Attached are plots of the cooling related signals from around the time of the laser trip on ~midday Sunday. The minimum head flow rate was set to be 0.5 lpm as a precaution because the front end and power meter circuit flow meters were disabled. From the XChilFlow_v_Head4 plot it looks like the flow rate in head 4 was down on its way beyond 0.5 lpm and then the crystal chiller shutdown, as it was supposed. The plots {In,Out}letPressure_v_Head4Flow show the pressures in the water manifold at the same time. The pressure oscillations occur as the chiller was shutting down and not before it. XChil_v_H4, {In,Out}P_v_H4 are plots for the Sunday afternoon laser trip. Again consistent with the flow rate in head 4 dipping below the trip threshold.
Removed check valve from CP4 exhaust and installed a thermocouple up inside the pipe several feet. Signal is being read out via H0:VAC-MY_CP4_TE252B_DISCHARGE_TEMP_DEGC. Tomorrow I'll overfill CP4 and collect temp data.
Kiwamu Daniel
With ISS PD A mounted in the main path we measured the spectrum of the second loop ISS. The attached plot shows a clear improvement in the signal sent to the inner loop ISS. The red curve is a representation of the new control signal, whereas the dark red curve is representing the old configuration. The second loop out-of-loop sensor also sees improvements (black against gray) between 600 Hz and 4 kHz. The jitter out of the HPO is unchanged. The measurements were done at 54W into the IMC.
WP 6234
FRS 4504
Installed D1300642 HWWD electronics for ITMX and ETMX. Units installed in monitor-only mode.
1. Units were powered up
2. DB37 cables connected
3. DB9 cable connected from HWWD chassis to binary input chassis
4. Three BNC cables were pulled to SEI ISI coil drivers
ISI coil drivers need to be replaced with modified units that will enable the HWWD electronics to power off the coil drivers.
Serial numbers of units installed.
ITMX - S1500333
EX - S1301706
Peter, Kiwamu,
We have taken out the PD A photodiode out of the ISS inner loop box and placed it at a location where the PWR_EOM photodiode was. We confirmed that we can close the loop with the moved PD A.
[New setup]
We opened up the inner loop box and removed the base plate on which the two photodiodes sat. Then we took out only PD A from the base plate while leaving PD B mounted on the base plate. We put the base plate back into the inner loop box. A black glass beam dump was placed at the location where PD A used to be. Careful: because we could not find a good screw hole, we could not clamp down the black glass beam dump which is currently just sitting on the base plate.
We placed PD A to the location where PWR EOM (Thoralbs PDA55) had been. We rerouted all the associated cables for PD A (a 5 pin lemo, 2 normal lemos) to the new location. We measured the beam power at this location to be 8 mW. Because this is too much for PD A (which we think typically runs with 1 mW), we installed an ND filter on the front panel of PD A (see the picture).
A few more pictures are available at ResourceSpace.
[ISS loop closed with PD A]
Here shows a screenshot of the setup for closing the inner loop with PD A. The gain slider needed to be a 12 dB higher (which still smells like a factor of two calibration error...) than the usual. The ref signal for PD A needed to be -0.46.
Here are some plots of the open loop transfer function with PD A used as the in-loop sensor. A gain of more than 20-30 dB in the gain slider actually does not do the job -- needs more investigation. The ugf is about 46 kHz with the gain slider set to 30 dB. Note that when PD B was in use, the ugf had been 54 kHz (29942).
Intend to confirm that CP3 isn't overfilling following today's delivery via observing absence of vapor at exhaust at some point before leaving today (It's similar to a sentence - only without all of the unnecessary comprehension!)
I lowered it again to 17% because the last length of the exhaust pipe was frosty and LN2 was trickling out. (this is Chandra, not Bubba)
State of H1: in Maintenance, 18 Work Permits in progress / done
Activities: (Corey 8:00-10:38(15:00-17:38UTC))
As of 18:00UTC (11:00PT) Work in progress: (Cheryl)
Activities Since (UTC):
Work that continues:
as of 22:18:
I selected nine periods of ten minutes during last night's locks (see fig. 1). For each period I computed the transfer function from jitter (as measured by the diagnostic brteadboard Q1Y signal) to DARM. The second figure shows that the coupling indeed changes over time.
I used the period martked as (4), which correspond to the largest coupling, fit a transfer function and used it in the time domain to perform jitter subtraction for all nine periods. The third figure shows the reduction in DARM noise: clearly the filter works well for period (4), but the performance is significantly degraded for the other periods.
In conclusion, if we want to subtract the jitter noise, we'll need some level of adaptive filtering.
After Jason had to fill the TCSY chiller this morning he and I decided to make another round of water leak inspections. We "poured" (pun intended) over the inside of the table enclosure, including removing a few table panels in order to carefully look behind some things. We found no water leaks. We then crawled the LVEA length of piping under the chambers and up to the wall junction and also found nothing. We inspected the flow meter area under BSC2, nothing. And so we keep filling a bit every dayish...
J. Betzwieser, D. Barker, D. Tuyenbayev,
Overview
Updated the h1calcs model to include modifications from LLO, restarted the DAQ system (LHO WP #6238). Now H1 and L1 are running the same version of the CAL-CS model.
Details
CTRL_DELAY
filter bank was added to the DELTAL_CTRL
signal path, before the summation with DELTAL_RESIDUAL
(see LLO alog 28268).BUFFER_AND_AVERAGE.c
, currently using version of the script in CDS SVN r14393 (see LHO alog 30293).After the DAQ restart the coherence calculation settings were changed to:
Number of averages: H1:CAL-CS_TDEP_COH_BUFFER_SIZE 13
Seconds between averages: H1:CAL-CS_TDEP_COH_STRIDE 10
The new CTRL_DELAYfilter is currently empty (unused), and the DELAY_CYCLES (ring buffer / integer delay cycles) is set to 7.
The synchronized oscillators in the CAL-CS time-dependent parameter and coherence calculations were restarted manually. This is a necessary step to get correct phases in the oscillators after a model restart (a bug is described in LHO alog 30220).
WP 6235:
We added a feedforward path from the DBB QPDs to the LSC DARM or LSC REFL_DC_BIAS. There are new filters name H1:PSL-DBB_FF_QPD1X, 2X, 1Y and 2Y, followed by a matrix H1:PSL-DBB_FF_QPDMAT. Then the signal is sent to the LSC model, where there is a filter module H1:LSC-JITTERFF followed by an output matrix H1:LSC-JITTERFF_MAT. The signal is then added to either the DARM error point, or sent to the REFL_DC_BIAS output.
In the LSC model the temporary third loop ISS which is now defunct was deleted and the EXTRA_AO_3 path restored. The hardware was also disconnected.
We also noticed that the REFL_DC_ERR and COMM_A_RF_ERR paths were swapped. The same was true for REFL_A_RF9_ERR and REFLAIR_A_RF9_ERR. They should be correct now. The REFL_DC_BIAS output is directly connected to the REF_DC_ERR input. If we need dewhitening we should switch this to the excitation input.
WP 6239:
The model part for the second loop ISS QPD was changed to one which supports the whitening filter switching.
I restarted the primary and redundant calibration pipelines at Hanford at gps time 1160244770. Based on tests, the current latency is ~5-7 seconds. This restart picked up the latest release gstlal-calibration-1.0.5, with bug fixes for a "time-reversal" errors and (hopefully) the overlapping frame bug. The filters file used can be found in the calibration SVN: aligocalibration/trunk/Runs/PreER10/GDSFilters/H1GDS_1159648300.npz The new filters contain the updated calibration line frequencies, so the kappas should be correctly computed once we enter a lock stretch. For more information on the filters, see this aLOG: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=30210 Below is the command line used to run the pipeline: gstlal_compute_strain --data-source=lvshm --shared-memory-partition=$LIGOSMPART --filters-file=$filter_file --ifo=H1 --frame-duration=4 --frames-per-file=1 --write-to-shm-partition=$HOFTSMPART --compression-scheme=6 --compression-level=3 --control-sample-rate=4096 --expected-fcc=341.0 --partial-calibration
To remove missing ISI & HEPI DACKILL widgets--WPs 6217 & 6227. SUS & IOP DACKILLs not touched.
ECR E1600042 WP 6217; ECR E1500325 WP 6227
To Remove DACKILL elements from HAM ISIs and HEPIs:
HAM ISI
.) Removed DACKILL Widgets on WD Block--Attachment 1.
.) Removed DACKILL link from WD Block to the ERRMON Block--Attachment 2.
.) Routed WD_STATE from WD Block to ERRMON--Attachment 2.
.) Added WD_STATE Logic in ERRMON Block for Rogue Excitation Evaluation--Attachment 3.
HEPI
.) Removed DACKILL elements from HEPI (Top) Level--Attachment 4.
.) Removed DACKILL parts on WD Block--like ISI Attachment 1.
To update HEPIs to Bleedoff-Accumulated-Saturations feature running on ISIs for months:
.) Add WINDOWTIME inputs on HEPI WD Block--Attachment 5.
.) Removed Test Point pickoffs WD Flag channels--also on Attachment 5.
.) Replace model saturation counter on WD/IPS, L4C & ACT Blocks with WD_SATCOUNT_vb.c counter & bleedoff Function--Attachment 6 becomes Attachment 7, e.g.
JimB restarted all these models after the build and install. Reisolation was not a problem. HAM2 did have one trip on CPS during 1st isolation attempt but it worked fine on the 2nd...
SVN COMMITS:
/opt/rtcds/userapps/release/isi/common/models/
hugh.radkins@opsws1:models 0$ svn commit -m "Removed DACKILL remenants & wired WD_STATE to ERRMON"
Sending models/isihammaster.mdl
Transmitting file data .
Committed revision 14424.
/opt/rtcds/userapps/release/hpi/common/models
hugh.radkins@opsws1:models 0$ svn commit -m "Added sensor/actuator WD Saturation Bleedoff ala ISI & removed Test Point WD Flag channels"
Sending models/hepitemplate.mdl
Transmitting file data .
Committed revision 14425.
Still have some medm and SDF cleanup to do. In progress.
Yes I do know how to spell remnants!
I've edited the HEPI and ISI Watchdog medms getting rid of the DACKILL widgets that do not connect to anything now. Also added the IOP DACKILL to the HEPI screen which were absent. Also removed is the RESET ALL button as all it did was push the DACKILL and the RSET buttons. Only 1 WD reset button remains, RESET WD. CLEAR SATURATIONS ONLY button is on the ISIs, pretty self explanitory there. On the HEPIs, I elected to not add the Clear Saturations Only infrastructure as the RESET WD button will do the trick anyway and won't harm the platform if it is not tripped. The RESETs for the IOPDACKILL and the Rogue Exc WD on the ISIs still need to be done in addition to the RESET WD, if, the medms suggest (red) they need it. There is no Rogue Excitation Watchdog on the HEPIs.
I will commit these medms to the SVN when I confirm that LLO does not need the RESET ALL button.
Corey informed me that he was getting low water level alarms on the TCS chillers. I went out to investigate and found the following:
WP6240:
The TwinCAT code has been updated on all interferometer Beckhoff machines. Three new features were added related to error reporting:
The svn version on the end stations is 3185, whereas the corner is 3186.
At the request of DetChar, I have reviewed the LHO PSL ODC thresholds for relevancy now that the HPO is operating. The threshold for Bit 12 (PMC Transmission Limit OK) was still set to 11.5W, which was ~50% of the PMC transmitted power during O1 but is now too low for an operational HPO. Keeping the 50% of output intact, I changed the threshold to 50W; I chose 50W as that is roughly 50% of our current 101W transmitted by the PMC. I accepted the change in the PSL PMC SDF.
This completes WP #6243.