI-HAM1_BIO_IN_WHT_L4C_V3_RB added to the DAQ
Thu17Apr2025
LOC TIME HOSTNAME MODEL/REBOOT
09:09:41 h1seih16 h1isiham1 <<< model restart, fix wiring, add missing-adc-chans
09:12:10 h1daqdc0 [DAQ] <<< 0-leg
09:12:20 h1daqfw0 [DAQ]
09:12:21 h1daqtw0 [DAQ]
09:12:22 h1daqnds0 [DAQ]
09:12:29 h1daqgds0 [DAQ]
09:13:19 h1daqgds0 [DAQ] <<< 2nd gds0 restart
09:16:23 h1daqdc1 [DAQ]
09:16:33 h1daqfw1 [DAQ] <<< 1-lde
09:16:34 h1daqtw1 [DAQ]
09:16:35 h1daqnds1 [DAQ]
09:16:44 h1daqgds1 [DAQ]
10:10:21 h1seih16 h1isiham1 <<< model restart, change bio address
10:27:28 h1seih16 h1isiham1 <<< model restart, add BIO-1 H32
10:32:12 h1daqdc0 [DAQ] <<< 0-leg
10:32:23 h1daqfw0 [DAQ]
10:32:24 h1daqtw0 [DAQ]
10:32:26 h1daqnds0 [DAQ]
10:32:32 h1daqgds0 [DAQ]
10:35:28 h1daqgds0 [DAQ] <<< 2nd gds0 restart
10:36:21 h1daqdc1 [DAQ] <<< 1-leg
10:36:32 h1daqfw1 [DAQ]
10:36:32 h1daqtw1 [DAQ]
10:36:34 h1daqnds1 [DAQ]
10:36:42 h1daqgds1 [DAQ]
10:57:48 h1seih16 h1isiham1 <<< model restart, drive BIO-0 H32
Two more h1isiham1 model restarts, the first with an associated DAQ restart.
14:35 h1isiham1 binary output block was upgraded, adding slow channels to the DAQ. During DAQ restart gds0 and gds1 needed second restarts.
15:53 h1isiham1 input bus selector to binary output block was corrected, no DAQ restart needed.
14:35:41 h1seih16 h1isiham1 <<< new binary output block
14:37:30 h1daqdc0 [DAQ] << 0leg
14:37:40 h1daqfw0 [DAQ]
14:37:40 h1daqtw0 [DAQ]
14:37:41 h1daqnds0 [DAQ]
14:37:48 h1daqgds0 [DAQ]
14:38:22 h1daqgds0 [DAQ] <<< 2nd gds0 restart
14:41:43 h1daqdc1 [DAQ] <<< 1leg
14:41:54 h1daqfw1 [DAQ]
14:41:54 h1daqtw1 [DAQ]
14:41:55 h1daqnds1 [DAQ]
14:42:03 h1daqgds1 [DAQ]
14:43:00 h1daqgds1 [DAQ] <<< 2nd gds1 restart
15:53:57 h1seih16 h1isiham1 <<< correct input bus of binary output block
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 |
Edgard, Oli
In 83662 it was discussed that the osem compensating filter z:p = 10:0.4 wasn't as accurate as it should be. Jeff worked out that the zero and pole from the satamp are 0.3835 Hz and 10.6103 Hz, respectively, so our compensating filter should be the opposite of that, with a zero at 10.6 Hz and a pole at 0.38 Hz.
Today we updated those filters for PR3 and SR3. They appear in all three stages in the initial OSEMINF filter bank (FM1) (H1:SUS-PR3_M{1,2,3}_OSEMINF_{sensor}) as well as in all three stages of the watchdog bandpass filter bank (FM6) (H1:SUS-PR3_M{1,2,3}_WD_OSEMAC_BANDLIM_{sensor}). So where before those filters there were 10:0.4, they now read 10.6:0.38 and have these updated zero and pole values. We've loaded in the coefficient changes.
I've attached the script that we used to update these filters below. It's an edit of Jeff's script in 80189
Edgard, Oli, Brian
Checking on the sat amp compensation filter change from 10:0.4 to 10.6:0.38, we noticed that it has the net effect of decreasing the OSEM signal with respect to before the change [see first attachement].
The compensation would make the OSEM corrections from 83605 about 5-6% larger, which we can estimate by looking at the ratio between the new compensation filter and the old compensation filter. [see second attachment].