Day Shift: 15:00-23:00UTC, 8:00-16:00PT, times listed in UTC
Update on IFO:
- morning alignment issues: LSC to ETMX gain was zero when trying to lock the X arm on IR
--- the gain needed to lock was 0.10, when the usual gain set by Guardian is 0.05
- 18:40-18:41UTC switched ISI platforms to Quite_90s from 45mHz
--- reason: Quite_90s are better in wind, and 45mHz are know to be bad in wind, and wind is between 20 and 25mph
--- result: X and Y ALS arm signals dip to 0.7-0.8 while arms are locked in green (max is 1.09)
--- before switching to 45nMz, arms only dip down to 0.9-0.95
- as of 20:40UTC, IFO is well aligned and locking DRMI, but not making it much past DRIM
--- plan is to continue to let the IFO try for DARM_WFS
When an SEI platform trips and then relocks, there is DC control to zero the error point stearing to a fixed position. Not all ISI platforms/dofs do this but for HEPI, all platforms and all DOFs servo to the 'reference location', except, the pringles modes. These are the potato chip like distortions required to allow the other 'standard' cartesian dofs to be realised given the physics of the hardware. As an example, the four horizontal actuators on a HEPI platform are all situated at 45 degrees to the X & Y direction. For RZ, you can picture that you push or pull on the 4 actuators to easily get RZ (Yaw.) But consider X or Y, to move in X, the 2 far actuators will squeeze the Y dof together and the near actuators will push the Y apart. See the Attached for a visual of a BSC (G1000125.) The green arrows represent the signed directions of the local Actuator coordinates. Maybe better said, to achieve a motion in X, a movement in the Y component must occur. This 'distortion' is what is measured by the Pringle mode.
The pringle mode isolation loops of HEPI are not DC coupled, this is what Kiwamu noted in alog 22719. So despite the other cartesian positions being servo'd and back to their reference position, the pringle difference means that the local positions are not where they were before the trip. The second plot shows the four horizontal IPS positions (local) and the horizontal cartesian Location Mons. Clearly all the horizontal cartesian positions are where we tell them to go and the Pringle ends up where it does. Obviously too, the local sensors are not where they were before the trip. They all indicate about a 0.2mil (~6um) shift across the trip.
1) Kiwamu reports that the HAM2 ISI OpLev (looking at a fixed mirror on the ISI table) is only about a urad different at worst if that can be trusted.
2) It seems extreme to think that these shifts in the HEPI Actuator positions can translate ultimately to the ISI and cause shift requirements in the optics. These pringle distortions are not taken by the real support structure, the HEPI Actuator is designed to deal with that. However, the horizontal shift of the platform is experienced by the Vertical Actuators as a lateral shift of the IPS sensors wrt its flag. There will in fact also be an associated tilt with this lateral slide. These out-of-axis shifts of the sensor/flag can result in real shifts of position. The four vertical local IPS sensors all indicate around a 4um shifts.
3) So despite having restored the cartesian computations to the reference location, the actual actuators are not in their previous positions and these may lie to us at some level, some worse likely more than others, and maybe we are shifting the ISI Stage0 and ultimately the Optical Table.
Maybe this should be considered low priority but we should consider how we can close these loops so we can get repeated positions:
1) Rather than closing these loops all at once, maybe in a particular sequence to achieve a repeatable local position result
2) Maybe we actually put DC authority into the pringle modes and we'll achieve 1) without all the thinking, modeling, and teeth gnashing
GregM, RickS, DarkhanT, JeffK, SudarshanS
This was an attempt to study what the GDS output will look like with kappa factors applied. GregM volunteered to create test data with kappa applied, kappa_C and kappa_tst, on 'C01' data for the days between October 1 through 8. The kappa corrected data is referred as 'X00'. The correction factors are applied by averaging the kappa's at 128s. This was loosely determined from the study done last week (alog 22753) on what the kappa's look like with different time-averaging duration.
Here, comparisons are made between 'C01' as 'X00'. The first plot contains the kappa factors that are relevant to us. kappa_tst and kappa_C are applied and are thus relevant, whereas cavity pole (f_c) varies quite a bit at the beginning of each lock-stretch and is thus significant but we don't have an infrastructure to correct it. The first page contains kappa's calculated at a 10s FFT and is plotted on red and a 120s averaged kappa's plotted in blue. Page 2 has similar plot but has kappa plotted at 20 minutes averaging (it helps to see the trend more clearly).
Page 3 and onwards has plots of GDS/PCal at pcal calibration line frequencies for both magnitude and phase plotted for C01 and X00 data. The most interesting plots are the magnitude plots because applying real part of kappa_tst and kappa_c does not have a significant impact on phase. The most interesting thing is that applying kappa's flattens out the long-term trends in GDS/Pcal in all four frequencies. However, at 36 Hz, it flattens out the initial transient as well but introduces some noise into the data. At 332 Hz and 1 Khz it introduces the transient at the beginning of the lock stretch and it does not seem to have much effect at 3 KHz line. We think that this transient should be flattened out as well with the application of kappa's. The caveat is we don't apply cavity pole correction and we know that the cavity pole has a significant effect in the frequency region above the cavity pole.
DarkhanT, RickS, SudarshaK
After seeing the ~2 % transient at the beginning of almost each lock stretch in GDS [h(t)] trend at around 332 Hz, we had a hunch that this could be a result of not correcting for cavity pole frequency fluctuation. Today, Drarkhan, Rick and I looked at old carpet plots to see if we expect variation similar to what we are seeing and indeed the carpets plot predicted few percent error in h(t) when cavity pole is varying by 10 Hz.
So we decided to correct for the cavity pole fluctuation to h(t) at calibartion line frequency. We basically assumed that h(t) is sensing dominated at 332 Hz and used absolute value of the correction factor that change in cavity pole would incur [C/C' = (1+ i* f /f_c)/(1+ i* f /f_c')] and appropriately multiplied it to the GDS output.
The result is attached below. Applying cavity pole fluctuation gets rid of the transient seen at the beginning of each lock stretch as well as 1 % overall systematic we saw on the whole trend. We used cavity pole as 341 Hz for nominal value which is calculated from the model at the time of calibration. In the plot below, the cyan in both bottom and top left are the output of GDS CALIB_STRAIN/ PCAL uncorrected for Kappas, the green on the top left is corrected for kappa_tst, kappa_C and cavity pole whereas the green on the bottom left is corrected for kappa_C and kappa_tst only ( we only know how to correct these in time domain).
Ops Day Shift: 15:00-23:00UTC, 8:00-16:00PT
H1 current state: relocking after an initial alignment
Help: Jenne
Summary:
Earthquake and useism and wind at EY have caused some locking issues.
Currently IFO has locked DRMI and attempted ENGAGE_ASC once without success.
Relocking continues.
Subsystem Reports:
Kyle - trips around the site, y28 and x28, closest to the end stations.
Hugh - no invasive work
Richard - electronics cabling
Jason - PSL plumbing change
Maintenance tomorrow:
Bubba - HAM1 pier grouting, laser safe, many hours
Richard - temperature sensor install
Kiwamu/Sedarshan - ISS 2nd loop
JeffB - cabling
Jodi - heavy things moved to Mid Stations
Richard - more solar panel work
Betsy - Tip-Tilt inventory
The main report can be found on the detchar wiki, but here are the highlights:
The script had stopped, same connection error as usual. I restarted it in the same screen (pid: 4403).
One stage of heat was added Friday 23rd but the LVEA temperature control is still marginal so we have energized an additional heater. HC3B is now operating on one stage. It appears that the control signal for this heater is not working correctly. It is set to 0ma which should not turn it on but when we energized it the duct temperature rose to 81F which is consistent with one stage.
TITLE: Oct 26 OWL Shift 7:00-15:00UTC (00:00-08:00 PDT), all times posted in UTC
STATE Of H1: Aligning
SUPPORT: Jenne
LOCK DURATION:
INCOMING OPERATOR: Cheryl
ACTIVITY LOG:
07:49 DARM “breathed” between 60Hz and 300Hz with no saturation verbal.
08:00 Wind speeds have picked up, sometimes gusting to 40mph.
08:12 Lockloss. More than likely due to high winds. µSei approaching .9microns/s.
08:30 Wind has dropped down to below 20mph. IFO is locking again.
08:50 Lockloss after being at ENGAGE_ASC_PART3 for a minute or so.
09:01 IFO made it to RF_DARM then lost lock.
09:08 Wind picking up again to almost 30mph. This time the CS is taking the brunt.
10:00 Started switching GS13 gains to LO to get everything as damped as I can.
10:34 Re-Aligned/Isolated HAMs 2&3. GS13s switched back to high gain. IMC relocked. EQ band getting back down to 1micron/s
12:41 I’ve been having trouble trying to find my ALS spots. I’ve trended optic alignments, I’ve cleared ALS WFS histories, I’ve run the dither scripts, I’ve checked shutters for “open” and I’ve called Jenne. I left a message and haven’t heard back yet. Since microseism is still kind of high I don’t want to bother anyone who isn’t on call today until it gets a little better and the time gets a little later.
13:19 GRB alarm. Neither observatory is up.
13:24 PR3 was still in damped mode!!!!! GRRRR! I got my ALS spot back. :)
15:00 Finally got some semblance of an initial alignment happening.
SHIFT SUMMARY: After a harrowing night of wind and earthquake activity, Initial alignment is happening. Ground motion is still high. Handing off to Cheryl.
Apologies. My activity log doesn't reflect the eq activity between 09:08-10:00UTC. This gives the impression that I was switching GS13 gains because of wind.
MID-SHIFT SUMMARY: IFO was locked and holding it’s own, despite the rise in wind speed and high microseism until 08:12UTC. Perhaps it was the building tilt that was eventually the demise of this lock stretch. Then while trying to relock, the 7.7mag quake near Afghanistan started tripping everything. I’ve gotten everything back up, isolated and gained up. The IMC is re-locked but I’m having trouble finding Green ALS Beams. µSei is still up around .7microns and the eq bands are still up in the .3-.4micron range. I don’t think a phone call to wake anyone is warranted until I think I at least have a chance of actually re-locking. I’ll keep plugging away at my problem for now.
EQ band still showing in excess of 10 microns/s. I've got all tripped ISIs damped and the GS13 gains set to low. I also have the Quads and Beam Splitter damped. Most of the tripped smaller suspensions stayed untripped without damping. Look like it's going to be a while befor I can do anything here. :/
This isn't Jim Warner. It's Ed. There were some Firefox sessions left open, on another workspace. I use Chromium.
Summary: Figures 8 and 9 are summary plots for calculating vibration effects on DARM or for determining the SNR in environmental channels needed to produce a certain SNR in DARM. We summarize with our current working model of vibrational coupling at LHO:
Above 50 Hz
At the corner station there are three sites that strongly couple ground or acoustically induced vibrations into DARM: HAM6, HAM2 and the PSL table. The most important vibration sensors for monitoring these couplings are the PSL periscope accelerometer and the GS13s in HAMs 2 and 6. We think that the PSL table vibrations couple mainly by causing beam jitter. Our best guess is that the coupling at HAM2 is similarly produced by jitter: vibrations couple through the ISI suspension and move optics on the table. The two steering mirrors and the periscope just upstream of the IMC are not suspended and so are good candidates. At HAM6, sound shakes the blue cross beam, which would shake stage 0, which, in turn, would shake the table top, especially at ISI suspension resonances. More speculatively, this HAM6 table top motion may couple through the OM or OMC suspensions causing small relative motions of the mirrors in the OMC (if the OMC is not a rigid body at 1000 Hz), amplified by the finesse, or motion of the OMs. The motion of these mirrors would modulate the light, which results in intermodulation with the 4100 Hz OMC dither frequency, producing up and down-converted features as well as direct coupling. The contention that we have identified the dominant vibration coupling sites is supported by our observation that, at least for linear coupling, the effects of global acoustic injections can mainly be explained using the GS13s at HAM6 and coupling factors from the shaking injections.
At the end stations, we have not narrowed down the coupling sites or mechanisms. There is high coupling in the EX VEA and the large sidebands that Sheila saw suggest that coupling is via scattering.
Below 50 Hz
At the corner station there is high coupling at certain frequencies between 10 and 50 Hz, but we were shaking the whole building and so we have not narrowed down the coupling sites. At the end stations we did not see coupling in this band. We also found that ground motion at the corner station in the 10-50 Hz band produced noise in at least the 82-100 Hz band of DARM.
Ambient environmental levels at the following sensors are estimated to produce noise in DARM that is within a factor of 3 of the current DARM floor:
LVEA floor seismometers: at 10 Hz and at least another couple of regions between 20 and 80 Hz
HAM6 GS13s: around 370, 875, 995,1050 Hz
HAM2 GS13s: around 225 Hz
Output optics microphone: around 450 Hz, 875, 995 Hz
PSL periscope accelerometer: several places between 100 and 1500 Hz
EX VEA microphones: around 55 Hz and 70 Hz
Shaking
Global shaking
We found that our standard shakers and speakers did not provide sufficient amplitude below 30 Hz for our shaking signals to be visible in DARM. We instead used tampers, which have the additional advantage that they can shake so strongly that they can be sited far from the building, shaking everything with the same amplitude (this is only true to roughly a factor of 2, most likely because of scattering of the surface waves). We used a jumping jack (provides ~10 Hz comb) and a plate tamper (30-70 Hz range), both of which are pictured at the closest site (140 m) to the corner station vertex in Figure 1. We also used sites at 275 m and 430 m for the corner station and sites at similar distances from the end stations. The different distances were used to control shaking amplitude and especially the harmonics (higher frequencies attenuate faster with distance). The most distant site was used to minimize the harmonics in the 80-100 Hz band so that we could look for up-conversion.
Direct coupling
Figure 2 shows spectra for a single one of the tamper injections and shows noise estimates compiled from all of the injections at the 3 stations. The most notable result is the high coupling around 10 Hz for the corner station only. Ground motion at the corner station appears close to dominating the DARM noise floor around 10 Hz. The coupling around 10 Hz is at least (we only obtained upper limits) 2 orders of magnitude smaller at the end stations. The corner station coupling is also less than a factor of ten below the current DARM noise floor at frequencies above 40 Hz. Obviously this coupling needs to be reduced for us to reach our sensitivity goals.
Up-conversion
In addition to high direct coupling, a close examination of Figure 2 shows apparent up-conversion above 40 Hz (the red line is above the blue line more than it is below it). This up-conversion is certainly not obvious so we did 10 cycles of shaker injections at this 430m site, 1 minute on, 1 minute off. We then took the BLRMS between 82 and 100 Hz and statistically compared the on and off times. The average “on” value was 5% greater than the average off value and Students-T and Wilcoxon matched signed pairs tests indicate that the difference is significant at greater than 95% probability. The seismometer signal was 4% higher during the on period (though this difference did not reach the 95% level), probably because higher harmonics weren’t completely attenuated. However, injections in the 82-100 Hz band show that vibrations are not right at the DARM floor and a 4% increase in ground motion should not produce a 5% increase in DARM. Thus the tamper injections indicate that we suffer from upconversion at least into the 82-100 Hz band.
The tamper upconversion prompted us to try a site-wide HVAC shutdown, since the HVAC dominates the ground motion in the tens of Hz band. The results were consistent with the upconversion hypothesis: the BNS range increased by a few Mpc (https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=22532). However, all turbines on the site were off, so there is also the possibility that the DARM improvement was due to reduced HVAC noise in the 70-100 Hz band at EX where there is high direct coupling (this could be checked).
Finally, Figure 2 also shows 1 and 2 Hz estimates from rolling cart injections at the CS. Signal was not seen in DARM at 1 and 2 Hz, so ambient levels are further from DARM then at 10 Hz.
Local shaking
HAM6 ISI shaking
High vibration coupling has been noted at HAM6 (Link, Link), which contains the OMC and GW diodes. It is associated with motion of the table, with the vibrations coming up through the ISI suspension (Link), and some damping remedies have been suggested to mitigate coupling through the suspensions (Link, Link).
Figure 3 shows results from shaking by injecting bands of uniform noise using the ISI actuators. The solid symbols are made by multiplying the level produced by the injection in DARM by the ratio of the ambient motion amplitude to the injection amplitude in the sensor signal from the GS13s. This provides the plotted estimate of the noise that the ambient background contributes to DARM. The unfilled symbols indicate that the injection did not produce features in DARM and so they represent upper limits to the ambient contribution to DARM.
The assumption in these estimates is that the feature in DARM increases linearly with injection amplitude. Figure 4 shows that DARM features appearing at the injection frequency increase approximately linearly with injection amplitude.
In addition to direct coupling, we found that vibrational coupling at HAM6, in certain bands, can produce up/down-conversion features in DARM as a result of intermodulation with the OMC dither. To illustrate this, the injections were split into frequency bands. The DARM spectrum features in red in Figure 4 were produced by ISI injection in the 800-1200 Hz band, including the red features in the 100 Hz region. The up/down-conversion features usually do not increase linearly with injection amplitude, so the red stars (stars indicate up/down conversion) should be thought of as indicating the factor by which the ambient level in the injection band would have to increase to produce the red features in the spectrum, and not the noise contribution to DARM at present ambient levels. Also, the up/down conversion stars are calculated by dividing DARM by the average ratio of ambient to injection in the 800-1200 Hz instead of the ratio at the frequency of the star on the plot.
The closest approach of the ambient estimates to DARM is near 1050 Hz, indicating that an increase in GS13 signal by a factor of a little more than 2 at this frequency would produce a feature in DARM. The GS13 signals are not stored at a high enough rate (currently 2048) to record this frequency and we propose that the sample rate should be increased, at least at HAM6, to record this band.
HAM6 blue cross beam shaking
Figure 5 shows estimates of coupling levels between HAM6 GS13 signals and DARM, but for an external shaker injection (mounted on a blue cross-beam) instead of an ISI actuator injection. The ISI and shaker injection results are similar in that they both show roughly the same sensitivity in the same bands (the bands associated with peaks in the ISI transfer function), but they are quite different in detail. We think that the likely source of the difference between ISI and shaker injections is that the drives on the HAM6 tabletop are at two different locations: the ISI actuators and the suspension points, and the table is not a rigid body at these frequencies.
We focused more on ISI injections than on shaker injections for the formal PEM injection program this time and, in view of the differences, we now think this was a mistake. Since we concentrate not on servo noise but on external environmental signals, the shaker injections, coupling in at the suspension points, represent more realistic estimates for environmental signals.
Figure 5 also shows the GS13 signals during the 400-800 Hz injection. While there was some noise injected in the region around 1000 Hz, the red points from the injection in that band show that the orange features could not have been produced by the excess noise from the 400-800 Hz injection. Also, the GS13 spectra illustrate what the ambient levels look like. Over much of the band the signal is flat, indicating the electronic noise floor. Estimates in such regions would overestimate the ambient contribution to DARM, but in the regions where we made estimates of the ambient contribution, we made sure that the GS13s were not flat, indicating that they were “seeing” ambient motion.
We also shook in the 1200 - 7200 Hz band (not shown). The GS13s give signals out to 1800 Hz (test points, not stored) so we are not sure of the injection levels, but the injection level produced motion at a couple of orders of magnitude over background when it was in band. We saw no features produced in DARM for this level. Even higher levels, though (estimated to be about 3 orders of magnitude above ambient), did produce up and down conversion features that are apparently produced by beating with the 4100 OMC dither frequency. Any such environmental signals would be monitored by the 16k microphones and the 16k accelerometer on HAM6.
The HAM6 shaker injections suggest that increases over ambient of less than a factor of 5 will appear in DARM near 75 Hz, near 370 Hz, and in the 850-1100 Hz band.
HAM2 ISI shaking
Figure 6 shows results of ISI actuator injections at HAM2. Unlike HAM6, we saw no up/down conversion for injections that increased the motion by a couple of orders of magnitude. In addition to the 800-1200 Hz ISI suspension resonance band, HAM2 is sensitive in the 200-300 Hz band, with the contribution of ambient motion at 225-229 Hz expected to be within a factor of 2 or 3 of the DARM floor.
The high coupling at HAM2 may be associated with the unsuspended mirrors that touch the main beam, the two mirrors in the in-vacuum periscope and the 2 steering mirrors just upstream of the mode cleaner. The sharp peak at 227 Hz is likely an optic resonance, possibly the periscope.
Other chambers
Prior to the start of O1, Robert and his SURF student Katie Banowetz shook every chamber at the LHO corner station using shakers attached to blue cross-beams, HAM1, HAM2, HAM3, HAM4, HAM5, HAM6, BSC1, BSC2 and BSC3. For shaking at about 2 orders of magnitude above background, features in DARM were only seen for HAM6 and HAM2. The end station chambers were postponed to the PEM injections but time again ran out. These chambers should probably be shaken during the O1 run.
Potential scattering sites
During PEM injections, we shook a number of potential scattering sites that had been identified in photographs taken from the point of view of the test masses (Link). These included the valve seats just beyond the test masses, the beam tubes between HAMs 2 and 3 and between HAMs 4 and 5. For shaking at about 2 orders of magnitude above ambient in the 50-7000 Hz band, we did not see features in DARM.
PSL table
The PSL table is one of the most sensitive vibration coupling sites at acoustic frequencies, (see below) but shaking with a table-mounted shaker below 40 Hz did not produce detectable coupling. The upper limits are shown in Figure 7.
Coupling functions for vibration sensors
Figure 8 shows a compilation of coupling functions (meters of test mass motion per meter of sensor motion) for both global and local shaking. The coupling functions can be multiplied by the level of the signal from the sensor indicated in the legend for an estimate of the noise in DARM produced by that level of motion. The accuracy of this prediction depends on how close to linear the coupling is.
Acoustic injections
Figure 9 is a summary of acoustic coupling, showing, for all stations, the coupling functions for all injections that produced features in DARM, and the estimated level of noise in DARM for ambient sound levels. The coupling functions can be multiplied by the level in the particular microphone indicated in the legend in order to predict the resulting level in DARM. The estimated ambient levels show the estimated ambient contribution to DARM. In addition, the ratio between the estimated ambient levels and the DARM floor indicates how much larger the SNR would be in the environmental channel than in DARM (if the estimated ambient is 1/10 of the DARM floor then the SNR would be 10 times greater for an event produced by the environment. The plots are for linear coupling and do not show up or down-conversion coupling but, like the vibration summary, they show warning bands where non-linear coupling may occur.
Figures 10-15 show the sources of the data for Figure 9 and include up and down-conversion. Figure 10, for example, shows, in the top plot, four different band limited injections as seen on the vertex microphone. The DARM spectra for each injection, in the lower plot, are the same color as the injection trace. The bands were chosen to highlight the up and down conversion from intermodulation with the OMC dither. The orange 700-1200 Hz injection produces features around 2000 Hz and in higher bands, as well as in the 10-120 Hz region. The lower plot also shows the estimated contribution to DARM of ambient levels of sound, assuming linearity. Notice that the estimated levels are the same factor below the DARM noise produced by the injection as the injection level is above the ambient sound level. Upper limits (when no signal is induced in DARM or the sensor is at its electronic noise floor for ambient sound level) are also indicated, as well as the up/down conversion levels.
The estimated ambient points indicating up/down conversion from intermodulation are made by dividing DARM during the injection by the ratio of injection/ambient in the 700-1200 Hz band. We use the average for that band. However, this is only a rough estimate, as the injection amplitude varies over the band and the upconversion is likely produced at very specific resonances within the injection band. And, of course, the estimated ambient level for up/down conversion is an upper limit since the coupling is non-linear.
Robert, Anamaria
08:12UTC More than likely due to high winds. µSei approaching .9microns/s.
This entry was mad by me, not Jim. An alog session had been left open on another workspace that I was unaware of.
As Corey and Kiwmau noted, ETMY has 2 violin mode harmonics fairly close to each other (1008.45 and 1008.49). ETMY MODE3 has been set up to damp the higher frequency one with a broad bandpass, a phase of +60 and a gain of +100 set in the guardian (FM1,3,4,10, total phase at 1008 is 82 degrees). Cheryl looked at the DARM spectrum over some of the long locks recently, and it seems that with these settings the lower frequency one 1008.45 has slowly rung up.
The phase shifting filter modules also had 6 dB of gain, which cause some unintended saturations, so I edited them to have 0 dB of gain at 1008.45 Hz. We addded two stop bands to the filter bank, one for 1008.493 and one for 1008.45 Hz.
After some confusion, we have been able to slowly damp this with a positive gain and FM1,2,4,5 (the new notch) ,and 10 on. This means a total phase of -75 degrees. This is not ringing up any other modes that we can see so far.
So for now:
The damping of both of these modes are commented out in the guardian, so it will only be damped if you engage one or the other by hand.
To damp 1008.49Hz use FM1 (broad bandpass at 1010), 3 (+60 degrees phase),4 (100dB), FM6 (to notch the 1008.45 mode), FM10 to notch 1009.6 mode and a positive gain
To damp 1008.45 use FM1,FM2 (-60 degrees) FM4, FM5 (to notch 1008.49Hz) and FM10 and a positive gain.
We can make two different filters to damp these two modes simulateously in the future.
This configuration causes the mode at 1009.03 Hz to ring up. Note that this mode already has its own dedicated damping FM (MODE7).
I added a stopband for this frequency in the MODE3 filter module. So far both modes (1008.45 Hz and 1009.03 Hz) are damping simultaneously now.
Damping the 1008.45 Hz mode with MODE3 was very slow going, so I implemented a separate damping loop using MODE9 and the following settings: FM1, FM2, FM4, FM9, positive gain, and length drive to the PUM (instead of pitch). This seems to be somewhat faster than before, but still much slower than some of our other damping loops. Anyway, the ADC counts for the DCPDs are topping out around 25000 ct in full lock with 1 stage of whitening (the limit is 32000 ct), so this is enough to proceed to nominal low noise. The mode should continue to damp down if we can maintain lock with these new damping settings.
To keep the 1008.49 Hz mode from ringing up again, I have turned on MODE3 with the settings that Sheila described above: FM1, FM3, FM4, FM6, FM9, FM10, positive gain, and pitch drive to the PUM.
As before, these settings will NOT engage automatically during lock acquisition. However, since we accepted these settings in SDF, either the loops will need to be engaged by hand, or new SDF settings accepted.
The Violin Mode Table has been updated. From what I have in my note, ETMY MODE3 filter has always been turned on by Guardian. I have the same question as Dan, what changes?
The LHO SEI team has known about a .6-ish hz peak on the HAM3 ISI for a long time (see my alog 15565, December of last year for the start, Hugh has a summary of LHO alogs in the SEI log for more). I was working with Ed on a DTT template for the operators when I noticed it was now gone. Very strange. Looking a little closer, it seems to have been decreasing over the last couple of days to a week, and disappeared completely this morning about 7-8:00 UTC. Attached spectra are from ~0:00 UTC (red) and ~16:00 UTC (blue, when I found it was missing). Looking at random times over the last week, it looks like it may have been trending down.
Could someone in Detchar look at this peaks longish term BLRMS, say over the last month, or even over the last year since we found it? Pretty much every sensor in that chamber saw this, but the GS-13s are the best witness.
I checked the coherence of H1:SUS-PR2_M1_ISIWIT_L_DQ with some PEM sensors for frequencies around 0.6 Hz.
Note - it reappeared for a few hours on Oct 13 - picture at https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=22775