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AdV-DAQ (Software Framework)
fiori, vajente, carbognani - 13:41 Tuesday 27 February 2018 (40686) Print this report
Bruco code now ported to CL7

 The brucoVirgo code has been modified (thanks to Gabriele) to work under CL7.  The CL7 compatible version is v1r5.

You can check it out of svn: svn co https://svn.ego-gw.it/svn/advsw/brucoVirgo/tags/v1r5

This latest version of the brucoVirgo package is now also available in  /virgoDev/brucoVirgo/v1r5/src/bruco-master

Detector Characterisation (Broadband noise)
fiori, boschi, carbognani, vajente - 17:37 Wednesday 07 June 2017 (37876) Print this report
Bruco again operational

Since about May 13th Bruco stopped working, as also noted by mwas. The problem was not an easy one, but Gabriele and Valerio managed to spot it, and Bruco is again operational. The problem was a memory overflow error associated to the processing of channels with 16384Hz sampling. After adding channels *AdcMaxVal* e *AdcMinVal* to the exclusion list BruCo runs again without problems.

The change has been checkedout in /VirgoDev/brucoVirgo/v1r2. So to run bruco now use (example):

olserver115> nice +30 /virgoDev/brucoVirgo/v1r2/src/bruco-master/bruco.py --ifo=V1 --channel=LSC_DARM --gpsb=XXXXXXXXXX --length=300 --nproc=5 --minfs=100 --outfs=10000 --naver=100 --dir=/data/procdata/web/bruco/2017-MM-GG/LSC_DARM_XXXXXXXXXX/ --top=100 --webtop=20 --xlim=10:5000 --ylim=1e-11:1e-4 --excluded /virgoDev/brucoVirgo/v1r2/src/bruco-master/share/virgo_excluded_channels_LSC_DARM.txt

The detchar doc page has been updated accordingly.

T help debugging this memory problem Franco added this python library: http://pynash.org/2013/03/06/timing-and-profiling/

In [1]: import line_profiler
In [2]: import memory_profiler
In [3]: line_profiler
Out[3]: <module 'line_profiler' from
'/virgo/InstallArea/Linux-x86_64-SL6/lib/python2.7/site-packages/line_profiler.pyc'>
In [4]: memory_profiler
Out[4]: <module 'memory_profiler' from
'/virgo/InstallArea/Linux-x86_64-SL6/lib/python2.7/site-packages/memory_profiler.pyc'>
Detector Characterisation (General)
fiori, vajente - 12:26 Thursday 09 March 2017 (36848) Print this report
BruCo software updated

The BruCo software has been updated by Gabriele to solve the following issue :

# 2017-03-08 - Virgo sampling rate is not always a power of 2, and this caused a crash
#              for some auxiliary channels with sampling rate lower than the desired
#              output. Implemented an upsamping of the aux channel to solve the issue

This latest version has been tested and installed at Cascina, see documentation page.

A minor drawback is that not physical coherence is generated for the upsampled channels at the upsampled frequencies, these shoud be ignored.

AdV-COM (AdV commissioning (1st part) )
hoak, allocca, genin, pillant, vajente - 17:51 Friday 26 August 2016 (34599) Print this report
PR-NI locked -- SIB2, SPRB, SDB2 aligned

This morning we re-locked the north arm to verify the alignment of NI was good, and then aligned the PR to overlap with the beam from NI.

In this state, with the NI misaligned, we checked the alignment of the B2 beam on SIB2.  The beam was re-centered on both PDs and the camera.  When we compare the DC signal of the B2 PDs in this configuration to the IMC transmitted power, we find a drop in coherence between 1-10Hz, see Figure 1.  Somehow the prompt reflection from the PR is not agreeing well with the transmission of the IMC.  We can see the spectrum of the B2 PDs breathing in this region, and while we were on the table we observed some dust particles flickering in the B2 beampath (which is 6W when it enters the bench).  If the disagreement between IMC_TRA and B2_DC is due to dust, we can expect the coherence to improve when we bring the bench under vacuum.  The coherence had not improved ~30min after the work on the bench had finished, so either the dust is a continuous problem or there is some additional clipping on the beam path.

In the afternoon, we locked the PRNI cavity, using first the 6MHz signal from B2 and then the 8MHz signal from the same photodiode.  The noise was largely the same, except for a large 3023Hz line in the 8MHz signal, see Figure 2.  During the lock we apparently excited the 219Hz violin mode of the PR.  Previously we had excited the harmonic of this mode at 438Hz, so I added a 219Hz notch to the PRCL locking filters and the noise was reduced, see Figure 3.

With PRNI locked, we aligned the beam on the SPRB and SDB2 benches.  On SPRB this was easy, the beam was well-centered on the optics and we improved the alignment usig the final steering mirrors before the PD and the camera.

On SDB2 there were many issues, some of which we fixed, some of which should be fixed next week:

  • The B1p beam was about 1cm too low when it exited the mini-link onto the bench.  Michal, on the phone from Annecy, used the SDB1 M4 picomotor to increase the height.  We aligned the B1p beam on the photodiode.
  • the B5 beam is offset by almost a centimeter in the horizontal direction, compared to the lens and mirrors on teh beam path.  We did not fix this, but these optics should be moved to accomodate the beam position (it is awkward to move the beam from inside the SDB1 chamber).  We centered the B5 beam on the PD, but the beam is clearly clipping somewhere.  This should be OK for locking but needs to be fixed.
  • We aligned the B1 beam on the DC PD and the camera, although this beam will need to be realigned once the 2nd OMC alignment is resolved.
  • The B1s1 and B1s2 beams are missing some photodiodes, and some of these bright beams are not dumped and exiting the table.  This is not ideal from a laser safety perspective, and probably scatters a lot of light.
  • One extra beam is dumped on the bench using a razor dump, which is certainly not clean and not vacuum compatible.  This dump should be replaced with something that doesn't risk making the in-vacuum components (on the detection bench!) dirty.
  • The B1s1 and B1s2 beams are very large on their photodiodes, at least a few mm across.  Since these beams appear to be much larger than the PDs we did not bother to center them.  Are the lenses in these beam paths not the final versions?  They are not focusing the beams as we expected.

So, the various PDs in the corner building are in a better-aligned state with respect to the arms, and we are ready to begin CITF locking. yes  The beam was cenetered on the B2 and B4 cameras, these can be used as a reference for whether the beam is centered on the PDs.  We didn't center the B5 camera since this path will be realigned.

Images attached to this report
Comments to this report:
hoak - 16:32 Saturday 27 August 2016 (34602) Print this report

Three clarifications to the original entry on bench alignments and PRNI locking:

The first plot, of the coherence between IMC TRA and the prompt reflection from the PR to B2, should be compared to this entry from June when we aligned the beam on the B2 bench.

In the second plot, the data from the PRNI lock with the B2 8MHz signal is in purple, the usual 6MHz signals is black (with red rms). Both signals have a line at 3023Hz, but it's larger in the 8MHz data.  Also the 8MHz data has a larger coupling to the 50Hz line.

The third plot shows the effect of using a notch filter to block the excitation of the 219Hz PR violin mode.  The purple data are before the notch was installed, when the mode was ringing up.  The black data are a few minutes after the notch was turned on.  Both traces were taken with PRNI locked on B2 6MHz.

Injection system (General activities)
genin, vajente - 10:33 Thursday 09 February 2012 (30637) Print this report
Laser back in operation and INJ loop closed with EIB-SAS flooting and controlled.
First, we installed the plexiglass tube between the EIB and INJ tower window. Then we relocked the PMC and sent the beam on the EIB.
The IMC was locked at the begining but when we closed the BMS the cavity get misaligned and to realign it we had to move by about 40 urad the SIB in vertical.
So it is clear that something has moved during this operation.
Activity to relock and realign the north arm is going on...
A first snapshot is given on the attached plot. A more detailled analysis will be done in the next future.
What we can just say is that as expected the structures around 45Hz and 18Hz have been removed.
Note that to reduce as much as possible to low frequency beam jitter we had to leave the Acoustic enclosure door open.
Images attached to this report
Comments to this report:
genin - 10:34 Thursday 09 February 2012 (30638) Print this report
Purple curve: signals with EIB-sas.
Black curve: signals with old EIB support.
Injection system (General activities)
genin, marque, ruggi, tacca, vajente, swinkels - 18:19 Tuesday 07 February 2012 (30633) Print this report
Injection system final tuning.
Today we worked on the Injection system to finalize the alignment of the RFC and recenter BMS quadrants.
We had a bit of troubles to relock the RFC and this turned out to be mainly related to mistuning of the 6MHz modulation frequency.
After retuning it, we could easily relocked the RFC. Finally, the fine alignment could be made.
THe BMS quadrants have been manually recentered and the loop close properly. In order to avoid air current problems that were affecting the good functionning of IMC AA and BMS, we had to let open on door of the EIB acoustic enclosure.
Note that 6MHz modulation frequency has been retuned and CalibFModerr macro has been launched and the calibration factor updated in IB DSP card.
Length Sensing and Control (North cavity locking)
swinkels, vajente - 17:00 Thursday 03 November 2011 (30472) Print this report
Non-linear lock acquisition with reduced force
This morning, we did another test for AdV by locking the north-cavity with reduced actuation force. This time, the algorithm was not implemented in the DSP as before, but in Global Control (CavityTest algorithm, GcLocking v2r14p1). The idea is that when the cavity sweeps through a resonance, you measure the velocity using the Pound-Drever signal and then apply one positive and one negative rectangular shaped impulse, which are applied even after the cavity gets out of resonance. The length of the impulses is calculated so that the cavity arrives in minimum time back at the position of the resonance with velocity close to zero. When the transmission of the cavity is above a certain threshold, a standard linear feedback is then switched on. More details will be given at Wednesday's ISC meeting. After the tests, we restored the old situation.
Images attached to this report
Length Sensing and Control (North cavity locking)
ruggi, vajente, passuello, calloni - 19:10 Wednesday 19 October 2011 (30431) Print this report
Low force mirror damping
A new algorithm for the locking of a cavity has been tested. The goal was to control the mirror using a small force applied from the reaction mass, not larger than the one really needed.
The algorithm has been developed in the DSP. In order to do that, the two communication channels from Gc to DSP has been used to send the power and the demodulated signal (position error signal) acquired by the photodiode in transmission at the end of the north cavity. In the following plots, Sc_NE_pow is equivalent to Pr_B7_DC, and Sc_NE_sig is equivalent to Pr_B7_ACp/Pr_B7_DC (the normalization increase the linear range of the error signal).

As a first step, a pure derivative damping has been implemented and tested.
The velocity signal is computed by filtering the position error signal by a zero@0 and a pole@200Hz.
A force proportional to the velocity is sent in feedback to the RM coils.
The computation of the velocity is limited to the crossing time of the resonance (a trigger on the power is used); out of resonance, the signal does not make sense, and v is kept as a constant at its latest computed value.

The force starts to be applied when the
The application period of the force is limited too, but the window is larger (the triggerOut is very low).
The available force is limited to a value which is about 300 times lower than the maximun provided by the present actuation setup. In this way we want to test the possibility to use smaller magnets for Advaced VIRGO mirrors.

In figure 1 we see a successful locking attempt: the cavity stays close to the resonance for 2 seconds, while the loop keeps the velocity at zero. The position signal is expressed in microns, the velocity in um/s, the correction in uN.

In fig 2 a zoom of the first instant of the lock acquisition is shown. When the action is triggered, the requested force exceeds the limit, and it is kept constant during the first crossing of the resonance. But this force is enough to reverse the motion, and the resonance is crossed again with a lower speed. A second full-dynamic action is applied in the opposite direction for a while, then the signal enters the linear regime and the loop is closed.

to be continued...
Images attached to this report
Mirror Suspension Control (Mirror Suspension Control)
Vajente - 11:06 Tuesday 20 September 2011 (30325) Print this report
Actuation noise in LN1
This morning the ITF was locked with coil drivers in low noise 1. We switched at low noise 2 at about 7.55 local time. We saw a significant increase of horizon (plot 1) and sensitivity. Second plot shows there was an improvement even below 10 Hz.

The third plot compares the sensitivity (in meters) of this morning in LN1 and LN2, calibrated using the most recent calibration TFs available. The black curve is an estimate of the level of LN1 actuation noise, obtained requiring its sum with LN2 curve to match the LN1 curve.

The best matching noise has a f^-3 slope with a value of 1.4e-17 m/rHz at 10 Hz.
Images attached to this report
Comments to this report:
ruggi - 11:03 Wednesday 21 September 2011 (30333) Print this report
The situation described in this entry is not reproducible by switching manually the actuators to LN1. Many configuration has been tested, and no similar excess of actuation noise has been observed.
Length Sensing and Control (SSFS Noise)
Vajente - 9:12 Thursday 15 September 2011 (30302) Print this report
Out-of-loop measurement of B5 shot noise
Looking at tonight coherences I discovered that B1 shows some (small) coherence with B2_d2_ACp at almost all frequencies (see first plot). B2 is expected to be sensitive to frequency noise. Therefore one can use it as an out-of-loop measurement of residual frequency noise, which is B5 shot noise.

The second plot shows a projection in dark fringe of B2_ACp using the measured coherence. In the same plot I also put the standard projection of B5 shot noise we obtain from frequency noise injections (see for example Measurement of frequency noise coupling).

There is very good agreement, meaning that
1) our estimation of B5 shot noise is correct
2) SSFS electronic does not introduce additional noise
Images attached to this report
Detection system (Detection system)
Vajente, Marque - 18:14 Tuesday 13 September 2011 (30286) Print this report
Motivation for switch between Lo1 and Lo3
Last night, some non stationarities could be observed in the sensitivity as reported in the Gabriele's entry 30283: some noise appearing and disappearing around 60-70Hz. These periods of extra noise are well visible in the signal Pr_B1_ACq_diff23 (see first plot, xaxis is wrong by one hour and a half due to a bug of datadisplay, plot actually starts at 00H00).
Looking at the difference betwwen both photodiodes on both quadratures, it looks like the noise comes from the demodulation of B1_d3 (see second plot).
We went to the detection lab and were able to trig such period of noise by touching the BNC connector which make the connection between the Lo signal and the B1_d3 demodulation board. Indeed, this connector seems a bit loose.
This connector is now bringing the Lo signal to the B1_d1 demodulation board.
Images attached to this report
Detection system (Detection system)
Vajente, Marque - 16:17 Tuesday 13 September 2011 (30285) Print this report
Lo3 / Lo1
Interferometer_sensitivity_studies (General)
Vajente - 8:46 Tuesday 13 September 2011 (30283) Print this report
New horizons
Last week interventions had a good result on the interferometer. This night we stayed stably above 12 Mpc and reached 13 Mpc for some long periods. High mass horizon reached 150 Mpc. See first plot.

The second plot compares the best sensitivity of this night with one of the best obtained during VSR4. There is a clear broad-band improvement below few kHz.

There are some periods of reduced sensitivity visible in the horizon trend, which seems associated with an increase of noise between 50 and 80 Hz, see last plot. The origin is not understood yet.
Images attached to this report
Injection system (General activities)
genin, vajente - 9:48 Monday 12 September 2011 (30278) Print this report
PMC matching adjustment to remove glitchs in the Injection system.
The mathcing on PMC cavity worsened in the last days. The consequence was some glitches at the output of IMC cavity due to saturation of Pstab loop.
In order to improve a bit the matching and remove these glitches we have play with the pumping configuration of the laser amplifier.
Now we have: I1=I2=52.5A and I3=I4=45.5A.
As you can see on the plot no glitch is visible anymore but we have not improve that much the matching this means that the problem should appear again in the next days/weeks. Next action should be to adjust the telescope between the laser amplifier and the PMC cavity to significantly improve the matching on the PMC.
Images attached to this report
Length Sensing and Control (Recombined ITF locking)
Tacca, Vajente - 10:57 Wednesday 07 September 2011 (30260) Print this report
Procedure tolock PR-NI
We had to revise the algorithm to lock PR-NI. It used to trigger on B7_DC, which is not available today (valves are closed).

We changed the TwoLengths code to trigger on a rescaled, reversed version of B2_DC (GcLocking v2r13p5). Two new onfly parameters are available in Sensing to create the trigger signal:

trigger = Trigger_Offset + Trigger_Gain * B2_DC

Current working parameters are
Trigger_In = 0.7
Trigger_Offset = 8.4
Trigger_Gain = -83

PROCEDURE

To lock the PR-NI, commit the following algorithm in database:
Gc/Locking/Locking_Half 1.37
Gc/Locking/Sensing/PR_NI 1.91
Gc/Locking/Filtering/PR_NI_INT 1.7
Gc/Locking/driving/PR_NI 1.11

We updated the AlpGC macro LOCK_PR_NI_WITH_B2.
Images attached to this report
Length Sensing and Control (SSFS Noise)
Vajente - 14:42 Tuesday 06 September 2011 (30249) Print this report
Measurement of frequency noise coupling
This morning I injected some noise into the SSFS loop to measure again the coupling of frequency noise to dark fringe.
Here are GPS times:

Clean data
Time: Sep06,11-08:00:00 -> GPS: 999324015
Time: Sep06,11-08:10:00 -> GPS: 999324615
DARM noise (ampl. 1e-13
Time: Sep06,11-08:15:43 -> GPS: 999324958
Time: Sep06,11-08:20:54 -> GPS: 999325269
Frequency noise ampl
Time: Sep06,11-08:24:15 -> GPS: 999325470
Time: Sep06,11-08:30:40 -> GPS: 999325855

The first plot compares the CMRF measured today with one measurement done at the beginning of August. Beware the units are arbitrary here. The shape is completely different.

Second plot shows a projection of frequency noise and B5 shot noise into the sensitivity. Both are far from being limiting.
Images attached to this report
Detection system (Detection system)
Vajente - 7:48 Friday 02 September 2011 (30222) Print this report
No results on 2Khz noise
Images attached to this report
Detection system (Detection system)
Vajente - 18:06 Thursday 01 September 2011 (30219) Print this report
Investigations on 2kHz noise
Detection system (Detection system)
Vajente - 14:59 Thursday 01 September 2011 (30216) Print this report
More on 2 kHz noise
Following Didier's observation in Less HF glitches between Aug11 and Aug18, I had a look at what happened around the time when the 2kHz bump disappeared and re-appeared.

The times are correlated with changes in the demodulation phase of B1_d3 photo-diode. It is however not connected to the phase being tuned or mis-tuned, but apparently only on the absolute value of the phase shifting asked to B1_Lo3. Before August 11 and after August 18 the dephasing was between 0 and -20 and the noise was present. In between these two times the dephasing was around -180 and the noise was not there.

In conclusion, it seems that the noise coupling depend on the dephasing asked to B1_Lo3 board. I do not understand how this can happen, unless there is some strange malfunctioning of the board itself.

We might try to make a short experiment rotating the phase and see if we can switch on or off the noise.
Images attached to this report
Online Data Analysis (Omega)
Vajente - 13:36 Monday 29 August 2011 (30198) Print this report
(30196)
The region between 457 and 464 Hz is crowded by a large number of violin modes (very narrow spectral lines due to the resonance of the monolithic fibers suspending the arm cavity mirrors. 4 mirrors times 4 fibers per mirror makes at least 16 lines). Since mirrors and fibers are very similar one to the other, these lines are very close in frequency. The variation of the BRMS computed over a 2 Hz wide band is expected to contain all the beating frequencies between the violin modes.
Detection system (Output Optics)
Genin, Vajente - 10:10 Tuesday 23 August 2011 (30149) Print this report
SFP fine realignment
This morning we went to the detection lab to realign the scanning Fabry-Perot that was slightly misaligned.
Fine tuning has been done at step 8.
Detection system (Detection system)
Vajente, Marque - 15:51 Thursday 18 August 2011 (30124) Print this report
B1 setup moved back to External Detection Bench
This morning, we removed the B1 setup from the little bench attached to the detection tower and re-installed it on the External Detection Bench (as it was up to August 9th, see 30068).
After 10 days taking data in this configuration, it was clear that there was no improvement at any frequency due to the shortening of the optical path in air (120cm -> 55cm).
There was however a worsening of the sensitivity around 90Hz. These bumps disappeared when the setup has been moved back to the EDB (plot1).
On the same plot, one can see that another bump around 65Hz, which has always been present, disappeared after this morning intervention (?).
Looking at the coherence with the seismometer attached to the detection tower, there is no clear evidence but some indication that these bumps may be due to backscattered light from the B1 setup.
Images attached to this report
Detection system (Detection system)
Vajente, Marque - 14:40 Wednesday 17 August 2011 (30119) Print this report
(30109)
We changed the configuration of Lo25 to assign the name B1_Lo1 instead of B1_Lo5 to the phase shifter now attached to B1_d1.
Mirror Suspension Control (Mirror Suspension Control)
Carbognani, Vajente - 9:05 Wednesday 17 August 2011 (30115) Print this report
Glitches at NE
Yesterday afternoon we surveyed the NE building while the suspensions was shaken by electromagnetic glitches. We very likely found the culprit to be one high power relay in one of the vacuum racks which was commuting from time to time. The cause triggering the relay to switch is likely related to the turbo pump failure.

We found good correlation with the glitches seen on filter 0 LVDT. Vacuum people were contacted and switched off the rack. We had no more glitches since yesterday afternoon. Let's anyhow collect a bit more statistics.
Mirror Suspension Control (Mirror Suspension Control)
Vajente, Tacca - 16:30 Tuesday 16 August 2011 (30111) Print this report
Glitches at NE suspension
The long series of unlocks of this night were caused by the "electromagnetic" glitches at NE, alredy reported in Unlocks due to electro-mechanical glitches at the NE.

These glitches can start appearing at any time and last for few hours. They are making lock acquistion impossible even in this moment. More investigations are needed to understand their origin, but so far there is no solution.

To identify them look at fast glitches in NE_F0 LvdT signals (without downsampling them!), as shown in the attached plot. Please check if unlocks are caused by these glitches before contacting any on-call person, since there is no known solution except waiting for the glitches natural disappearance.
Images attached to this report
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