[Jennie, Elenna, Oli, Keita, MattT, Jenne]
One of our locklosses this afternoon happens to have been while the OMC DCPD whitening was switching (reason is under separate investigation). It happens that the gains we use for these now are the A0 and B0 gains, in filter banks on the IOPOMC0 model, not the OMC model. The IOPOMC0 model is not part of the SDF revert process (probably because we never thought to add it in?). This means that upon relock, the OMC guardian was confused when it was asked to do the SET_WHITENING state and it found that the gains were 0 or 2, not 1 and 1.
The OMC guardian's DOWN state had an old comment (from before the omc0 days) where we explicitly set DCPD_A_GAIN and DCPD_B_GAIN both to 1, in case we lose lock during a whitening switch. For now (and in case we decide we don't want to add IOPOMC0 to the sdf revert list) I've added lines to also set DCPD_A0_GAIN and DCPD_B0_GAIN both to 1. Hopefully we won't get stuck on this small little piece again, and can get back to figuring out our bigger locking issues.
[Fil, Jonathan, Ej, Erik]
Two previously unused pairs of optical fiber between EY and the Corner station were extended from patch panels to the computer racks in EY and the MSR.
Two computers were setup on either end to test Ethernet throughput and reliability, lr-eth-c in the MSR and lr-eth-e and EY. Each computer had a Intel e810 with 100g SFP and an NVidia Mellanox with 25g/10g SFP.
The first pair tested did not produce a link light.
The second pair was able to push 80g on the Intel card and 25g on the NVidia card, with no lost data but with a low rate of correctable errors on the EY card.
In an attempt to lower that error rate, we swapped the extension fiber at EY from the first (failed) fiber pair to the second, and cleaned it multiple times. This in fact raised the correctable error rate, but it's still operating with no data losses.
TITLE: 10/28 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
INCOMING OPERATOR: Oli
SHIFT SUMMARY: Maintenance day today. Recovery has been troubling so far, we can get up to OMC_WHITENING but then lose lock. It will get to that point without issue, but then a quick 9Hz ringup in DARM will show up. I;ve attached a printout of the Trello of activities today, but none are glaring causes for something like this. The control room is currently looking into many possibilities and following up from 60W input with misaligned IM4, ISS injections today, and other activities.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 14:36 | FAC | Randy | Xarm | n | BTE sealing | 21:59 |
| 15:15 | FAC | Kim | EX | n | Tech clean | 16:36 |
| 15:15 | FAC | Nellie | EY | n | Tech clean | 16:26 |
| 15:16 | CDS | Fil, Erik | EY | n | RFM test | 19:02 |
| 15:17 | VAC | Gerardo | LVEA | n | CP1 fill line connect | 18:45 |
| 15:20 | FAC | Eric | site | n | Fire pump tests | 15:40 |
| 15:22 | VAC | Jordan | LVEA | n | Help at CP1 line then HAM4 AIP troubleshooting | 17:25 |
| 15:28 | FAC | Tyler | LVEA, VEAs | n | 3IFO checks | 17:14 |
| 15:30 | FAC | Chris | MX | n | Tractor clearing tumbleweeds | 17:35 |
| 15:33 | SUS | Jeff | CR | n | PRM meas. | 19:03 |
| 15:54 | VAC | Janos | EX, MX | n | Pump tests | 18:43 |
| 15:58 | SYS | Mitchell | LVEA | n | Parts hunt | 16:11 |
| 16:05 | PSL | Jason | CR | n | Ref cav tweak | 16:06 |
| 16:16 | SAF | Safety tour | EX, EY | n | Safety walkthrough | 18:03 |
| 16:20 | PEM | Ryan S | CR/LVEA | n | Magnetic injections | 18:47 |
| 16:20 | VAC | Norco | EX, MX | n | LN2 fill | 18:47 |
| 16:37 | FAC | Kim | LVEA | n | Tech clean | 18:05 |
| 16:45 | IO | Keita, Rahul | Opt Lab | LOCAL | ISS array | 18:58 |
| 16:45 | FAC | Nellie | LVEA | n | Tech clean | 18:04 |
| 16:52 | SEI | Jim | Remote | n | HAM6 HEPI FF injections | 18:15 |
| 17:35 | FAC | Benton PUD | Yarm | n | Grabbing equipment at transformer \ | 17:55 |
| 17:35 | FAC | Chris | Outbuildings | n | FAMIS checks | 18:26 |
| 18:04 | SAF | Safety tour | LVEA | n | Safety walkthrough | 18:30 |
| 18:13 | PCAL | Rick | PCAL lab | local | Grabbing blues | 18:15 |
| 18:31 | SAF | Safety tour | X1 BTE | n | Check on cracks, splaying of BTE | 19:16 |
| 18:42 | VAC | Jordan, Anna | LVEA | N | Join Gerardo CP1 | 18:59 |
| 18:53 | TCS | TJ | LVEA | n | Turn TCS CO2s back on | 18:54 |
| 18:54 | CDS | Marc | LVEA | n | Wrapping up cable pulling HAM3/2 | 18:57 |
| 18:55 | - | Ryan C | LVEA | n | Sweep | 19:05 |
| 19:38 | PCAL | Rick | PCAL lab | local | Parts | 19:52 |
| 20:34 | SPI | Corey, Ryan S | Opt Lab | n | Optics cleaning | 22:47 |
| 20:51 | SUS | Rahul | Opt Lab | LOCAL | Parts | 22:06 |
| 21:04 | TCS | Matt | Prep lab | n | Building racks | 22:57 |
| 21:43 | IO | Keita | Opt Lab | LOCAL | ISS array | 22:46 |
| 21:45 | SAF | Safety tour | FCES | n | Safety walkthrough | 22:06 |
| 22:30 | VAC | Gerardo | LVEA | n | Grab a cube for a cart | 22:35 |
| 22:57 | PEM | Ryan C | Opt Lab | n | Setup dust monitor | 23:07 |
TITLE: 10/28 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 12mph Gusts, 7mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.28 μm/s
QUICK SUMMARY:
Attempting to relock again and trying to figure out why we just had two locklosses directly after CLOSE_BEAM_DIVERTERS/start of OMC_WHITENING.
00:29UTC Back to Observing
Round 2 of testing the guardianization of turning on and off the high ASC gains (Round 1 - alog87462). SEI_ENV will now automatically move us into the high gain ASC state when a.) we are in the earthquake state b.) there is an incoming or ongoing earthquake that is at or below the dotted line on the "rasta plot". The transition takes 11 seconds to complete, and it will transition back when the ground motion is low enough to bring us out earthquake state.
I started testing with a few 10 and 5 second waits between steps, just as is done in the script that we currently use. Once those ran successfully a few times I started to decrease the wait times between steps. Eventually, I had success transitioning all the ASC at the same time, then the FF 10 seconds after. since this was the same configuration that I had last time I tried this, tried to reporduce the lock loss by requesting the High ASC state, then immediately requesting the Low ASC state. This did, again, cause a lock loss. To avoid this I have a wait timer in the High state so it won't switch quickly from one to the other.
Transitioning back out of the high ASC state has the same thresholds as the earthquake state currently. We didn't want to transition back and then have to do it all over again, or wait in earthquake for another 10 minutes for it to calm down. We might make this a bit shorter or smarter after we've seen it work a few times.
| Time (hhmmss UTC) | Transition to | Notes |
| 150251 | High | 10/5s timers |
| 150457 | Low | 10/5s timers |
| 150616 | High | Repeat of above |
| 150724 | Low | Repeat of above |
| 150754 | High | 1/5s timers |
| 150930 | Low | 1/5s timers |
| 151113 | High | All ASC engaged at once |
| 151218 | Low | All ASC engaged at once |
| 151326 | High | All ASC engaged at once |
| 151340 | Low | Lock loss |
I forgot that this would eventually trigger IFO_NOTIFY if the high gain state were to keep us out of Observing for longer than 10 minutes while IFO_NOTIFY was running. I've changed IFO_NOTIFY to not notify when the SEI_ENV node is in the high asc or transition states.
J. Kissel
Gathered H1SUSPRM M3, M2, and M1 Drive to M1 Response TFs to inform the "drive" models for a future H1SUSPRM estimator. I'll post the locations / file names in the comments. Here in the main entry, I discuss the state of the control system for H1 SUS PRM so we understand with how much salt would should take these measurements.
Executive summary :: there are some side quests we can launch -- especially on the actuation side of this suspension -- if we think that these measurements reveal "way too much cross coupling for an estimator to work." The first things I'd attack would be
- the frequency-dependent and scalar gain differences *between* the nominal low noise state of the coil drivers and the state we need to characterize the suspension.
- the very old coil balancing, which was done *without* first compensating for any frequency-dependent gain differences in the channels at the frequency used to balance the coils (see LHO:9453 for measurement technique.)
Here's the detailed summary of all the relevant things for these measurements:
- The suspension was ALIGNED, with alignment offsets ON, with slider values (P,Y) = (-1629.783, -59.868) ["urad"]
:: ALIGNED is needed (rather than just DAMPED [where the alignment sliders are OFF] or MISALIGNED where extra large alignment offsets are ON; per discussion of how the alignment impacts the calibration in LHO:87102)
:: the usual caveats about the slider calibration, which is still using the [DAC ct / "urad"] gains from LHO:4563).
- The M1 damping loop were converted to Level 2.0 loop shaping in Jan 2023; LHO:66859, nominally designed to have an EPICs gain of -1.0. However in Aug 2023, the EPICs gains were lowered to -0.5, and have been that way for most of O4, and remain that way now. For all of these measurements, I set the L, P and Y gains to -0.1; the "20% of nominal" gain mantra we've used for the HLTS estimators. I also gathered *almost* all the measurements again with only the Y gain at -0.1, but ran out of time to complete that set for comparison.
- Even though it was maintenance day, when we typically turn site-wide sensor correction OFF, I manually turned ON sensor correction for ISI HAM2 to get better coherence below 1 Hz (using instructions in LHO:87790)
- The M3 L to M3 P filter (and gain) in the M3 DRIVEALIGN frequency-dependent matrix is OFF, per LHO:87523.
- There are (M3 P to M3 L) = 1.7 and (M3 Y to M3 L) = 0.52 scalar gains ON in to off-diagonal elements of the M3 DRIVEALIGN matrix whose purpose is change the center of P and Y actuation to be around where the IFO's beam spot typically is.
- There is a set of M1 L to M1 P filters, "M1L_M3P" and "invM1P_M3P," in the M1 DRIVEALIGN matrix, with a EPICs gain of -1. I think these came from LHO:42549. The measurements I took aren't impacted by this, as I drove from the M1 TEST bank which does not send excitation through the DRIVEALIGN Matrix. HOWEVER, we'll definitely need to consider this when we model the ISC drive which *does* go through the M1 DRIVEALIGN matrix.
- All M1, M2, and M3 stages of OSEM PDs sat amp whitening filters have been upgraded with ECR E2400330's filter design, and compensated accordingly.
:: M1 stage LHO:85463
:: M2 & M3 stages LHO:87103
- All M1, M2, and M3 stages of OSEM PDs have been calibrated via the ISI GS13s, and calibrated in the ALIGNED state (LHO:87231)
- In order to get decent coherence over the band of interest for the M3, M2, and M1 drives, I had to drive the suspension actuators in their highest range state, which is different from the state the IFO usually needs.
:: M1 = State 1 "LP OFF" (a Triple TOP Driver)
:: M2 = State 2 "Acq ON, LP OFF" (An ECR E1400369 Triple Acquisition Driver "TACQ" modified for an extra 10x actuation strength. Modified in Sep 2013 LHO:7630)
:: M3 = State 2 "Acq ON, LP OFF" (An ECR E1400369 Triple Acquisition Driver "TACQ" modified for an extra 10x actuation strength. Modified in Sep 2014 LHO:13956)
:: The nominal state for the switches are M1 = State 2 "LP ON," M2 = M3 = State 3 "ACQ OFF, LP ON."
- No actuator channels have had any precise compensation for their coil driver's frequency response in any state.
:: M1 state 1 channels are all compensated with (z:p) = (0.9 : 30.9996) Hz
:: M2 state 2 channels are all compensated with (z:p) = (64.9966 : 13) Hz
:: M3 state 2 channels are all compensated with (z:p) = (64.9966 : 13) Hz
- There are scalar "coil balancing" non-unity magnitude gains on each of the M2 and M3 stage channels, but it's the same values that have been in play since Jan 2014 (LHO:9419; so, after the M2 TACQ driver mod, but before the M3 TACQ driver mod). There is no coil balancing gains on the M1 stage, they're all either +/- 1.0.
Here's the complete data set with L, P, and Y damping loop gains set to -0.1, with the T, V, and R gains at -0.5.
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PRM/SAGM1/Data/
2025-10-28_H1SUSPRM_M1toM1_CDState1_M1LPYDampingGain0p1_WhiteNoise_L_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M1toM1_CDState1_M1LPYDampingGain0p1_WhiteNoise_P_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M1toM1_CDState1_M1LPYDampingGain0p1_WhiteNoise_R_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M1toM1_CDState1_M1LPYDampingGain0p1_WhiteNoise_T_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M1toM1_CDState1_M1LPYDampingGain0p1_WhiteNoise_V_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M1toM1_CDState1_M1LPYDampingGain0p1_WhiteNoise_Y_0p02to50Hz.xml
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PRM/SAGM2/Data/
2025-10-28_H1SUSPRM_M2toM1_CDState2_M1LPYDampingGain0p1_WhiteNoise_L_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M2toM1_CDState2_M1LPYDampingGain0p1_WhiteNoise_P_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M2toM1_CDState2_M1LPYDampingGain0p1_WhiteNoise_Y_0p02to50Hz.xml
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PRM/SAGM3/Data/
2025-10-28_H1SUSPRM_M3toM1_CDState2_M1LPYDampingGain0p1_WhiteNoise_L_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M3toM1_CDState2_M1LPYDampingGain0p1_WhiteNoise_P_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M3toM1_CDState2_M1LPYDampingGain0p1_WhiteNoise_Y_0p02to50Hz.xml
Here's the almost entirely complete data set for *only* the Y damping loop gain set to -0.1, and L, T, V, R, P set to -0.5.
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PRM/SAGM1/Data/
2025-10-28_H1SUSPRM_M1toM1_CDState1_M1YawDampingGain0p1_WhiteNoise_L_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M1toM1_CDState1_M1YawDampingGain0p1_WhiteNoise_T_0p02to50Hz.xml
[did not get V]
[did not get R]
[did not get P]
[did not get Y]
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PRM/SAGM2/Data/
2025-10-28_H1SUSPRM_M2toM1_CDState2_M1YawDampingGain0p1_WhiteNoise_L_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M2toM1_CDState2_M1YawDampingGain0p1_WhiteNoise_P_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M2toM1_CDState2_M1YawDampingGain0p1_WhiteNoise_Y_0p02to50Hz.xml
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PRM/SAGM3/Data/
2025-10-28_H1SUSPRM_M3toM1_CDState2_M1YawDampingGain0p1_WhiteNoise_L_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M3toM1_CDState2_M1YawDampingGain0p1_WhiteNoise_P_0p02to50Hz.xml
2025-10-28_H1SUSPRM_M3toM1_CDState2_M1YawDampingGain0p1_WhiteNoise_Y_0p02to50Hz.xml
Took some more of the meaurements for PRM estimator here: 87950
Those four M1 to M1 with DAMP Y at 20% for V R P and Y are still needed
Here's the list of estimator measurements for PRM: 88063
The laser power guardian change 87603 is now in and loaded, so that we will use IM4 trans instead of IMC input request.
We should expect this to change the gain of LSC and ASC loops by 9% compared to earlier in the week, and 3% increase compared to before the power outage.
Bi-Weekly ISC Locking Histograms.
I turned this into a 1 click button to make these plots: Sitemap-> OPS-> WEEKLIES-> ISC Histograms.
Once it runs (should only take about 15 seconds) the terminal tells you where to find the plots, just upload the plots into your alog.
We run the Prep_for_Locking state before SDF_Revert, and Sheila and others have wondered how much of that state gets reverted during SDF_Revert. Not a huge amount, but we might want to consider changing these to work more cohesively.
Related: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=87729
We disconnected everything from the ISS array installation spare unit S1202965 and stored it in the ISS array cabinet in the vac prep area next to the OSB optics lab. See the first 8 pictures.
The incomplete spare ISS array assy originally removed from LLO HAM2 (S1202966) was moved to a shelf under the work table right next to the clean loom in the optics lab (see the 9th picture). Note that one PD was pulled from that and was transplanted to our installation spare S1202965.
Metadata for both 2965 and 2966 were updated.
ISS second array parts inventory https://dcc.ligo.org/E2500191 is being updated.
Rahul and I cleared the optics table so Josh and Jeff can do their SPI work.
Optics mounts and things were put in the blue cabinet. Mirrors, PBS and lenses were put back into labeled containers and in the cabinet in front of the door to the change area.
Butterfly module laser, the LD driver and TEC controller were put back in the gray plastic bin. There was no space in the cabinets/shelves so it's put under the optics table closer to the flow bench area.
Single channel PZT drivers were put back in the cabinet on the northwest wall in the optics lab. Two channel PZT driver, oscilloscopes, a function generator and DC supplies went back to the EE shop.
OnTrack QPD preamp, its dedicated power transformer, LIGO's LCD interface for QPD and its power supply were put in a corner of one of the bottom shelf of the cabinet on the southwest wall.
Thorlabs M2 profiler and a special lens kit for that were given to Tony who stored them in the Pcal lab.
aLIGO PSL ISS PD array spare parts inventory E2500191 was updated.
Closes FAMIS#28429, last checked 87622
ITMX didn't have enough coherence again this time :(
Closes FAMIS27404, last checked in alog87178
In general we can see blips at 10/21 and 09/10 from the BRS-Y damping issues and the power outage.
We can see the BRSY issues we had last week 10/21 alog87634, ETMY BRS temperature seems to still be slowly increasing just like last month?
BRS-X looks to be drifting down for ~all of October.
Jeff, Ryan S, Oli
During last week's set of issues, something that we saw happen a few times during our lock reacquisition attempts were lots of EY saturations while going through LOWNOISE_COIL_DRIVERS/TRANSITION_FROM_ETMX. The saturations would stop once L2 to R0 damping was turned off (87713), so it seemed like the issue was with the ETMY L2 satamp, so we swapped it out with a different one (87722). We didn't see any of these repeating saturations after that, but also we were changing a lot of things at the time trying to figure out the problem, plus we hadn't been seeing these saturations during every single relock attempt.
The DAC channels that were showing saturations were from DAC1 channels 1 and 2. Checking the model, those channels line up with R0 F2 and F3, which are the channels that control Length on R0. We plotted R0's MASTER OUTs during times where we saw lots of the EY saturations, and at times where the saturations heard on verbals were normal, including a time before we swapped the ETMY L2 satamp on October 14th.
Here's a breakdown of the different examples we looked at:
| Normal amount of saturations during LOWNOISE_COIL_DRIVERS / TRANSITION_FROM_ETMX | |||
| Date | SatAmp | verbals | ndscope |
| Oct 1 | unmodified | oct1_verbals | oct1_ndscope |
| Oct 20 | modified | oct20_verbals | oct20_ndscope |
| Oct 22 | modified | oct22_verbals | oct22_ndscope |
| Lots of EY saturations during LOWNOISE_COIL_DRIVERS / TRANSITION_FROM_ETMX | |||
| Oct 23 | modified | oct23_verbals | oct23_ndscope oct23_ndscope_zoomout |
| Oct 24 | modified | oct24_verbals | oct24_ndscope |
We saw that for the times where the amount of saturations were what we consider 'normal', the LOWNOISE_COIL_DRIVERS/TRANSITION_FROM_ETMX states behave similarly in the R0 MASTER OUT channels, including after swapping the satamp. The OSEMs will see some movement, but it's not too far outside of where they usually sit. However, for the two times that we checked where we had the excessive EY saturations, we saw that right before they started, there was a high frequency glitch seen in the ETMY L2 Length witness channel. This glitch only moved L2 a small amount, about 0.5 um, but it was causing R0 to move a lot in Length, saturating or nearly saturating for a long time.
Plotting the impulse response of the SUS-ETMY_L2_R0DAMP_L filter bank, we see that these filters have an impulse response time of ~16 seconds, and breaking down the impulse response by each filter's contribution, we see that the FM8 (module 7) filter module, invPsmoo, has a wild impulse response. Because of this filter module, the impulse response of the entire R0_L2DAMP_L filter bank is extremely long, and the signal is very large. The frequency response plot for module 7 shows us that it approaches the 10^15 gain at higher frequencies. Additionally, these new satamps have about double the gain at high frequencies as compared to the old satamps, so that would also be exacerbating any issues at higher frequencies.
With all that said, it looks like the conclusion is that the EY saturation issues from last week were not caused by a faulty satamp, but instead by something else that caused L2 to glitch, and the long impulse response and high gain causing R0 to take forever to calm down.
A temporary solution would be to keep the L2 to R0 damping off during locking until after LOWNOISE_LENGTH_CONTROL has finished, to make sure that we are avoiding having it on during all the sudden movements that could upset R0.
I am confused about the conclusions of this alog. Attached is a screenshot of the last time we had these saturations before the satamp was replaced. I did a test where I turned off the R0 tracking loop (ETMY L2->R0 length) by ramping the gain of the loop to zero on a 15 second ramp. The saturations stopped. I then ramped back on and saw the saturations return. I waited seven minutes and tried ramping on again and got the same saturation warnings. This test was done while we sat in state 560, which is lownoise_length_control. The state had completed and we held there in order to track down the saturations.
I can see the glitch that Jeff and Oli found in this alog, but I don't see any other glitches that caused the subsequent saturations when I was turning the gain on and off. The ramp time should be long enough to avoid any sort of issues with the impulse response, and the on/off test happened many minutes after the noted glitch, so I don't think they can be explained by this impulse response issue.
I don't necessarily think this indicates the satamp is the problem, except that we haven't had these saturations since the replacement, and this loop has been running for a long time without issue (my understanding is since O3b, but I don't know for certain).
I agree that a good way to avoid this issue is to engage the R0 tracking later on in the guardian.
Some DRMI locking info
MICH, PRCL, SRCL filter banks during the "acquire DRMI 1f" state before the lock is grabbed.
OLGs for MICH, PRCL, SRCL after 1F acquisition, DRMI ASC engaged.
WP 12844
ECR E2400330
Modified List T2500232
The following SUS SAT Amps were upgraded per ECR E2400330. Modification improves the whitening stage to reduce ADC noise from 0.05 to 10 Hz.
| Suspension | Old | New | OSEM |
| MC1 M2 | S1100182 | S1100148 | ULLLURLR |
| MC1 M3 | S1100176 | S1100135 | ULLLURLR |
| MC3 M2 | S1100069 | S1100106 | ULLLURLR |
| MC3 M3 | S1100123 | S1100093 | ULLLURLR |
| PR3 M2 | S1100063 | S1000274 | ULLLURLR |
| PR3 M3 | S1100113 | S1000277 | ULLLURLR |
| MC2 M2 | S1100110 | S1100169 | ULLLURLR |
| MC2 M3 | S1000294 | S1100174 | ULLLURLR |
| SR3 M2 | S1100105 | S1100146 | ULLLURLR |
| SR3 M3 | S1100074 | S1100134 | ULLLURLR |
F. Clara, J. Kissel, O. Patane
Here's the characterization data and fit results for S1100148, assigned to MC1 M2's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100148_MC1_M2_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| MC1 | M2 | S1100148 | CH1 | UL | 0.0949:5.19 | 120.3 | zpk([5.19],[0.0949],1,"n") |
| CH2 | LL | 0.0961:5.24 | 120.5 | zpk([5.24],[0.0961],1,"n") | |||
| CH3 | UR | 0.0962:5.25 | 120.5 | zpk([5.25],[0.0962],1,"n") | |||
| CH4 | LR | 0.0967:5.27 | 120.375 | zpk([5.27],[0.0967],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1100148_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
Here's the characterization data and fit results for S1100135, assigned to MC1 M3's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100135_MC1_M3_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| MC1 | M3 | S1100135 | CH1 | UL | 0.0955:5.21 | 120.25 | zpk([5.21],[0.0955],1,"n") |
| CH2 | LL | 0.0962:5.25 | 120.25 | zpk([5.25],[0.0962],1,"n") | |||
| CH3 | UR | 0.0973:5.31 | 120.125 | zpk([5.31],[0.0973],1,"n") | |||
| CH4 | LR | 0.097:5.3 | 120.125 | zpk([5.3],[0.097],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1100135_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
Here's the characterization data and fit results for S1100106, assigned to MC3 M2's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100106_MC3_M2_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| MC3 | M2 | S1100106 | CH1 | UL | 0.0978:5.34 | 120.25 | zpk([5.34],[0.0978],1,"n") |
| CH2 | LL | 0.096:5.24 | 120.5 | zpk([5.24],[0.096],1,"n") | |||
| CH3 | UR | 0.0973:5.32 | 120.125 | zpk([5.32],[0.0973],1,"n") | |||
| CH4 | LR | 0.0955:5.21 | 120.5 | zpk([5.21],[0.0955],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1100106_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
Here's the characterization data and fit results for S1100093, assigned to MC3 M3's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100093_MC3_M3_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| MC3 | M3 | S1100093 | CH1 | UL | 0.0966:5.28 | 120.0 | zpk([5.28],[0.0966],1,"n") |
| CH2 | LL | 0.099:5.4 | 120.375 | zpk([5.4],[0.099],1,"n") | |||
| CH3 | UR | 0.0969:5.3 | 120.0 | zpk([5.3],[0.0969],1,"n") | |||
| CH4 | LR | 0.0966:5.28 | 120.125 | zpk([5.28],[0.0966],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1100093_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
Here's the characterization data and fit results for S1000274, assigned to PR3 M2's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1000274_PR3_M2_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| PR3 | M2 | S1000274 | CH1 | UL | 0.0947:5.17 | 120.25 | zpk([5.17],[0.0947],1,"n") |
| CH2 | LL | 0.0961:5.24 | 120.25 | zpk([5.24],[0.0961],1,"n") | |||
| CH3 | UR | 0.0963:5.26 | 120.0 | zpk([5.26],[0.0963],1,"n") | |||
| CH4 | LR | 0.0962:5.25 | 120.25 | zpk([5.25],[0.0962],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1000274_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
Here's the characterization data and fit results for S1000277, assigned to PR3 M3's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1000277_PR3_M3_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| PR3 | M3 | S1000277 | CH1 | UL | 0.0962:5.26 | 120.0 | zpk([5.26],[0.0962],1,"n") |
| CH2 | LL | 0.0948:5.17 | 120.5 | zpk([5.17],[0.0948],1,"n") | |||
| CH3 | UR | 0.0941:5.12 | 120.5 | zpk([5.12],[0.0941],1,"n") | |||
| CH4 | LR | 0.0958:5.23 | 120.25 | zpk([5.23],[0.0958],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1000277_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
Here's the characterization data and fit results for S1100169, assigned to MC2 M2's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100169_MC2_M2_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| MC2 | M2 | S1100169 | CH1 | UL | 0.0976:5.34 | 120.25 | zpk([5.34],[0.0976],1,"n") |
| CH2 | LL | 0.0964:5.26 | 120.25 | zpk([5.26],[0.0964],1,"n") | |||
| CH3 | UR | 0.0955:5.21 | 120.25 | zpk([5.21],[0.0955],1,"n") | |||
| CH4 | LR | 0.0973:5.31 | 120.2 | zpk([5.31],[0.0973],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1100169_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
Here's the characterization data and fit results for S1100174, assigned to MC2 M3's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100174_MC2_M3_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| MC2 | M3 | S1100174 | CH1 | UL | 0.0993:5.43 | 120 | zpk([5.43],[0.0993],1,"n") |
| CH2 | LL | 0.0969:5.3 | 120 | zpk([5.3],[0.0969],1,"n") | |||
| CH3 | UR | 0.0951:5.2 | 120 | zpk([5.2],[0.0951],1,"n") | |||
| CH4 | LR | 0.0952:5.2 | 120 | zpk([5.2],[0.0952],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1100174_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
Here's the characterization data and fit results for S1100146, assigned to SR3 M2's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100146_SR3_M2_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| SR3 | M2 | S1100146 | CH1 | UL | 0.0968:5.29 | 120.0 | zpk([5.29],[0.0968],1,"n") |
| CH2 | LL | 0.0989:5.4 | 120.0 | zpk([5.4],[0.0989],1,"n") | |||
| CH3 | UR | 0.0948:5.18 | 120.0 | zpk([5.18],[0.0948],1,"n") | |||
| CH4 | LR | 0.0966:5.27 | 120.25 | zpk([5.27],[0.0966],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1100146_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
Here's the characterization data and fit results for S1100134, assigned to SR3 M3's ULLLURLR OSEMs.
This sat amp is a UK 4CH sat amp, D0900900 / D0901284. The data was taken per methods described in T080062-v3, using the diagrammatic setup shown on PAGE 1 of the Measurement Diagrams from LHO:86807.
The data was processed and fit using ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Scripts/
plotresponse_S1100134_SR3_M3_ULLLURLR_20251020.m
Explicitly, the fit to the whitening stage zero and pole, the transimpedance feedback resistor, and foton design string are:
| Optic | Stage | Serial_Number | Channel_Number | OSEM_Name | Zero_Pole_Hz | R_TIA_kOhm | Foton_Design |
|---|---|---|---|---|---|---|---|
| SR3 | M3 | S1100134 | CH1 | UL | 0.0975:5.32 | 120.0 | zpk([5.32],[0.0975],1,"n") |
| CH2 | LL | 0.0958:5.23 | 120.0 | zpk([5.23],[0.0958],1,"n") | |||
| CH3 | UR | 0.0958:5.22 | 120.375 | zpk([5.22],[0.0958],1,"n") | |||
| CH4 | LR | 0.0985:5.38 | 120.25 | zpk([5.38],[0.0985],1,"n") |
The attached plot and machine readable .txt file version of the above table are also found in ${SusSVN}/trunk/electronicstesting/lho_electronics_testing/satamp/ECR_E2400330/Results/
2025-10-20_UKSatAmp_S1100134_D0901284-v5_fitresults.txt
Per usual, R_TIA_kOhm is not used in the compensation filter -- but after ruling out an adjustment in the zero frequency (by zeroing the phase residual at the lowest few frequency points), Jeff nudged the transimpedance a bit to get the magnitude scale within the ~0.25%, shown in the attached results. Any scaling like this will be accounted for instead with the absolute calibration step, i.e. Side Quest 4 from G2501621, a la what was done for PR3 and SR3 top masses in LHO:86222 and LHO:84531 respectively.
With Jumbo frames configured these are the iper3 results on the 100Gig (Intel E810):
- - - - - - - - - - - - - - - - - - - - - - - - -[ ID] Interval Transfer Bitrate Retr[ 5] 0.00-60.00 sec 168 GBytes 24.0 Gbits/sec 5 sender[ 5] 0.00-60.00 sec 168 GBytes 24.0 Gbits/sec receiver[ 7] 0.00-60.00 sec 206 GBytes 29.5 Gbits/sec 9 sender[ 7] 0.00-60.00 sec 206 GBytes 29.5 Gbits/sec receiver[ 9] 0.00-60.00 sec 188 GBytes 26.8 Gbits/sec 4 sender[ 9] 0.00-60.00 sec 188 GBytes 26.8 Gbits/sec receiver[SUM] 0.00-60.00 sec 561 GBytes 80.3 Gbits/sec 18 sender[SUM] 0.00-60.00 sec 561 GBytes 80.3 Gbits/sec receiverFor the 25 Gig real time testing we are getting a round trip time (mean) of 50.1 us. In the state we left it at the end of today there are some error counters ticking, but no lost packets.
controls@lr-eth-e:$ sudo ethtool -S ens4f0np0 | grep errrx_crc_errors_phy: 5
rx_in_range_len_errors_phy: 0
rx_symbol_err_phy: 4
tx_errors_phy: 0
rx_pcs_symbol_err_phy: 4
rx_err_lane_0_phy: 474801