I have made scripts that we can run that will adjust the a2l gains for PR2 and PR3.  These use the same a2l engine that the test mass script does, it just sets the settings for PR2 and PR3.  They can be found in the same location (just checked in): .../userapps/isc/common/scripts/decoup/a2l_min_PR*.py, where * is either 2 or 3. 

Each script has been run tonight, so we now have non-zero a2l elements for both those mirrors.

I tried to set up an acoustic injection that reproduced several of the bumps in DARM (last time I only did one shaker bump) and tried PR2 pitch, yaw and length injections and IM2 pitch. The best was PR2 pitch, see attached figure. The behavior at other bumps was similar.

I ran the current version of the calibration pipeline over a stretch of O1 data to reproduce the kappas and compare to those in the C02 frames.
The filters file used was aligocalibration/trunk/Runs/O1/GDSFilters/H1DCS_1131419668.npz, as suggested by the calibration configuration page for O1:
https://wiki.ligo.org/viewauth/Calibration/GDSCalibrationConfigurationsO1#LHO_AN2
The agreement looks quite good. Time series plots of the kappas and the cavity pole are attached. The start time used here was 2016-10-04 12:41:19 UTC (GPS 1127997696).

• Locked at NLN for a bit
• PI mode 26 was a bit of trouble, once. Matt twiddled some inout and output gains. Phase seemed right. That one has been in-check pretty well.
• PI mode 18 has been a bit of an ongoing issue.
• ran a2l at about 3:15UTC
• wind - not an issue
• uSei riding at just below the 905ile as a mean.
• no EQs
• Robert running injections when locked

alog 30897 has links to SRCL, PRCL and MICH BruCo's. Here hare some interesting highlights from those graphs:

SRCL:

IMC-MC2_YAW_OUT_DQ

IMC-WFS_B_Q_PIT_OUT_DQ

IMC-WFS_B_Q_YAW_OUT

IMC-WFS_B_I4_ERR_DQ

Sure looks like our SRCL sensing is limited by input YAW jitter below maybe 25Hz.

BTW: MICH sees the same noise: CAL-CS_MICH_DQ

PRCL:

This looks like all our PRCL noise is jitter in the recycling cavity...

ASC-POP_A_PIT_OUT_DQ

( ASC-POP_A_NSUM_OUT_DQ ... PIT is more than SUM ...

  ASC-POP_A_YAW_OUT_DQ ... or YAW. )

Also interesting:

SUS-MC2_M1_ISIWIT_L_DQ

ISI-HAM3_SUSPOINT_MC2_EUL_L_DQ

HPI-BS_L4CINF_V2_IN1_DQ

ISI-HAM3_ISO_RY_IN1_DQ

I attached all plots for archiving purposes.

Ed, Patrick and Jenne

Apologies if this is a repeat, but I've never seen this and was at a noticeable loss for action to take.

After the Lockloss at 23:30UTC, there was a diag main message that indicatd that ISC_LOCK wasn't going anywhere until the Fast Shuttter was tested. I'm making a Wiki in Troubleshooting H1 to address what to do in this situation. Jenne came to the rescue. Thanks Jenne!

Took well over 60 minutes to overfill CP3 by doubling LLCV to 36% open first, then open a little bit more, then a bit more, until finally it overfilled, I will change the setting LLCV from 18 to 20%.

Matt E., Dave, Jenne, Jeff K. and I tracked the problems with PI down to settings not being restored or not being restored correctly by SDF after the reboot on Tuesday. It is unclear if the problem with SDF was human or computer error. Jeff K. and Matt reverted the PI settings to those from a week ago. It appears that mode 27 is now back under control.

15:00 UTC Robert to end X to perform injections while at NLN
15:52 UTC Lock loss (PI mode 27). Tried changing sign of gain and turning off damping to no effect.
15:52 UTC Christine and Karen to mid stations
15:54 UTC Kyle to end X
15:54 UTC Robert back
15:56 UTC Robert to end Y to pickup hardware
16:15 UTC Changed to VERY_WINDY_NO_BRSXY
?         Robert back
16:19 UTC Pausing at violin mode damping 2 waiting for roll modes to damp.
16:33 UTC Kyle back. Checked that RGA does not have a leaky valve. It does not.
16:50 UTC Karen leaving mid Y
16:52 UTC mode 27 starting to rise
16:59 UTC Lockloss
Changed to WINDY during CHECK_IR
17:46 UTC Stopping at VIOLIN MODE DAMPING 2 again.
17:59 UTC King soft water through gate to check RO
18:04 UTC Changed BP filter for mode 26 from FM1 to FM8. Changed the set frequency to 207.8 from 207.7
Changed set frequency for mode 27 from 244 to 240.
18:08 UTC Turned on output to mode 27 damp filter
18:15 UTC Changed BP filter for mode 26 back to FM1. Changed the set frequency to 209.
18:19 UTC Daniel to LVEA
Changed set freq for mode 18 from 207.9 to 207.8
18:45 UTC Daniel back
19:02 UTC Struggling to lock PRMI. Starting initial alignment.
19:10 UTC G Wave candidate alert
19:14 UTC Daniel to floor (WP 6294). Says I am going to lose the MC. Aborting initial alignment and setting ISC_LOCK node to DOWN.
19:43 UTC Daniel back. Restarting initial alignment.
20:19 UTC Initial alignment done
20:41 UTC Stopped at DC readout. Diagnosing PI and SDF.
22:44 UTC PI settings reverted. Going to NLN.

Discovered that the error point of the first ISS loop was changed to PDB about 23 hours ago. Why? Changed it back to PDA.

• H1 was locked for a couple of hours before I came in and just lost lock 23:19UTC
• winds are negligible
• uSei is up to 90%ile
• from that chatter coming from the operator pit, PI seems to be the topic of discussion.
• CDS looks fine
• VAC looks ok
• no EQs to speak of

J. Kissel

I'm not sure why, but INJ EPICs "settings" channels that are used to store, news, state and time information have become re-monitored in the SDF system, which means that the CAL-CS model shows differences when an external alert arrives and/our when a standard hardware injection goes through. I had removed the monitoring of these channels before O1 had started last year -- see LHO aLOG 21154 -- so I don't know why these have suddenly come back into monitoring. Merp. They're back to being ignored by the SDF system as they should be.

Kyle, John 

In and out of X-end VEA.  Energized RGA filament and ran RGA just long enough to confirm that the Kr cal-gas isolation valve wasn't leaking at that the 5 x 10-4 torr*l of Krypton that I had dumped into the X-end had dissipated below detectable limits - OK all traces of Kr are gone.

Matt Daniel Fil (WP 6294)

The MCL and MCF readbacks have a 10/100 Hz Sallen-Key whitening stage which amplifies the high frequency spectrum to get above ADC noise. Since a while we have observed a 20-50 mHz/√Hz flat noise level in the these spectra when we are locked with the IMC only. Looking with the oscilloscope we estimated about 10m V signal between 100 kHz and 1 MHz, before the whitening. This seems too much for the AA board, so we included additional low pass filters in the readbacks with cut-offs around 15 kHz. A 15/150 kHz pole-zero was added to the Sallen-Key, and another 15 kHz pole was added to the output stage.

In detail (common mode board, IMC, s/n 1102626):

• Stuffed a 3.3 nF into C293 and C241
• Mounted a 330 pF on top of C295 and C243.

The attached spectra now show a frequency noise level which is compatible with the one observed in full lock. The coherence is also improved. The ADC noise is not too far away in regions with reduced coherence.

Notes:

0) A2L gains of order two are getting suspicious, because it essentially means some coils are shut off.

1) ITMY_Y2L was always large (~-2) , but since 10/29 7UTC it is even bigger.

2) ITMX_Y2L also got big (~2) on 10/29 7UTC

Not sure what to make of this...

WP#6255 and WP#6293 completed  

0930 hrs. local -> Valved-in RGA turbo to RGA volume and energized filament.  

1130 hrs. local -> Took scans of the RGA volume with and without cal-gases -> isolated RGA turbo from RGA volume -> combined RGA volume with X-end volume and took scans of the X-end with and without calibration gases (inadvertently dumped ~5 x 10-4 torr*L of Krypton or 2 hrs accumulation @ 5 x 10-8 torr*L/sec into site) -> vented RGA turbo and removed from RGA hardware -> installed 1 1/2" UHV valve in its place -> Pumped volume between two 1 1/2" valves to 10-4 torr range before decoupling and de-energizing all pumps, controllers and noise sources with the exception of the RGA electronics which was left energized and with its fan running 24/7.

Leaving RGA exposed to X-end, filament off and cal-gases isolated.  Will post scan data as a comment to this entry within next 24 hrs..