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ID Date Author Type Category Subject
15778   Tue Jan 26 12:59:51 2021 AnchalHowToCDSAcromag wiring investigation

Taking inspiration from SR785 on how it reads differential signal, I figured that acromag too always need a way to return current through RTN ports always. That must be the reason why everything goes haywire when RTN is not connected to IN-. Now for single ended signals, we can always short RTN to IN- and keep same GND but then we need to be careful in avoiding ground loops. I'm gonna post a wiring diagram in next post to show how if two signal sources connect to each other separately, a GND loop can be formed if we tie each IN- port to RTN on an acromag.
Coming to the issue of reading a differential signal, what SR785 does is that it connects 50 Ohm resistance between Earth GND and differential signal shields (which are supposed to signal GND). In a floating GND setting, SR785 connects a 1 MOhm resistor between input shield and Earth GND. This can be used to read a differential signal through a single BNC cable since the shiled can take arbitrary voltages thanks ti the 1 MOhm resistor.

We can do the same in acromag. Instead of shorting RTN to IN- ports, we can connect them through a large resistor which would let IN- float but will give a path for current to return through RTN ports. Attached here are few scenarios where I connected IN- to RTN throguh wire, 820 Ohms, 10kOhms and 1MOhms in two sub cases where RTN was left open or was shorted to Earth GND. In all cases, the signal was produced by a 9V battery outputing roughly 8.16V. It seems that 10kOhm resistor between RTN and IN- with RTN connected to Earth GND is the best scenario noise wise. I'll post more results and a wiring diagram soon.

Attachment 1: TestingDifferentialSignalWithFloatingRTNwrtIN-.pdf
15777   Tue Jan 26 10:58:30 2021 gautamUpdateSUSMC2 tickler stuck on

For whatever reason, the autolocker didn't turn the tickle off for several hours. Seems to work okay now. The linked plot suggests that the coil balancing on MC2 is pretty lousy.

15776   Mon Jan 25 18:18:04 2021 AnchalSummaryBHDSatellite Amplifier Transfer Functions and noise

I took transfer function and noise measurement of satellite amplifier box's photodiode transimpedance circuit. For the measurement, I created a makeshift connector to convert backside DB25 into DB9 with the 4 channels for PDA input. The output was taken in differential form at the front PD Output port. To feed current to the circuit, I put in 12 kOhm resistors in series at the inputs, so the V/V transfer function measured was multiplied by 12 kOhm to get the transimpedance of the circuit.

# Transfer Function Measurement details

• SR785 source out was fed into PDA input pins using a makeshift BNC-DB9-DB25 converter.
• The output from PDOut DB9 port was fed to test switch in D1900068 to separate differential signal.
• This differential signal was fed back to SR785 at input 2 in A-B configuration.
• Measurements are taken with file D1002818_TF.yml and D1002818_TF_LF.yml.
• A measurement of just cables without the DUT is taken as well.
• Commands.txt list all the commands used.
• All data is compiled and plotted in Plotting.ipynb
• D1100117_S2100029_TFandNoiseSpectrum.pdf shows all the transfer functions measured.

# Spectrum Measurements

• Two pair of BNC cables were twisted together and clips were added at ends.
• One of the GND was connected to board GND. Rest were left unconnected to avoid ground loops.
• Each pair of signal was connected to PDOutP/N.
• The PDA inputs were shorted together to make zero input current to the board.
• Instrument noise with cables was measured by shorting the clips of the center cores and one of the shields of the two BNC cables together.
• Measurements were taken with file D1002818_SP.yml and D1002818_SP_LF.yml.
• Input referred current noise spectrum was calculated by dividing the output voltage noise spectrum by the measured transfer function.
• D1100117_S2100029_TFandNoiseSpectrum.pdf shows all the output votlage noise spectrum and input referred current noise spectrum measured.

Edit Wed Feb 10 15:14:13 2021 :

THE NOISE MEASUREMENT WAS WRONG HERE. SEE 40m/15799.

Attachment 1: D1002818_S2100029_TFandNoiseSpectrum.pdf
Attachment 2: D1002818_Testing.zip
15775   Wed Jan 20 19:12:16 2021 gautamUpdateCDSSLwebview fixed

After fixing multiple issues, the model webviews are updating, should be done by tomorrow. It should be obvious from the timestamps on the index page which are the new ones. These new screens are better than the old ones and offer more info/details. Please look at them, and let me know if there are broken links etc. Once we are happy with this new webview, we can archive the old files and clean up the top directory a bit. I don't think this adds anything to the channel accounting effort but it's a nice thing to have up-to-date webviews, I found the LLO ones really useful in setting up the AS WFS model.

BTW, the crontab on megatron is set to run every day at 0844. The process of updating the models is pretty heavy because of whatever MATLAB overhead. Do we really need to have this run every day? I modified the crontab to run every other Saturday, and we can manually run the update when we modify a model. Considering this hasn't been working for ~3 years, I think this is fine, but if anyone has strong preference you can edit the crontab.

If someboy can volunteer to fix the MEDM screenshot that would be useful.

15774   Wed Jan 20 18:07:09 2021 AnchalSummaryBHDHAM-A Coil Driver measurements before modifications

I have taken transfer functions and noise measurements of the two HAM-A coil driver boxes D1100687 #S2100027 and #S2100028. All transfer functions look as expected. I'm not sure about the noise measurements. If anyone sees flaw in my measurement method, please let me know. I'm not sure why in some channels I got 10Hz harmoni peaks in the noise. That was very strange. Also let me know if my current noise estimate is wrong.

# Transfer Function Measurement details

• SR785 source out was connected to the differential amplifier input of D1900068.
• The one pair of two BNC outputs of this differential amplifier goes directly to the SR785 Input 1 A and B.
• The DB9 output of the differential amplifier goes to the Coil Input DB9 connector J3.
• Header W2 was shorted to provide ground to the incoming signal.
• Header P4 was shorted to enable all the channels manually.
• Normal operation is the Acquisition mode (Acq) while when pins of header P3 are shorted, we go into the Run mode for respective channel.
• The “To Satellite Box” DB25 port at the read side was conencted to a DB25 breakout circuit and pins 1-9, 3-11, 5-13 and 7-15 were connected to 36 Ohm resistor to simulate Coil load.
• The “Output Monitor” on the rear side is then connected to the test switch DB9 port on D1900068.
• The the pair of BNCs from the test switch is connected to SR785 Input 2 A and B.
• Measurements are taken with file D1100687_TF.yml and D1100687_TF_LF.yml.
• A measurement of just cables without the DUT is taken as well.
• Commands.txt list all the commands used.
• All data is compiled and plotted in Plotting.ipynb
• D1100117_S2100027_TF.pdf and D1100117_S2100028_TF.pdf shows all the transfer functions measured.

# Spectrum Measurements

• All channels were kept in disabled mode (Not shorting P4) to ensure their inputs are grounded on the board.
• I ran two BNC cables with their centers connected to output monitors V2+ and V2- and one of their shields connected to board GND.
• in SR785, A-B differential mode always runs with grounded shields mode, so effectively the board GND got grounded to SR785 GND through internal 50 Ohm resistor. But all ground loops have been evaded.
• The two BNC cables were twisted together to minimize the area between the two center cores of the cables as that is the remaining pickoff possible in this measurement.
• Instrument noise with cables was measured first but shorting the clips of the center cores and one of the shields of the two BNC cables together.
• Measurements were taken with file D1100687_SP.yml and D1100687_SP_LF.yml.
• D1100117_S2100027_Voltage_Noise_Spectrum.pdf and D1100117_S2100028_Voltage_Noise_Spectrum.pdf shows the measured voltage noise spectrum at the output monitors when loaded with 36 Ohms.
• D1100117_S2100027_Current_Noise_Spectrum.pdf and D1100117_S2100028_Current_Noise_Spectrum.pdf shows the esitmate current noise through the coil calculated by dividing the measured voltage noise by 2436 Ohms.
Attachment 1: MeasurementData.zip
Attachment 2: D1100117_S2100027_TF.pdf
Attachment 3: D1100117_S2100028_TF.pdf
Attachment 4: D1100117_S2100027_Voltage_Noise_Spectrum.pdf
Attachment 5: D1100117_S2100028_Voltage_Noise_Spectrum.pdf
Attachment 6: D1100117_S2100027_Current_Noise_Spectrum.pdf
Attachment 7: D1100117_S2100028_Current_Noise_Spectrum.pdf
15773   Wed Jan 20 10:13:06 2021 gautamUpdateElectronicsHV Power supply bypassing

Summary:

Installing 10uF bypass capacitors on the High Voltage power supply line for the HV coil driver circuit doesn't improve the noise. The excess bump around a few hundred Hz is still present. How do we want to proceed?

Details

• The setup is schematically shown in Attachment #1.
• Physically, the capacitors were packaged into a box, see Attachment #2.
• This box is installed between the HVPS and the 2U chassis in which the circuit is housed, see Attachment #3.
• I measured the noise, (using the same setup as shown here to avoid exposing the SR785 input to any high voltage), for a variety of drive currents. To make a direct comparison, I took two sets of measurements today, one with the decoupling box installed and one without.
• The results are shown in Attachment #4. You can see there is barely any difference between the two cases. I've also plotted the expected noise per a model, and the measured Johnson noise of one of the 25kohm resistors being used (Ohmite, wirewound). I just stuck the two legs of the resistor into the SR785 and measured the differential voltage noise. There is a slight excess in the measured Johnson noise compared to what we would expect from the Fluctuation Dissipation theorem, not sure if this is something to be worried about or if it's just some measurement artefact.

Discussion:

So what do we do about this circuit? For the production version, I can make room on the PCB to install two 10uF film capacitors on the board itself, though that's unlikely to help. I think we've established that

1. The excess noise is not due to the Acromag or the input Acromag noise filtering stage of the circuit, since the excess is present even when the input to the HV stage is isolated and shorted to ground.
2. There was some evidence of coherence between the supply rails and the output of the HV stage (with input isolated and shorted to ground). The coherence had the "right shape" to explain the excess noise, but the maximum value was only ~0.1 (could have been because I was not measuring directly at the PA95's supply rail pins due to space constraints).
3. The impedance of 10uF at 100Hz is ~150 ohms. idk what the impedance of the supply pins of the PA95 are at this frequency (this will determine the coupling of ripples in the HVPS output to the PA95 itself.

Do we have any better bipolar HV supply that I can use to see if that makes any difference? I don't want to use the WFS supplies as it's not very convenient for testing.

Not really related directly to this work but since we have been talking about current requirements, I attach the output of the current determining script as Attachment #5. For the most part, having 220ohm resistances on the new HAM-A coil driver boards will lead to ~half the DAC range being eaten up for the slow alignment bias. For things like MC1/MC3, this is fine. But for PRM/SRM/BS, we may need to use 100ohms. Chub has ordered all manner of resistances so we should have plenty of choices to pick from.

Attachment 1: bypassCaps.pdf
Attachment 2: IMG_9079.jpg
Attachment 3: IMG_9078.jpg
Attachment 4: HVampNoise_driven_chassis.pdf
Attachment 5: printCoilCurrents.pdf
15772   Tue Jan 19 15:43:24 2021 gautamConfigurationCDSUpdated CDS upgrade plan

Not sure if 1Y1 can accommodate both c1sus2 and c1bhd as well as the various electronics chassis that will have to be installed. There may need to be some distribution between 1Y1 and 1Y3. Does Koji's new wiring also specify which racks hold which chassis?

Some minor improvements to the diagram:

1. The GPS receiver in 1X7 should be added. All the timing in the lab is synced to the 1pps from this.
2. We should add hyperlinks to the various parts datasheets (e.g. Dolphin switch, RFM switch, etc etc) so that the diagram will be truly informative and self-contained.
3. Megatron and nodus, but especially chiara (NFS server), should be added to the diagram.
15771   Tue Jan 19 14:05:25 2021 JonConfigurationCDSUpdated CDS upgrade plan

I've produced updated diagrams of the CDS layout, taking the comments in 15476 into account. I've also converted the 40m's diagrams from Omnigraffle ($150/license) to the free, cloud-based platform draw.io. I had never heard of draw.io, but I found that it has most all the same functionality. It also integrates nicely with Google Drive. Attachment 1: The planned CDS upgrade (2 new FEs, fully replace RFM network with Gen 1 Dolphin IPC) Attachment 2: The current 40m CDS topology The most up-to-date diagrams are hosted at the following links: Please send me any further corrections or omissions. Anyone logged in with LIGO.ORG credentials can also directly edit the diagrams. Attachment 1: 40m_CDS_Network_-_Planned.pdf Attachment 2: 40m_CDS_Network_-_Current.pdf 15770 Tue Jan 19 13:19:24 2021 JonUpdateCDSExpansion chassis from LHO Indeed T1800302 is the document I was alluding to, but I completely missed the statement about >3 GHz speed. There is an option for 3.4 GHz processors on the X10SRi-F board, but back in 2019 I chose against it because it would double the cost of the systems. At the time I thought I had saved us$5k. Hopefully we can get the LLO machines in the near term---but if not, I wonder if it's worth testing one of these to see whether the performance is tolerable.

 Can you please provide a link to this "list of boards"? The only document I can find is T1800302....

I confirm that PCIe 2.0 motherboards are backwards compatible with PCIe 1.x cards, so there's no hardware issue. My main concern is whether the obsolete Dolphin drivers (requiring linux kernel <=3.x) will work on a new system, albeit one running Debian 8. The OSS PCIe card is automatically configured by the BIOS, so no external drivers are required for that one.

 Please also confirm that there are no conflicts w.r.t. the generation of PCIe slots, and the interfaces (Dolphin, OSSI) we are planning to use - the new machines we have are "PCIe 2.0" (though i have no idea if this is the same as Gen 2).
15769   Sat Jan 16 18:59:44 2021 gautamUpdateLSCModulation depth measurement

I decided to analyze the data I took in December more carefully to see if there are any clues about the weird LSC sensing.

Attachment #1 shows the measurement setup.

• The PSL shutter was closed. All feedback to both lasers was disconnected during the measurement. I also disabled the input switch to the FSS Box - so the two laser beams being interfered shouldn't have any modulations on them other than the free running NPRO noise and the main IFO modulations.
• Everything is done in fiber as I had the beams already coupled into collimators and this avoided having to optimize any mode matching on the beat photodiode.
• The pickoff of the PSL is from the collimator placed after the triply resonant EOM that was installed for the air BHD experiment.
• The other beam is the EX laser beam, arriving at the PSL table via the 40m long fiber from the end (this is the usual beam used for ALS).
• I didn't characterize precisely the PLL loop shape. But basically, I wasn't able to increase the SR560 gain any more without breaking the PLL lock. Past experience suggests that the UGF is ~20 kHz, and I was able to get several averages on the AG4395 without the lock being disturbed.

Attachment #2 shows the measured spectrum with the PSL and EX laser frequency offset locked via PLL.

• The various peaks are identified.
• There are several peaks which I cannot explain - any hypothesis for what these might be? Some kind of Sorensen pollution? They aren't any multiples of any of the standard RF sources. They are also rather prominent (and stationary during the measurement time, which I think rules out the cause being some leakage light from the EY beam, which I had also left connected to the BeatMouth during the measurement).
• In the previous such characterization done by Koji, such spurious extra peaks aren't seen.
• Also, I can't really explain why some multiples of the main modulation are missing (could also be that my peak finding missed the tiny peaks)?
• The measuremet setup is very similar to what he had - important differences are
• Much of the optical path was fiber coupled.
• Beat photodiode is NF1611, which is higher BW than the PDA10CF.
• The second laser source was the Innolight EX NPRO as opposed to the Lightwave that was used.
• The RF source has been modified, so relative phasing between 11 MHz and 55 MHz is different.

Fitting the measured sideband powers (up to n=7, taking the average of the measured upper and lower sideband powers to compute a least squares fit if both are measured, else just that of the one sideband measured) agains those expected from a model, I get the following best fit parameters:

\begin{align*} \Gamma_1 &= 0.193 \pm 0.004 \\ \Gamma_2 &= 0.246 \pm 0.008 \\ \phi &= 75.5^{\circ +17.5^{\circ}}_{\, -40.3^{\circ}} \end{align*}

To be explicit, the residual at each datapoint was calculated as

$\Delta = \bigg| \frac{\rm{model}-\rm{measurement}}{\rm{model}}\bigg|^2$.

The numbers compare favourably with what Koji reported I think - the modulation depths are slightly increased, consistent with the RF power out of the RF box being slightly increased after I removed various attenuators etc. Note the large uncertainty on the relative phase between the two modulations - I think this is because there are relatively few sidebands (one example is n=3) which has a functional dependence that informs on phi - most of the others do not directly give us any information about this parameter (since we are just measuring powers, not the actual phase of the electric field).

Attachment #3 shows a plot of the measured modulation profile, along with the expected heights plugging the best fit parameters into the model. The size of the datapoint markers is illustrative only - the dependence on the model parameters is complicated and the full covariance would need to be taken into account to put error bars on those markers, which I didn't do.

Attachment #4 shows a time domain measurement of the relative phasing between the 11 MHz and 55 MHz signals at the EOM drive outputs on the RF source box. I fit a model there and get a value for the relative phase that is totally inconsistent from what I get with this fit.

Attachment 1: PLL.pdf
Attachment 2: modDepth.pdf
Attachment 3: modProfile.pdf
Attachment 4: EOMpath_postMod.pdf
15768   Fri Jan 15 17:04:45 2021 gautamUpdateLSCMessed up LSC sensing

I want to lock the PRFPMI again (to commission AS WFS). Have had some success - but in doing characterization, I find that the REFL port sensing is completely messed up compared to what I had before. Specifically, MICH and PRCL DoFs have no separation in either the 1f or 3f photodiodes.

• A sensing line driven in PRCL doesn't show up in the AS55 photodiode signal - this is good and as expected.
• For MICH - I set the MICH--->PRM actuation matrix element so as to minimize the height of the peak at the MICH drive frequency that shows up at the PRCL error point. My memory is that I used to be able to pretty much null this signal in the past, but I can't find a DTT spectrum in the elog as evidence. Anyways, the best effort nulling I can achieve now still results in a large peak at the PRCL error point. Since the sensing matrix doesn't actually make any sense, idk if it is meaningful to even try and calibrate the above qualitative statement into quantitative numbers of cross coupling in meters.
• With the PRMI locked on 1f error signals (ETMs misaligned, PRCL sensed with REFL11_I, MICH sensed with AS55_Q) - I tried tweaking the digital demod phase of the REFL33 and REFL165 signals. But I find that the MICH and PRCL peaks move in unison as I tweak the demod phase. This suggests to me that both signals are arriving optically in phase at the photodiode, which is weird.
• The phenomenon is seen also in the REFL11 signal.

I did make considerable changes to the RF source box, and so now the relative phase between the 11 MHz and 55 MHz signals is changed compared to what it was before. But do we really expect any effect even in the 1f signal? I am not able to reproduce this effect in simulation (Finesse), though I'm using a simplified model. I attach two sensing matrices to illustrate what i mean:

1. Attachment #1 is in the PRFPMI state, with the IFO on RF control (CARM on REFL11, PRCL on REFL165_I, MICH on REFL165_Q, DARM on AS55_Q).
2. Attachment #2 is between the transition to RF control (CARM and DARM on ALS, PRCL on REFL165_I, MICH on REFL165_Q). The CARM offset is ~4nm (c.f. the linewidth of ~20pm), so the circulating power in the arm cavities is low.
Attachment 1: PRFPMI_Jan12sensMat.pdf
Attachment 2: PRMI3f_ALS_Jan11_largeOffsetsensMat.pdf
15767   Fri Jan 15 16:54:57 2021 gautamUpdateCDSExpansion chassis from LHO

Can you please provide a link to this "list of boards"? The only document I can find is T1800302. In that, under "Basic Requirements" (before considering specific motherboards), it is specified that the processor should be clocked @ >3GHz. The 3 new supermicros we have are clocked at 1.7 GHz. X10SRi-F boards are used according to that doc, but the processor is clocked at 3.6 or 3.2 GHz.

Please also confirm that there are no conflicts w.r.t. the generation of PCIe slots, and the interfaces (Dolphin, OSSI) we are planning to use - the new machines we have are "PCIe 2.0" (though i have no idea if this is the same as Gen 2).

 Quote: The motherboard actually has six PCIe slots and is on the CDS list of boards known to be compatible.

As for the CX4 cable - I still think it's good to have these on hand. Not good to be in a situation later where FE and expansion chassis have to be in different racks, and the copper cable can't be used.

Attachment 1: Screenshot_2021-01-15_17-00-06.png
15766   Fri Jan 15 15:06:42 2021 JonUpdateCDSExpansion chassis from LHO

Koji asked me assemble a detailed breakdown of the parts received from LHO, which I do based on the high-res photos that Gautam posted of the shipment.

## Parts in hand:

Qty Part Note(s)
2 Chassis body
2 Power board and cooling fans As noted in 15763, these have the standard LIGO +24V input connector which we may want to change
2 IO interface backplane
2 PCIe backplane
2 Chassis-side OSS PCIe x4 card
2 CX4 fiber cables These were not requested and are not needed

## Parts still needed:

 Qty Part Note(s) 2 Host-side OSS PCIe x4 card These were requested but missing from the LHO shipment 2 Timing slave These were not originally requested, but we have recently learned they will be replaced at LHO soon

## Issue with PCIe slots in new FEs

Also, I looked into the mix-up regarding the number of PCIe slots in the new Supermicro servers. The motherboard actually has six PCIe slots and is on the CDS list of boards known to be compatible. The mistake (mine) was in selecting a low-profile (1U) chassis that only exposes one of these slots. But at least it's not a fundamental limitation.

One option is to install an external PCIe expansion chassis that would be rack-mounted right above the FE. It is automatically configured by the system BIOS, so doesn't require any special drivers. It also supports hot-swapping of PCIe cards. There are also cheap ribbon-cable riser cards that would allow more cards to be connected for testing, although this is not as great for permanent mounting.

It may still be better to use the machines offered by Keith Thorne from LLO, as they're more powerful anyway. But if there is going to be an extended delay before those can be received, we should be able to use the machines we already have in conjunction with one of these PCIe expansion options.

15765   Thu Jan 14 12:32:28 2021 gautamUpdateCDSRogue master may be doing something good?

I think the "Rogue Master" setting on the RFM network may be doing some good. 5 mins, ago, all the CDS indicators were green, but I noticed an amber light on the c1rfm screen just now (amber = warning). Seems like at GPS time 1294691182, there was some kind of error on the RFM network. But the network hasn't gone down. I can clear the amber flag by running the global diag reset. Nevertheless, the upgrade of all RT systems to Dolphin should not be de-prioritized I think.

Attachment 1: Screenshot_2021-01-14_12-35-52.png
15764   Thu Jan 14 12:19:43 2021 JonUpdateCDSExpansion chassis from LHO

That's fine, we didn't actually request those. We bought and already have in hand new PCIe x4 cables for the chassis-host connection. They're 3 m copper cables, which was based on the assumption of the time that host and chassis would be installed in the same rack.

 Quote: Regarding the fibers - one of the fibers is pre-2012. These are known to fail (according to Rolf). One of the two that LHO shipped is from 2012 (judging by S/N, I can't find an online lookup for the serial number), the other is 2011. IIRC, Rolf offered us some fibers so we may want to take him up on that. We may also be able to use copper cables if the distances b/w server and expansion chassis are short.
15763   Thu Jan 14 11:46:20 2021 gautamUpdateCDSExpansion chassis from LHO

I picked the boxes up this morning. The inventory per Fil's email looks accurate. Some comments:

1. They shipped the chassis and mounting parts (we should still get rails to mount these on, they're pretty heavy to just be supported on 4 rack nuts on the front). idk if we still need the two empty chassis that were requested from Rich.
2. Regarding the fibers - one of the fibers is pre-2012. These are known to fail (according to Rolf). One of the two that LHO shipped is from 2012 (judging by S/N, I can't find an online lookup for the serial number), the other is 2011. IIRC, Rolf offered us some fibers so we may want to take him up on that. We may also be able to use copper cables if the distances b/w server and expansion chassis are short.
3. The units are fitted with a +24V DC input power connector and not the AC power supplies that we have on all the rest of the chassis. This is probably just gonna be a matter of convenience, whether we want to stick to this scheme or revert to the AC input adaptor we have on all the other units. idk what the current draw will be from the Sorensen - I tested that the boards get power, and with noi ADCs/DACs/BIOs, the chassis draws ~1A (read off from DCPS display, not measured with a DMM). ~Half of this is for the cooling fans It seems like KT @ LLO has offered to ship AC power supplies so maybe we want to take them up on that offer.
4. Without the host side OSSI PCIe card, timing interface board, and supermicro servers that actually have enough PCIe slots, we still can't actually run any meaningful test. I ran just a basic diagnostic that the chassis can be powered on, and the indicator LEDs and cooling fans run.
5. Some photos of the contents are here. The units are stored along the east arm pending installation.

>     Koji,
>
>     Barebones on this order.
>
>        1. Main PCIe board
>        2. Backplane (Interface board)
>        3. Power Board
>        4. Fiber (One Stop) Interface Card, chassis side only
>        5. Two One Stop Fibers
>        6. No Timing Interface
>        7. No Binary Cards.
>        8. No ADC or DAC cards
>
>     Fil Clara
>
15762   Wed Jan 13 16:09:29 2021 AnchalHowToCDSAcromag wiring investigation

I'm working on a better wiring diagram that takes into account multiple power supplies, how their GND is passed forward to the circuits or sensors using those power supplies and what possible wiring configurations on Acromag would give low noise. I think I have two configurations in mind which I will test and update here with data and better diagrams.

I took some striptool images earlier yesterday. So I'm dumping them here for further comments or inferences.

Attachment 1: SimpleTestsStriptoolImages.pdf
15761   Tue Jan 12 11:42:38 2021 gautamHowToCDSAcromag wiring investigation

Thanks for the systematic effort.

1. Can you please post some time domain plots (ndscope perferably or StripTool) to clearly show the different failure modes?
2. The majority of our AI channels are "Referenced Single Ended Source" in your terminology. At least on the c1psl Acromag crate, there are no channels that are truly differential drive (case #3 in your terminology). I think the point is that we saw noisy inputs when the IN- wasn't connected to RTN. e.g. the thorlabs photodiode has a BNC output with the shield connected to GND and the central conductor carrying a signal, and that channel was noisy when the RTN was unconnected. Is that consistent with your findings?
3. What is the prescription when we have multiple power supplies (mixture of Sorensens in multiple racks, Thorlabs photodiodes and other devices powered by an AC/DC converter) involved?
4. I'm still not entirely convinced of what the solution is, or that this is the whole picture. On 8 Jan, I disconnected (and then re-connected) the FSS RMTEMP sensor from the Acromag box, to check if the sensor output was noisy or if it was the Acromag. The problem surfaced on Dec 15, when I installed some new electronics in the rack (though none of them were connected to the Acromag directly, the only common point was the Sorensen DCPS. And between 8 Jan and today, the noise RMS has decreased back to the nominal level, without me doing anything to the grounding. How to reconcile this?
15760   Tue Jan 12 08:21:47 2021 anchalHowToCDSAcromag wiring investigation

I used an Acromag XT1221 in CTN to play around with different wiring and see what works.  Following are my findings:

### Referenced Single Ended Source (Attachment 1):

• If the source signal is referenced single ended, i.e. the signal is only on the positive output and the negative side is tied to GND on the source side AND this GND is also shared by the power supply powering the Acromag, then no additional wiring is required.
• The GND common to the power supply and the source is not required to be Earth GND but if done so, it should be at one point only.
• RTN terminal on Acromag can be left floating or tied to IN- terminal.

Floating Single Ended Source (Attachment 2):

• If the source signal is floating single-ended i.e. the signal is only on the positive output and the negative output is a floating GND on the source, the the IN- should be connected to RTN.
• This is the case for handheld calibrators or battery powered devices.
• Note that there is no need to connect GND of power supply to the floating GND on the source.

Differential Source (Attachment 3):

• If the source is differential output i.e. the signal is on both the positive output and the negative output, then connect one of the RTN terminals on Acromag to Earth GND. It has to be Earth GND for this to work.
• Note that you can no longer tie the IN- of different signals to RTN as they are all carrying different negative output from the source.
• Earth GND at RTN gives acromag a stable voltage reference to measure against the signals coming in IN+ and IN-. And the most stable voltage reference is of course Earth GND.

### Conclusion:

• We might have a mix of these three types of signals coming to a single Acromag box. In that case, we have to make sure we are not connecting the different IN- to each other (maybe through RTN) as the differential negative inputs carry signal, not a constant voltage value.
• In this case, I think it would be fine to always use differential signal wiring diagram with the RTN  connected to Earth GND.
• There's no difference in software configuration for the two types of inputs, differential or single-ended.
• For cases in which we install the acromag box inside a rack mount chasis with an associated board (example: CTN/2248), it is ok and maybe the best to use the Attachment 1 wiring diagram.

Related elog posts:

Edit Tue Jan 26 12:44:19 2021 :

Note that the third wiring diagram mentioned actually does not work. It is an error in judgement. See 40m/15762 for seeing what happens during this.

Attachment 1: SingleEndedNonFloatingWiring.pdf
Attachment 2: SingleEndedFloatingWiring.pdf
Attachment 3: DifferentialSignalWiring.pdf
15759   Mon Jan 11 19:10:10 2021 ranaUpdateBHDMonte Carlo loop coupling Simulations
• looking better, but the CARM plot still looks weird.
• you should plot from 0.01 - 10,000 Hz
• All of the loops should have true integrators below 1 Hz.
• I don't think these loops are stable; the Bode plot is not a good way to check stability for LTI systems since you can be fooled by phase wrapping.
15758   Mon Jan 11 16:11:51 2021 YehonathanUpdateBHDMonte Carlo loop coupling Simulations

I dived into the alog to make the OLTFs in the MC_controls example more realistic. I was mainly inspired by these entries:

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=18742

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=20466

and Evan's and Dennis's Theses.

Attachment 1 shows the new OLTFs. I tried to make them go like 1/f around the UGF and fall as quickly as possible at higher frequencies. I didn't do more advanced stability checks.

I also noticed that imbalances and detunings in the MC simulation can change the plants significantly. Especially DARM, CARM, and sometimes PRCL. I added the option to fix some OLTFs throughout the simulation. At every iteration, the simulation computes the required control filter to fix the selected OLTFs such that it will match the OLTFs in the undetuned and balanced IFO.

Attachment 1: MC_LANCE_OLTFs.pdf
15756   Fri Jan 8 20:01:11 2021 gautamUpdateALSNoisy ALS

I did this test today. The excess noise around 100 Hz doesn't show up in the green beat.

See Attachment #1. The setup was as usual:

• X-Arm cavity length stabilized to PSL frequency using the POX locking loop.
• EX laser frequency locked to the X-Arm cavity length using the AUX PDH loop.
• The "BEATX" channel records frequency fluctuations in the beat sensed on the IR beat photodiode, while the "BEATY" channel records frequency fluctuations in the beat sensed on the Green beat photodiode.
• Since the green beat frequency fluctuations are twice that of the IR beat frequency fluctuations, I scaled the former ASD by a factor of 0.5 so as to compare apples to apples.
• At low frequencies, the green beat is noisier, but that channel doesn't show the excess noise at mid frequencies you see in the IR beat. So the AUX PDH sensing noise is not to blame I think.

So, this excess appears to truly be excess phase noise on the fiber (though I have no idea what the actual mechanicsm could be or what changed between Aug and Oct 2020 that could explain it. Maybe the HEPA?

For this work, I had to spend some time aligning the two green beams onto the beat photodiode. During this time, I shuttered the PSL, disabled feedback via the FSS servo, turned the HEPA high, and kept the EX green locked to the arm so as to have a somewhat stable beat signal I could maximize. Everything has been returned to nominal settings now (obviously, since I locked the arms to get the data).

You may ask, why do we care. In terms of RMS frequency noise, it would appear that this excess shouldn't matter. But in all my trials so far, I've been unable to transition control of the arm cavity lengths from POX/POY to ALS. I suppose we could try using the green beat, but that has excess low frequency noise (which was the whole point of the fiber coupled setup).

 Quote: How about resurrecting the PSL table green beat for the X arm to see if the non-fiber setup shows the same level of the freq noise (e.g. the PDH locking became super noisy due to misalignment etc).
Attachment 1: ALSX_IR_green.pdf
15755   Thu Jan 7 23:25:19 2021 KojiUpdateALSNoisy ALS

If the sensing noise level of the end PDH degraded for some reason, it'd make the out of loop stability worse without making the end pdh error level degraded.
It's just speculation.

15754   Thu Jan 7 21:16:22 2021 gautamUpdateALSNoisy ALS

I thought about it, but wouldn't that show up at the AUX PDH error point? Or because the loop gain is so high there we wouldn't see a small excess? I suppose there could be some clipping on the Faraday or something like that. But the GTRX level and the green REFL DC level when locked are nominal.

 Quote: How about resurrecting the PSL table green beat for the X arm to see if the non-fiber setup shows the same level of the freq noise (e.g. the PDH locking became super noisy due to misalignment etc).
15753   Thu Jan 7 20:07:27 2021 KojiUpdateALSNoisy ALS

How about resurrecting the PSL table green beat for the X arm to see if the non-fiber setup shows the same level of the freq noise (e.g. the PDH locking became super noisy due to misalignment etc).

15752   Thu Jan 7 19:16:11 2021 gautamUpdateALSNoisy ALS

I'm also wondering why the error monitors for the X and Y loops report such wildly different spectra for the suppressed frequency noise of the AUX laser relative to the cavity length, see Attachment #1. The y-axis should be approximately Hz/rtHz. In both cases, the servo's error point monitor is connected to the DAQ system via a G=10 SR560. With the SR785, I measure for EX a nice bucket-shaped spectrum, bottoming out at ~10 uV/rtHz around 40 Hz, see Attachment #2. The SR560 should have an input-referred noise much less than this at the G=10 setting. The ADC noise level is only ~5 uV/rtHz, and indeed, the EY spectrum shows the expected shape. So what's up with the EX error mon? Tried swapping out the SR560 for a different unit, no change. And both the SR560 noise, and the ADC noise, check out when everything is checked individually. So some kind of interaction once everything is connected together, but it's only present at EX...

Today, I tried switching the EX and EY fibers going into the beat mouth, but I preserved the channel mapping after the beat mouth by switching the electrical outputs as well (the goal was to make sure that the beat photodiodes weren't the issue here, I think the electronics are already exonerated since driving the channel with a Marconi doesn't produce these noisy features). The EX spectrum remains noisy. I've switched everything back to the nominal configuration now to avoid further confusion. So it would appeat that this is real frequency noise that gets added in the EX fiber somehow. What can I do to fix this? The source of coupling isn't at the PSL table, else the EY channel would also show similar features. Visually, nothing seems wrong to me at EX either. So the problem is somehow in the cable tray along which the 40m of fiber is routed? This is already inside some nice foam/tubing setup, what can be done to improve it? Still doesn't explain why it suddenly became noisy...

Attachment 1: ALS_ERR_MON.pdf
Attachment 2: AUXnoise.pdf
15751   Wed Jan 6 22:47:41 2021 gautamUpdateALSNoisy ALS

Summary:

I want to get back to locking the interferometer so I can test out the newly installed AS WFS. However, the ALS noise is far too high, at least the transition of arm length control from IR to ALS fails reliably with the same settings that worked so reliably previously. I worked on investigating it a bit today.

Timeline

In the latter half of last year, I was focused on the air-BHD setup, so I wasn't checking in on the ALS noise as regularly.

1. On Aug 17, the noise was fine.
2. But on Oct 29, the noise is bad (and it continues to remain so, to the point where I cannot lock the interferometer).
3. Koji and Anchal confirmed nothing was touched while they were investigating the ALS system, also on Oct 29. The spectra attached in #15650 don't make any sense to me, the noise at 100 Hz cannot be <100mHz/rtHz. So, inconclusive.

Excess noise:

All tests are done with the arm cavity length locked to the PSL frequency using POX. Then, the EX laser is locked to the arm cavity length using the AUX PDH servo. The fluctuations in the beatnote between the two lasers is what is monitored as a diagnostic. See Attachment #1. The reference traces in the top pane are from a known good time. The large excess noise between ~80-200 Hz is what I'm concerned about.

A separate issue that can improve the noise is to track down the noise in the 20-80 Hz band - probably some IMC frequency noise issue.

Noise budget:

See Attachment #2

• I am pretty confident the electronics after the beat mouth are not to blame - I injected a 50 MHz signal from a Marconi and adjusted the signal amplitude to mimic what we get from the beat mouth. The trace labelled "DFD electronics noise" is the noise in this config.
• The unsuppressed AUX frequency noise was measured with an SR785 (converted to freqnecy noise units knowing the PDH horn-to-horn voltage and the cavity linewidth). I didn't confirm the sensing noise level (dark noise of the AUX PDH loop), but I figure that at 100 Hz (voltage noise of ~100 uV/rtHz on the SR785), we are above the sensing noise level, and so are truly measuring the in-loop frequency noise of the stabilized AUX laser. I also confirmed that the loop UGF was ~10 kHz and phase margin was ~60 degrees, which are nominal numbers.
• The fact that the excess noise is only in the X arm channel means the PSL frequency is not to blame.

So what could it be? The only things I can think of are (i) the beat mouth photodiode (NF1611) or (ii) excess noise in the fiber carrying the light from EX to the PSL table (but only on this fiber, and not on the EY fiber). Both seem remote to me - I'll test the former by switching the EX and EY fiber inputs to the beat mouth, but apart from this, I'm out of ideas...

To avoid this kind of issue, we should really have scripted locks of all the basic IFO configs and record the data to summary pages or something - maybe something to do once Guardian is installed, it'd be pretty hacky to do cleanly with shell scripts.

Attachment 1: ALSX_excess.png
Attachment 2: budget.pdf
15750   Wed Jan 6 19:00:04 2021 gautamUpdateLSCPhase loss in POX/POY loops

I've noticed that there is some phase loss in the POX/POY locking loops - see Attachment #1, live traces are from a recent measurement while the references are from Nov 4 2018. Hard to imagine a true delay being responsible to cause so much phase loss at 100 Hz. Attachment #2 shows my best effort loop modeling, I think I've got all the pieces, but maybe I missed something (I assume the analog whitening / digital anti-whitening are perfectly balanced, anyway this wasn't messed with anytime recently)? The fitter wants to add 560 us (!) of delay, which is almost 10 clock cycles on the RTS, and even so, the fit is poor (I constrain the fitter to a maximum of 600 us delay so maybe this isn't the best diagnostic). Anyway, how can this change be explained? The recent works I can think of that could have affected the LSC sensing were (i) RF source box re-working, and (ii) vent. But I can't imagine how either of these would introduce phase loss in the LSC sensing. Note that the digital demod phase has been tuned to put all the PDH signal in the "I" quadrature, which is the condition in which the measurement was taken.

Probably this isn't gonna affect locking efforts (unless it's symptomatic of some other larger problem).

Attachment 1: POXloop.pdf
Attachment 2: loopFit.pdf
15749   Wed Jan 6 16:18:38 2021 gautamUpdateOptical LeversBS Oplev glitchy

As part of the hunt why the X arm IR transmission RIN is anomalously high, I noticed that the BS Oplev Servo periodically kicks the optic around - the summary pages are the best illustration of this happening. Looking back in time, these seem to have started ~Nov 23 2020. The HeNe power output has been degrading, see Attachment #1, but this is not yet at the point where the head usually needs replacing. The RIN spectrum doesn't look anomalous to me, see Attachment #2 (the whitening situation for the quadrants is different for the BS and the TMs, which explains the HF noise). I also measured the loop UGFs (using swept sine) - seems funky, I can't get the same coherence now (live traces) between 10-30 Hz that I could before (reference traces) with the same drive amplitude, and the TF that I do measure has a weird flattening out at higher frequencies that I can't explain, see Attachment #3.

The excess RIN is almost exactly in the band that we expect our Oplevs to stabilize the angular motion of the optics in, so maybe needs more investigation - I will upload the loop suppression of the error point later. So far, I don't see any clean evidence of the BS Oplev HeNe being the culprit, so I'm a bit hesitant to just swap out the head...

Attachment 1: missingData.png
Attachment 2: OLRIN.pdf
Attachment 3: BS_OL_P.pdf
Attachment 4: BS_OL_suppression.pdf
15748   Wed Jan 6 15:28:04 2021 gautamUpdateVACVac rack UPS batteries replaced

[chub, gautam]

the replacement was done this afternoon. The red "Replace Battery" indicator is no longer on.

15747   Sun Jan 3 16:26:06 2021 KojiUpdateSUSIMC WFS check (Yet another round of Sat. Box. switcharoo)

I wanted to check the functionality of the IMC WFS. I just turned on the WFS servo loops as they were. For the past two hours, they didn't run away. The servo has been left turned on. I don't think there is no reason to keep it turned off.

Attachment 1: Screen_Shot_2021-01-03_at_17.14.57.png
15746   Wed Dec 23 23:06:45 2020 gautamConfigurationCDSUpdated CDS upgrade plan
1. The diagram should clearly show the host machines and the expansion chassis and the interconnects between them.
2. We no longer have any Gentoo bootserver or diskless FEs.
3. The "c1lsc" host is in 1X4 not 1Y3.
4. The connection between c1lsc and Dolphin switch is copper not fiber. I don't know how many Gbps it is. But if the switch is 10 Gbps, are they really selling interface cables that have lower speed? The datasheet says 10 Gbps.
5. The control room workstations - Debian10 (rossa) is the way forward I believe. it is true pianosa remains SL7 (and we should continue to keep it so until all other machines have been upgraded and tested on Debian 10).
6. There is no "IOO/OAF". The host is called "c1ioo".
7. The interconnect between Dolphin switch and c1ioo host is via fiber not copper.
8. It'd be good to have an accurate diagram of the current situation as well (with the RFM network).
9. I'm not sure if the 1Y1 rack can accommodate 2 FEs and 2 expansion chassis. Maybe if we clear everything else there out...
10. There are 2 "2GB/s" Copper traces. I think the legend should make clear what's going on - i.e. which cables are ethernet (Cat 6? Cat 5? What's the speed limitation? The cable? Or the switch?), which are PCIe cables etc etc.

I don't have omnigraffle - what about uploading the source doc in a format that the excellent (and free) draw.io can handle? I think we can do a much better job of making this diagram reflect reality. There should also be a corresponding diagram for the Acromag system (but that doesn't have to be tied to this task). Megatron (scripts machine) and nodus should be added to that diagram as well.

 Please send me any omissions or corrections to the layout.
15745   Wed Dec 23 10:13:08 2020 gautamUpdateCDSNear term upgrades

Summary:

1. There appears to be insufficient number of PCIe slots in the new Supermicro servers that were bought for the BHD upgrade.
2. Modulo a "riser card", we have all the parts in hand to put one of the end machines on the Dolphin network. If the Rogue Master doesn't improve the situation, we should consider installing a Dolphin card in the c1iscex server and connecting it to the Dolphin network at the next opportunity.

Details:

Last night, I briefly spoke with Koji about the CDS upgrade plan. This is a follow up.

Each server needs a minimum of two peripheral devices added to the PCIe bus:

• A PCIe interface card that connects the server to the Expansion Chassis (copper or optical fiber depending on distance between the two).
• A Dolphin or RFM card that makes the IPC interconnects.
• I'm pretty certain the expansion chasiss cannot support the Dolphin / RFM card (it's only meant to be for ADCs/DACs/BIO cards). At least, all the existing servers in the 40m have at least 2 PCIe cards installed, and I think we have enough to worry about without trying to engineer a hack.
• I attach some photos of new and old Supermicro servers to illustrate my point, see Attachment #1

As for the second issue, the main question is if we had an open PCIe slot on the c1iscex machine to install a Dolphin card. Looks like the 2 standard slots are taken (see Attachment #1), but a "low profile" slot is available. I can't find what the exact models of the Supermicro servers installed back in 2010 are, but maybe it's this one? It's a good match visually anyways. The manual says a "riser card" is required. I don't know if such a riser is already installed.

Questions I have, Rolf is probably the best person to answer:

1. Can we even use the specified host adaptor, HIB25-X4, which is "PCIe Gen2", with the "PCIe Gen3" slots on the new Supermicro servers we bought? Anyway, the fact that the new servers have only 1 PCIe slot probably makes this a moot point.
2. Can we overcome this slot limitation by installing the Dolphin / RFM card in the expansion chassis?
3. In the short run (i.e. if it is much faster than the full CDS shipment we are going to receive), can we get (from the CDS test stand in Downs or the site)
• A riser card so that we may install the Gen 1 Dolphin card (which we have in hand) in the c1iscex server?
• A compatible (not sure what PCIe generation we need) PCIe host to ECA kit so we can test out the replacement for the Sun Microsystems c1ioo server?
• A spare RFM card (VMIC 5565, also for the above purpose).
4. What sort of a test should we run to test the new Dolphin connection? Make a "null channel" differencing the same signal (e.g. TRX) sent via RFM and Dolphin? Or is there some better checksum diagnostic?
Attachment 1: IMG_0020.pdf
15744   Tue Dec 22 22:11:37 2020 gautamUpdateCDSAA filt repaired and reinstalled

Koji fixed the problematic channel - the issue was a bad solder joint on the input resistors to the THS4131. The board was re-installed. I also made a custom 2x4-pin LEMO-->DB9 cable, so we are now recording the PMC and FSS ERR/CTRL channel diagnostics again (spectra tomorrow). Note that Ch32 is recording some sort of DuoTone signal and so is not usable. This is due to a misconfiguration - ADC0 CH31 is the one which is supposed to be reserved for this timing signal, and not ADC1 as we currently have. When we swap the c1ioo hosts, we should fix this issue.

I also did most of the work to make the MEDM screens for the revised ASC topology, tried to mirror the site screens where possible. The overview screen remains to be done. I also loaded the anti-whitening filters (z:p 150:15) at the demodulated WFS input signal entry points. We don't have remote whitening switching capability at this time, so I'll test the switching manually at some point.

 Quote: The main issue is that in the AA chassis I built, Ch14 (with the first channel as Ch1) has the output saturated to 28V (differential). I'm not sure what kind of overvoltage protection the ADC has - we frequently have the inputs exceed the spec'd +/-20 V (e.g. when the whitening filters are engaged and the cavity is fringing), but pending further investigation, I am removing the SCSI connection from the rear of the AA chassis.
15743   Mon Dec 21 18:18:03 2020 gautamUpdateCDSMany model changes

The CDS model change required to get the AS WFS signals into the RTCDS system are rather invasive.

• We use VCS for these models. Linus Torvald may question my taste but I also made local backups of the models, just in case...
• Particularly, the ADC1 card on c1ioo is completely reconfigured.
• I also think it's more natural to do all the ASC computations on this machine rather than the c1lsc machine (it is currently done in the c1ass model). So there are many IPC changes as well.
• I have documented everything carefully, and the compile/install went smoothly.
• Taking down all the FE servers at 1830 local time
1. To propagagte the model changes
2. To make a hardware change in the c1rfm card in the c1ioo machine to configure it as "ROGUE MASTER 0"
3. To clear the RFM errors we are currently suffering from will require a model reboot anyways.
• Recovery was completed by 1930 - the RFM errors are also cleared, and now we have a "ROGUE MASTER 👾" on the network. Pretty smooth, no major issues with the CDS part of the procedure to report.
• The main issue is that in the AA chassis I built, Ch14 (with the first channel as Ch1) has the output saturated to 28V (differential). I'm not sure what kind of overvoltage protection the ADC has - we frequently have the inputs exceed the spec'd +/-20 V (e.g. when the whitening filters are engaged and the cavity is fringing), but pending further investigation, I am removing the SCSI connection from the rear of the AA chassis.

In terms of computational load, the c1ioo model seems to be able to handle the extra load no issues - ~35us/60us per cycle. The RFM model shows no extra computational time

After this work, the IMC locking and POX/POY locking, and dither alignment servos are working okay. So I have some confidence that my invasive work hasn't completely destroyed everything. There is some hardware around the rear of 1X2 that I will clear tomorrow.

Attachment 1: CDSoverview.png
15742   Mon Dec 21 09:28:50 2020 JamieConfigurationCDSUpdated CDS upgrade plan
 Quote: Attached is the layout for the "intermediate" CDS upgrade option, as was discussed on Wednesday. Under this plan: Existing FEs stay where they are (they are not moved to a single rack) Dolphin IPC remains PCIe Gen 1 RFM network is entirely replaced with Dolphin IPC Please send me any omissions or corrections to the layout.

I just want to point out that if you move all the FEs to the same rack they can all be connected to the Dolphin switch via copper, and you would only have to string a single fiber to every IO rack, rather than the multiple now (for network, dolphin, timing, etc.).

15741   Sat Dec 19 20:24:25 2020 gautamUpdateElectronicsWFS hardware install

I installed 4 chassis in the rack 1X2 (characterization on the E-bench was deemed satisfactory, I will upload the analysis later). I ran out of hardware to make power cables so only 2 of them are powered right now (1 32ch AA chassis and 1 WFS head interface). The current limit on the +24V Sorensens was raised to allow for similar margin to the limit with the increased current draw.

Remaining work:

1. Make 2 more power cables for ISC whitening chassis and quad demod chassis.
2. Make a 2x 4pin LEMO-->DB9 cable to digitize the FSS and PMC diagnostic channels with the new AA chassis. If RnD cables has a very short turnaround time, might be worth it to give this to them as well.
3. Connect ADC1 on c1ioo machine to new AA chassis (transfer SCSI cable from existing AA unit to the new one). This will necessarily involve some model changes as well.
4. Make a short cable to connect 55 MHz output from RFsource box to the LO input on the quad demod chassis.
5. Install the WFS head on the AS table at a suitable location. Probably will need a focusing lens as well.
6. Connect WFS head to the signal processing electronics (the cables were already laid out by Jordan and I).
7. Make the necessary CDS model changes (WFS filters, matrices, servos etc). I personally don't see the need for a new model but if anyone feels strongly about separating the IMC WFS and AS WFS we can set up another model.
8. Commission the system.

While I definitely bumped various cables, I don't seem to have done any lasting damage to the CDS system (the RFM errors remain of course).

15740   Sat Dec 19 02:42:56 2020 KojiUpdate New SMA cables on order

Our favorite (flexible) RF cable is Belden's 1671J (Jacketed solder-soaked coax cable). It is compatible RG405. I'm not sure if there is off-the-shelf SMA cables with 1671J.

15739   Sat Dec 19 00:25:20 2020 JonUpdate New SMA cables on order

I re-ordered the below cables, this time going with flexible, double-shielded RG316-DS. Jordan will pick up and return the RG-405 cables after the holidays.

 Quote: As requested, I placed an order for an assortment of new RF cables: SMA male-male, RG405. x3 12" x3 24" x2 48"
15738   Fri Dec 18 22:59:12 2020 JonConfigurationCDSUpdated CDS upgrade plan

Attached is the layout for the "intermediate" CDS upgrade option, as was discussed on Wednesday. Under this plan:

• Existing FEs stay where they are (they are not moved to a single rack)

• Dolphin IPC remains PCIe Gen 1

• RFM network is entirely replaced with Dolphin IPC

Please send me any omissions or corrections to the layout.

Attachment 1: CDS_2020_Dec.pdf
Attachment 2: CDS_2020_Dec.graffle
15737   Fri Dec 18 10:52:17 2020 gautamUpdateCDSRFM errors

As I was working on the IFO re-alignment just now, the rfm errors popped up again. I don't see any useful diagnostics on the web interface.

Do we want to take this opportunity to configure jumpers and set up the rogue master as Rolf suggested? Of course there's no guarantee that will fix anything, and may possibly make it impossible to recover the current state...

Attachment 1: RFMdiag.png
15736   Thu Dec 17 15:23:56 2020 gautamUpdateASCWFS head characterization

Summary:

I think the WFS head performs satisfactorily.

• The (input-referred) dark noise level at the operating frequency of 55 MHz is ~40pA/rtHz (modelled) and ~60 pA/rtHz (measured, converted to input-referred). See Attachment #1. Attachment #5 has the input referred current noise spectral densities, and a few representative shot noise levels.
• The RF transimpedance gain at the operating frequency is ~500 ohms when driving a 50 ohm load (in good agreement with LTspice model). See Attachment #2 and Attachment #3.
• The resonant gain to notch ratios are all > 30 dB, which is in line with numbers I can find for the WFS installed at the sites (and in good agreement with the LTspice model as well).
• There are a few lines visible in the noise measurement. But these are small enough not to be a show-stopper I think.

Details and remarks:

1. Attachment #4 shows a photo of the setup.
• The QPD used was S/N #84.
• The heat sinks have a bunch of washers because the screw holes were not tappe at time of manufacture.
• There isn't space to have 8 SMA feedthroughs in the D-shaped cutouts, so we can only have the 4 "RF HI" outputs without some major metalwork.
• C9 has been remvoed in all channels (to isolate the "TEST INPUT").
2. I found that some quadrants displayed a ~35 MHz sine-wave of a few mV pk-pk when I had the back of the enclosure off (for tuning the notches). The hypothesis is that this was due to some kind of stray capacitance effect. Anyways, once I closed everything up, for the noise measurement, this peak was no longer visible. With an HP8447A preamp, I measured an RMS voltage of ~2mV rms on an oscilloscope. After undoing the 20 dB gain of the amplifier, each quadrant has an output voltage noise of ~200 uVrms (as returned by the "measure" utility on the scope, I don't know the specifics of how it computes this). Point is, there wasn't any clear sine-wave oscillations like I saw on two channels when the lid was off.
3. Some of the lines are present during some measurement times but not others (e.g. Q4 blue vs red curve in Attachment #1). I was doing this work in the elec-bench area of the lab, right next to the network switches etc so not exactly the quietest environment. But anyway, I don't see anything in these measurements that suggest something is seriously wrong.
4. In the transfer function measurements, above 150 MHz, there are all sorts of features. But I think this is a measurement artefact (stray cable capacitance etc) and not anything real in the RF signal path. Koji saw similar effects I believe, and I didn't delve further into it.
5. The dark noise of the circuit is such that to be shot noise limited, each quadrant needs 10 mA of DC photocurrent. The light bulb we have has a max current rating of 0.25A, with which I could only get 3 mA DC per quadrant. So the 55 MHz sideband power needed to be shot noise limited is ~50 mW - we will never have such high power. But I think to have better performance will need a major re-work of the circuit design (finite Qs of inductors, capacitors etc).
6. Regarding the transimpedance gains - in my earlier plots, I omitted the 50ohm input impedance of the AG4395A network analyzer. The numbers I report here are ~half of those earlier in this thread for this reason. In any case, I think this number is what is important, since the ADT-1-1 on the demod board RF input has an input impedance of 50ohm.
7. Regarding grounding - the RF ground on the head is actually isolated from the case pretty well. Two locations of concern are (i) the heat sinks for the voltage regulator ICs and (ii) the DB15 connector shield. I've placed electrically insulating (but thermally conducting) pads from TO220 mounting kits between both sets of objects and the case. However, for the Dsub connector, the shape of the pad doesn't quite fit all the way round the connector. So if I over-tighten the 4-40 mounting bolts, at some point, the case gets shorted to the RF ground, presumably because the connector deforms slightly and touches the case in a spot where I don't have the isolating pad installed. I think I've realized a tightness that is mechanically satisfying but electrically isolating.
8. I will do the fitting at my leisure but the eye-fit is already suggesting that things are okay I think.

If the RF experts see some red flags / think there are more tests that need to be performed, please let me know. Big thanks to Chub for patiently supporting this build effort, I'm pleasantly surprised it worked.

Attachment 1: oNoise.pdf
Attachment 2: Z_Hi.pdf
Attachment 3: Z_Low.pdf
Attachment 4: IMG_9030.jpg
Attachment 5: iNoise.pdf
15735   Tue Dec 15 12:38:41 2020 gautamUpdateElectronicsDC power strip

I installed a DC power strip (24 V variant, 12 outlets available) on the NW upright of the 1X1 rack. This is for the AS WFS. Seems to work, all outlets get +/- 24 V DC.

The FSS_RMTEMP channel is very noisy after this work. I'll look into it, but probably some Acromag grounding issue.

In the afternoon, Jordan and I also laid out 4x SMA LMR240 cables and 1x DB15 M/F cable from 1X2 to the NE corner of the AP table via the overhead cable trays.

15734   Mon Dec 14 11:09:28 2020 YehonathanUpdateBHDMonte Carlo loop coupling Simulations

I spent a few hours monkeying around with the control filters. They are totally made up and also it's my first time trying to design control filters.

The OLTFs of the different length controls are shown in attachment 1.

The open-loop couplings of the DOFS to DARM are shown in attachment 2.

Note that in Lance/Pytickle the convention is that CLTFs are 1/(1 - G). Where G is the OLTF.

 Quote: Cool. Can you give us Bode plots of the open loop gain for each of the 5 length control loops?

Attachment 1: MCMC_LANCE_OLTFs.pdf
Attachment 2: MCMC_LANCE_OLCoupling2DARM.pdf
15732   Fri Dec 11 09:28:52 2020 ranaUpdateBHDMonte Carlo loop coupling Simulations

Cool. Can you give us Bode plots of the open loop gain for each of the 5 length control loops?

 Quote: I have rebuilt the MCMC simulation in an OOP fashion and incorporated Lance/Pytickle functionality into it. The usage of the MCMC now is much less messy, hopefully.

15731   Thu Dec 10 22:46:57 2020 gautamUpdateASCWFS head assembled

The assembly of the head is nearly complete, I thought I'd do some characterization before packaging everything up too nicely. I noticed that the tapped holes in the base are odd-sized. According to the official aLIGO drawing, these are supposed to be 4-40 tapped, but I find that something in between 2-56 and 4-40 is required - so it's a metric hole? Maybe we used some other DCC document to manufacture these parts - does anyone know the exact drawings used? In the meantime, the circuit is placed inside the enclosure with the back panel left open to allow some tuning of the trim caps. The front panel piece for mounting the SMA feedthroughs hasn't been delivered yet so hardware-wise, that's the last missing piece (apart from the aforementioned screws).

Attachment #1 - the circuit as stuffed for the RF frequencies of relevance to the 40m.

Attachment #2 - measured TF from the "Test Input" to Quadrant #1 "RF Hi" output.

• There is reasonable agreement, but not sure what to make of the gain mismatch at most frequencies.
• The photodiode itself hasn't been installed yet, so there will be some additional tuning required to account for the interaction with the photodiode's junction capacitance.
• I noticed that the Qs of the resonances in between the notches is pretty high in this config, but the SPICE model also predicts this, so I'm hopeful that they will be tamed once the photodiode is installed.
• One thing that is worrying is the feature at ~170 MHz. Could be some oscillation of the LM opamp. All the aLIGO WFS test procedure documentation shows measurements only out to 100 MHz. Should we consider increasing the gain of the preamp from x10 to x20 by swapping the feedback resistor from 453 ohms to 1 kohm? Is this a known issue at the sites

Update 11 Dec: For whatever reason, whoever made this box decided to tap 4-40 holes from the bottom (i.e. on the side of the base plate), and didn't thread the holes all the way through, which is why I was unable to get a 4-40 screw in there. To be fair the drawing doesn't specify the depth of the 4-40 holes to be tapped. All the taps we have in the lab have a maximum thread length of 9/16" whereas we need something with at least 0.8" thread length. I'll ask Joe Benson at the physics workshop if he has something I can use, and if not, I'll just drill a counterbore on the bottom side and use the taps we have to go all the way through and hopefully that does the job.

The front panel I designed for the SMA feedthroughs arrived today. Unfortunately, it is impossible for the D-sub shaped holes in this box to accommodate 8 insulated SMA feedthroughs (2 per quadrant for RF low and RF high) - while the actual SMA connector doesn't occupy so much space, the plastic mold around the connector and the nut to hold it are much too bulky. For the AS WFS application, we will only need 4 so that will work, but if someone wants all 8 outputs (plus an optional 9th for the "Test Input"), a custom molded feedthrough will have to be designed.

As for the 170 MHz feature - my open loop modeling in Spice doesn't suggest a lack of phase margin at that frequency so I'm not sure what the cause is there. If this is true, just increasing the gain won't solve the issue (since there is no instability at least by the phase margin metric). Could be a problem with the "Test Input" path I guess. I confirmed it is present in all 4 quadrants.

Attachment 1: aLIGO_wfs_v5_40m.pdf
Attachment 2: TF_meas.pdf
15730   Thu Dec 10 22:45:42 2020 gautamUpdateSUSMore spare OSEMs

I acquired several spare OSEMs (in unknown condition) from Paco. They are stored alongside the shipment from UF.

15729   Thu Dec 10 17:12:43 2020 JonUpdate New SMA cables on order

As requested, I placed an order for an assortment of new RF cables: SMA male-male, RG405.

• x3 12"
• x3 24"
• x2 48"

They're expected to arrive mid next week.

15728   Thu Dec 10 16:24:13 2020 gautamUpdateEquipment loanNoliac PZT --> Paco

I gave one Noliac PZT from the two spare in the metal PMC kit to Paco. There is one spare left in the kit.

15727   Thu Dec 10 14:48:00 2020 YehonathanUpdateBHDMonte Carlo Simulations

I have rebuilt the MCMC simulation in an OOP fashion and incorporated Lance/Pytickle functionality into it. The usage of the MCMC now is much less messy, hopefully.

I made an example that calculates the closed-loop noise-coupling from SRCL sensing and displacement to DARM in A+. I used the control filters that Kevin defined in his controls example.

The resulting noise budget is in attachment 1. The code is in the 40m/bhd git.

I also investigated why aLIGO simulations behave so different than the A+ simulation (See few previous elogs in this thread). That is why aLIGO results are much less variable, and the simulations in aLIGO barely pass the validity checks, while A+ simulations almost always pass.

The way I check for the validity of a kat model is by scanning all the DOFs and checking that the corresponding sensing RFPDs demodulated signals cross zero. Attachment 2 shows these scanning for 3 such RFPDS for 3 cases:

A+ model with maxtem = 2

ALigo model with maxtem = 2

ALigo model with maxtem = 'off'

It seems like the scanning curves for A+ and ALigo with no HOMs are well behaved and look like normal PDH signals, while the ALigo with maxtem = 2 curves look funky. I believe that the aLIGO+HOMS curves indicate that the IFO is not really in a good locking point. All the IFO lockings were done by using the locking methods straight out of the PyKat package.

Attachment 1: MCMCLance_NoiseBudget_Example.pdf
Attachment 2: IFO_Check.pdf
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