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Reports until 15:07, Friday 02 February 2018
H1 PSL
jason.oberling@LIGO.ORG - posted 15:07, Friday 02 February 2018 (40391)
PSL HPO Diode Box Tweaks

Thomas informed me that the PSL ISS was having issues.  Upon investigation I found the HPO was only outputting ~117W.  To keep the laser running for the remainder of the day, I tweaked the pump diode operating temperatures for DB1 and increased the operating current of DB2, 3, and 4 from 59.0A to 59.7A.  The output power of the HPO increased to 131.0W; this also cleaned up the ISS, which was oscillating because of the low power out of the HPO.

H1 CDS
david.barker@LIGO.ORG - posted 13:43, Friday 02 February 2018 - last comment - 15:37, Friday 02 February 2018(40390)
managing two versions of svn code while working directories are being upgraded

During the upgrade process, some local working directories on the CDS file system will still be using the old 1.6 svn version, and others will be using the upgraded 1.8 version.  Remember that the two versions are completely incompatible (in both directions).

The CDS workstations now have version 1.8 svn code installed in the default svn location (/usr/bin/svn). To permit running the 1.6 code if and when needed, please create an alias in your .bashrc file

alias svn1.6="/ligo/apps/debian8/subversion-1.6-17/bin/svn"


This is only a temporary work around, eventually all working directories will be migrated to 1.8.

IMPORTANT NOTE: when viewing a 1.6 working directory with a 1.8 svn program, the system may suggest you upgrade the directory using the 'svn upgrade' command.

Please do not do this!

In the upgrade process I am resolving local modification, adding files which should be under config control, and making sure files which are cluttering up the old working directories do not migrate to the new directories.

Comments related to this report
david.barker@LIGO.ORG - 15:37, Friday 02 February 2018 (40392)

I've changed the CDS standard environment such that your default svn client should now be /usr/bin/svn (version 1.8).

If your svn code version does not match that which was used to create the working directory you are in, you will get an error message. The exact message differs for the different combinations of client-code/working-directory versions. In order to understand this, we must first understand the basic differences in the working-directory meta-data layout between SVN1.6 and SVN1.8.

In the old SVN1.6, every directory under the top level directory has a .svn directory. In SVN1.8, the .svn directory only exists in the top level directory, there are none in the lower directories.

If you are running client svn1.6 and looking at a SVN1.8 created working dir, then at the top level the client sees the .svn and sees that it has the wrong version. You get the error message

svn: The path '.' appears to be part of a Subversion 1.7 or greater
working copy.  Please upgrade your Subversion client to use this
working copy.


However, if you navigate to lower directories, because they don't have .svn meta-data directories (this is SVN1.8), then client svn1.6 gives the bogus error

svn: warning: '.' is not a working copy

Now onto the second case of running client svn1.8 and looking at a SVN1.6 created working dir. Each sub directory has a .svn dir (this is SVN1.6), so at every level you get the message

svn: E155036: Please see the 'svn upgrade' command
svn: E155036: The working copy at '/opt/rtcds/userapps/trunk/cds_1.6/h1'
is too old (format 10) to work with client version '1.8.10 (r1615264)' (expects format 31). You need to upgrade the working copy first.
 

(again,please  do not do an 'svn upgrade')

H1 ISC (ISC)
marc.pirello@LIGO.ORG - posted 13:25, Friday 02 February 2018 - last comment - 11:24, Monday 05 February 2018(40389)
Corner 4 & Corner 6 Channels Repaired

Elizabeth C., Marc P.

Taking advantage of a one hour window in operation we repaired the Corner 4 and Corner 6 squeezer readbacks per WP7309

In Corner 4 we replaced module 19 on the left rail with a new EL3104 (4 channel differential ADC)

In Corner 6 we replaced module 5 on the right rail with a new EL1124 (4 channel digital input)

Both of the replaced modules appear to be working.

Comments related to this report
daniel.sigg@LIGO.ORG - 15:44, Friday 02 February 2018 (40393)

ASC-AS_B_RF42_DEMOD_LOMONCHANNLE_3/4 is fixed.

H1:ISC-RF_C_AMP42M4_POWEROK still reads zero. Maybe a cabling problem?

marc.pirello@LIGO.ORG - 11:24, Monday 05 February 2018 (40413)

Fil C., Marc P.

It was a indeed an internal wiring problem.  We moved the wires to the correct positions on the beckhoff terminal and verified OK1 through OK12 are working as intended.

H1 CDS
david.barker@LIGO.ORG - posted 12:03, Friday 02 February 2018 - last comment - 13:11, Friday 02 February 2018(40385)
AS WFS45 code changes installed on h1asc0 and h1lsc0

WP7227

Daniel, Sheila, Dave:

New models for h1asc, h1ascimc, h1lsc and h1omc were installed. DAQ was restarted.

Comments related to this report
david.barker@LIGO.ORG - 12:20, Friday 02 February 2018 (40386)

DAQ changes are shown in attached text files.

Non-image files attached to this comment
david.barker@LIGO.ORG - 13:11, Friday 02 February 2018 (40388)

there was a problem in h1ascimc.mdl with the bus-selector for the ADC inputs to the top-named ASC part. This was fixed and the h1ascimc model was restarted at 13:08PST

H1 SQZ (SQZ)
sheila.dwyer@LIGO.ORG - posted 12:01, Friday 02 February 2018 (40384)
OPO M1 swap aborted

Sheila, Nutsinee, (with Lisa and Fabrice on the phone)

Yesterday afternoon we made prepared to swap the M1 mirror for the higher 532 reflectivity version.  I pulled the low finesse mirror out of the cavity, but then noticed that the high finesse mirror isn't usable because of glue on the back of the optic.  We put the original mirror back in using the tooling that Fabrice sent.  There are spots for two alignment pins to be used in installing the mirrors, Fabrice had only used one of the pins (the front one) in constructing the cavity.  I found it easier to place the mirror such that I could see cavity flashes without the pin in place.  The pin is now in the bag with the tooling in case we want to use it for a future swap.  

I placed the mirror without moving the green beam which had originally been alinged to the cavity, to get cavity flashes, but then adjusted the input alingment for both red and green to get a good alignment into the cavity. 

Fabrice and Lisa are making another attempt at gluing today at MIT, so we might have one more chance to swap the optic. 

H1 PSL (PSL)
peter.king@LIGO.ORG - posted 05:53, Friday 02 February 2018 (40381)
Laser trip
Came into the Control Room this morning to find that the laser had tripped off from the power watchdog.  Looking at
the trend data suggested that it tripped around 2:30 am.  Had some minor problems bringing the laser back on, whereby
the Beckhoff computer was not responding.  Opted to reboot the computer.  It came back without any problems.  The
laser restarted okay afterwards, with the output power considerably down from yesterday (as indicated on the main
user screen).  I opted to increase the diode currents.

    The  power watchdogs are currently OFF.
Images attached to this report
H1 TCS (TCS)
greg.grabeel@LIGO.ORG - posted 18:36, Thursday 01 February 2018 (40376)
CO2X&Y status

CO2X faulted out due to a chiller issue. I suspect the pzt servo control loop, as the integrator seems to do a weird count up issue and eventually try to set the chiller set point too high and cause the chiller to exceed its limit and shutdown. Both CO2X and Y are doing this. For now that control loop is shutoff.

Also, the CO2X power monitor isn't working correctly and is showing a 20.9 A with a ~0 V reading on the laser, but a quick check on the power supply shows 28V and ~0.7A reading which is consistent with the laser on standby. 

Images attached to this report
H1 AOS (SQZ)
terry.mcrae@LIGO.ORG - posted 17:55, Thursday 01 February 2018 (40374)
Step Motor Waveplate rotators installed on ISCT6

Nutsinee, Sheila, Daniel

The 4 D9 cables (H1:ISC_SQ_394, H1:ISC_SQ_395, H1:ISC_SQ_396, H1:ISC_SQ_397) from the patch panel to the picomotor four axis breakout boxes had to be replaced for low profile versions as the ends of the custom D9 cables were too fat to fit to the patch panel (see attachment).

Note some of the connections from the breakout boxes to the picomotors are currently inconsistent with with the schematic D1700384. The working arrangement is listed below.

H1:ISC_SQ_394   PSL fibre pol 1/2 1X, PSL fibre pol 1/4 1Y, PSL power 1/2 2X  (ok)

H1:ISC_SQ_395   CLF 1/2 2X,  CLF 1/4  2Y, Green fibre pol 1/2 1X, Green fibre pol 1/4 1Y (different to schematic)

H1:ISC_SQ_396   CLF power 1Y, Green Power 1/2 1X (different to schematic)

Also the software for the Step rotator on SQZT6 is currently inoperative.

Images attached to this report
H1 IOO (IOO)
cheryl.vorvick@LIGO.ORG - posted 17:41, Thursday 01 February 2018 - last comment - 00:08, Friday 02 February 2018(40373)
second camera on HAM2 West door aligned, first camera pointing slightly changed

second camera: I aligned the camera on the upper right viewport on HAM2 West door to the calcite wedge on the input of the IO Faraday.

first camera: I maintained a view of baffle HA1 (downstream of IM1) on the camera on the upper left viewport on HAM2 West door, but shifted the view of the camera upward in real space, to capture the double aperture on the beam path to the ISS Array.

Comments related to this report
cheryl.vorvick@LIGO.ORG - 23:07, Thursday 01 February 2018 (40378)

To check out the new camera view of the CW, I drove IMs and PRM and I broke the IMC to get a single bounce off of MC2, and relocked the IMC with no issues, and all optics are back where they started, as seen in the attached screenshot, which has the live alignment screen on the left, and the screenshot I took before I started, with it's time stamp, on the right.

 

Images attached to this comment
cheryl.vorvick@LIGO.ORG - 00:06, Friday 02 February 2018 (40379)IOO

images: as seen on the camera, misaligned PRM, as seen on camera: PRM intentionally clipping on the SiC baffle (0.7W): the shot, or an approximation, through the IM1 tower: the shot, showing the bottom of the specialized CW mount through IM1's tower: the CW in it's mount, not the same angle but close.

Images attached to this comment
cheryl.vorvick@LIGO.ORG - 00:08, Friday 02 February 2018 (40380)

first two camera images are rotated 90 deg counterclockwise from the display on the CRT

LHO VE
kyle.ryan@LIGO.ORG - posted 16:47, Thursday 01 February 2018 (40372)
"Switching Error" found on Y-end purge-air drying tower
During a routine check of the Y-end purge-air supply today, I found that the drying tower had a "switching error" with the Left tower regenerating and the Right tower drying.  I reset this and confirmed that both towers were switching normally.  Hmmm..  Chandra also had this happen in the past but the issue seems to be intermittent - with long periods of no errors detected.  For now I will try and check this on a daily basis as opposed to every few days.  

Also, the current demand for purge-air from the VE is resulting in an output pressure of 0.8 psig.  Even so, the skid is alternating between 3 - 4 compressors.  I'll try and revisit if the programmed pressure set points at which the PLC adds addition compressors is easily changed.  If so, I would like to see fewer compressors running for this, relatively modest, demand.  
H1 ISC (ISC)
thomas.vo@LIGO.ORG - posted 16:27, Thursday 01 February 2018 - last comment - 12:56, Friday 02 February 2018(40370)
Done aligning HAM6 OMC Trans Path

Keita, Corey, TVo

We finished aligning the OMC Trans path, it was quite difficult to lock the OMC, even with purge air turned down, but Keita was able to lock long enough for me to trace the beam to the viewport emulator.  Keita will post a picture of the beam position in the emulator.

Yesterday we quoted a beam clearance for the fast shutter wire with the shutter closed, we've repeated the measurement with the shutter open and found that the clearance is grater than 12-13 mm, Keita wil post a picture of this as well.

We also took a ton of pictures of the table for future references, Corey will post pictures as a comment.

At the end of the day, we turned up the purge air and took the viewport emulator back down and placed it southwest of the PSL enclosure where Jason and I found it yesterday. 

Comments related to this report
corey.gray@LIGO.ORG - 21:53, Thursday 01 February 2018 (40377)

Photographic highlights from today's HAM6 work (names of photos describe the photos).

Images attached to this comment
keita.kawabe@LIGO.ORG - 09:49, Friday 02 February 2018 (40383)

Other pictures.

IMAG1031~2 (1st picture): Clearance between the FS wire and the beam when the FS is open.

IMAG1036~2 (2nd): One pair of FS wires ("continuity test" or some such) with a clear kapton tubing for insulation.

IMAG1008 (3rd): OMC TRANS beam is at the top corner of the card TVo is holding.

IMAG1010 (4th): SiC beam dump.

IMAG1012 (5th): OM1, high power beam dump and other things.

IMAG1017 (6th): OM3 and FS.

IMAG1019 (7th): OM3 and 1st OMC REFL steering mirror.

IMAG1020 (8th): OM2.

IMAG1023 (9th): AS WFSs and sled.

IMAG1024 (10th): Two OM3 trans steering mirrors for AS WFS sled.

IMAG1025 (11th): OMC trans steering mirror.

IMAG1026 (last): 2nd OMC REFL steering mirror.

 
Images attached to this comment
anamaria.effler@LIGO.ORG - 12:56, Friday 02 February 2018 (40387)

The neat thing is that now both OM1's (L1 and H1) seem to want to be about 2 inches off in the -X ifo direction. So at least we're consistent? See LLO alog about OM1 here: LLO alog 37279 and compared to drawing D1000342.

H1 AOS (ISC)
thomas.vo@LIGO.ORG - posted 11:57, Thursday 01 February 2018 - last comment - 18:11, Thursday 01 February 2018(40363)
IMC Open Loop Gain Changed

Sheila, TVo

I had trouble locking the IMC yesterday when increasing the input power.  So we measured the OL TF at the Common Mode board and found that the UGF was about 100 kHz with maybe 20 degrees phase margin while locked at 1 W.  So we changed the guardian common mode gain calc by -4db to get a little more phase margin and match what Kiwmau's suggestion was in aLOG-36354 of about 50 kHz nominal, it now stably working at 10W.  I've attached the plots of different power levels input into the IMC.

Images attached to this report
Comments related to this report
kiwamu.izumi@LIGO.ORG - 18:11, Thursday 01 February 2018 (40375)

blush

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