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Reports until 16:38, Tuesday 26 January 2016
H1 SEI
filiberto.clara@LIGO.ORG - posted 16:38, Tuesday 26 January 2016 (25180)
CPS Sync Fanout Install
Ran new cables at EX for CPS sync fanout install. Cables are run from SUS-R1 rack to CPS units on chamber. Fanout chassis and RF cable (71MHz) still need to be installed/pulled.

Filiberto C. & Ed M.
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 16:33, Tuesday 26 January 2016 - last comment - 14:39, Wednesday 27 January 2016(25179)
CDS maintenance summary

New lab dust monitors

Jeff B, Jim, Dave [WP5697]

As part of the install of the new OSB lab dust monitors:

generated new autoBurt.req file. Generated new DAQ EDCU INI file. Recanned conlog against autoBurt.req file.

New GDS version

Jim [WP 5696]:

completed this morning.

Clearing partially loaded filter modules

Was able to do full loads on susbs, susitmx, susitmy, susprm, sussrm. Still have partial loads on lsc, omc, suspr2 and sussr2 which are waiting for the system experts to clear.

DAQ reconfigure

DAQ EDCU was reconfigured for the missing h1tw0 and new DUST channels. Was applied during today's two DAQ restarts.

DAQ Restarts

In both DAQ restarts the dataconcentrator, tw1 and both framewriters started with no issues. In the first restart the broadcaster started by both NDS daqd process were no longer controlled by monit. A simple monit restart of the daqd processes cleared the error. On the second restart the broadcaster started, stopped and later restarted. Again both NDS processes did not start, and when they were restarted they failed. The error was that high dcuid nodes for the Beckhoff SDF system has been mistakenly added to the testpoint.par file, and only the NDS machines objected to this. The file was repaired and monit was able to restart the NDS daqd processes.

TCS model changes

Aidan and Dave [WP5688]:

Installed new h1tcscs model onto h1oaf0. DAQ was restarted.

New Beckhoff SDF code release

Jonathan [WP5695]:

Jonathan tested the new code on EY Beckhoff. He found an issue with enumerated binaries and backed this version out.

RACCESS monitoring/control of h1hwinj1

Jonathan, Jim, Dave:

Jonathan added the hardware injection machine h1hwinj1 to his RACCESS control system. MEDMs were updated accordingly.

H1OAF change to drive audio in control room

Richard, Evan, Dave [WP5704]:

h1oaf and h1pemcs models were changed to permit oaf to drive the 8th DAC channel of PEM's 18-bit DAC card. This analog signal is then routed from the CER to the control room using the audio channel in the digital video fiber link between the rooms.

New operator table install in the control room

Richard, Carlos, Jim, Dave:

The new powered, adjustable-height operator table was installed in the control room at the operator station. The access control PC, gate cam and alarm machines were shuffled to the left and a new workstation was installed on the new table.

HPI and ISI safe.snap work

Hugh, Dave:

Hugh worked on the safe.snap files for HPI and ISI. I was able to offer some help by creating a new script to convert sub-systems to safe SDF mode and converted all HPI and ISI to safe. Later I converted them back to OBSERVE mode.

New ECAT EPICS channels for corner station

Daniel, Dave:

Daniel made Beckhoff changes in the corner station. I updated the ECAT DAQ INI files and the target autoBurt.req files.

Server patching and rebooting

Carlos, Dave:

Carlos applied security patches and rebooted cdsssh, cdslogin and cdsadminctrl. We restarted the vacuum alarms system on cdslogin.

 

 

 

 

Comments related to this report
david.barker@LIGO.ORG - 14:39, Wednesday 27 January 2016 (25207)

Note that at the time the DAQ was restarted during Tuesday's maintenance the DAQ dataconcentrator and both frame writers had been running continuously for 55 days 20 hours with no problems.

H1 SUS
filiberto.clara@LIGO.ORG - posted 16:29, Tuesday 26 January 2016 (25175)
ETM Low Voltage ESD Driver units modified
Installed Whitening Board (D1500389) to ETM Low Voltage Driver Chassis (D1500129) per ECR E1500417.

ETMY LV Driver S1500066
- Whitening board installed S1600032


ETMX LV Driver S1500073
- Whitening board installed S1600035

High voltage was disabled prior to disconnecting of any cables. Verified outputs were not railing when units were reinstalled. One thing worth noting, is that the wiring for the binary cables is not consistent at both end stations. For now, we left cables in the same configuration we found them this morning.

Filiberto C. & Ed M.
H1 General
cheryl.vorvick@LIGO.ORG - posted 16:24, Tuesday 26 January 2016 (25178)
Maintenance Day Summary:

Day Shift: 16:00-23:59UTC (08:00-16:00PT)

State of H1: down all day, down more than 12 hours, currently JimW at EY to fix ESD driver

Shift Summary:

Activities logged in alogs 25155, 25163, and 25171

Other activities:

H1 CDS
jonathan.hanks@LIGO.ORG - posted 16:22, Tuesday 26 January 2016 (25177)
Maintenance activities

Two items:

H1 CDS
jonathan.hanks@LIGO.ORG - posted 16:20, Tuesday 26 January 2016 (25176)
SDF on slow controls update was rolled back
I started updating the slow controls SDF models to the latest version in trunk.  This was to fix a bug Daniel saw after the power outage.  Unfortunately there were problems with the channel type detection code so we fell back to running the old code again.

I have left the work permit open, I will debug, test, and deploy later.
H1 SUS
cheryl.vorvick@LIGO.ORG - posted 16:18, Tuesday 26 January 2016 (25174)
oplev trends for 7 days

Images attached to this report
H1 CDS
patrick.thomas@LIGO.ORG - posted 15:21, Tuesday 26 January 2016 (25173)
Conlog restarted
Crashed earlier in the day, I'm guessing with the Beckhoff restart:

Jan 26 13:07:00 h1conlog1-master conlog: ../conlog.cpp: 301: process_cac_messages: MySQL Exception: Error: Out of range value for column 'value' at row 1: Error code: 1264: SQLState: 22003: Exiting.

Dave updated the channel list to remove the dust monitor channels.
H1 CDS (ISC)
evan.hall@LIGO.ORG - posted 15:00, Tuesday 26 January 2016 (25172)
Audio output for LSC signals

Richard, Dave, Evan

We added infrastructure in the OAF model to take LSC error signals, filter them, and output them to an 18-bit DAC channel in the PEM frontend. This signal is then piped into the control room and can be played on a speaker.

MEDM screeens still need to be made.

Images attached to this report
H1 General
cheryl.vorvick@LIGO.ORG - posted 14:53, Tuesday 26 January 2016 (25171)
as of 22:52UTC (14:52PT) Maintenance winding down: some listed here are done/suspended until the next Maintenance opertunity

 1           h1psl             PSL.team                 HPO optic exam                 x113   00:02:19
 2      ISC/IO/ALS              Richard      add sensors to all tables                  202   00:01:19
 3            TCSY             Alistair             startup TCSY laser                  202   00:01:19
 4      LVEA crane                Bubba     shim rails - requires lift                  202   00:00:48
 5             TCS       Aidan/Alastair                 install/modify                  202   00:01:21
 6      optics lab                Betsy                           work                  212   00:02:19
 7      ESD drives         filiberto/ed                      EX and EY                  212   00:02:38
 8           mid-y           john/bubba               check cryo pumps                  202   00:02:43
 9              EY                 Kyle                    check pumps                  202   00:02:48
10             OAF            Dave+Evan new oaf and pem, audio testing                  202   00:03:44

 

H1 General
cheryl.vorvick@LIGO.ORG - posted 14:45, Tuesday 26 January 2016 (25163)
Maintenance Day as of 21:25UTC (1:25PT)
List of reservation system - some times are longer than the task is expected to take

 1           h1psl             PSL.team                 HPO optic exam                 x113   00:03:40
 2      ISC/IO/ALS              Richard      add sensors to all tables                  202   00:02:40
 3            TCSY             Alistair             startup TCSY laser                  202   00:02:40
 4      LVEA crane                Bubba     shim rails - requires lift                  202   00:02:09
 5             LN2             company?               delivery on site                  202   00:01:03
 6             TCS       Aidan/Alastair                 install/modify                  202   00:02:42
 7      optics lab                Betsy                           work                  212   00:03:40
 8      ESD drives         filiberto/ed                      EX and EY                  212   00:03:59

H1 SEI
hugh.radkins@LIGO.ORG - posted 14:33, Tuesday 26 January 2016 (25169)
All ISI & HEPI HPI safe.snaps checked and updated as required.

Before bringing the SEI platforms back up.  Checked the diffs with the safe.snaps in SDF.  There were a few chages related to GS13 gains and FF ON/OFFs.  All updated and committed to svn.

H1 SEI
hugh.radkins@LIGO.ORG - posted 14:25, Tuesday 26 January 2016 (25168)
LHO HEPI Fluid System Accumulators Checked--All Good--None needed Charging

Brought all the SEI Platforms down and spun down the HEPI Pumps to check the Accumulator charge.  Most accumulators showed a few PSI drop--likely from pressure gauge loss.  No charge dropped to action level.  It was mid July last time this was done.  This suggests none of the accumulators are leaking.  I'll check again in a couple months--checking the pressure sometimes loosens the valve and it can start leaking.

H1 SEI
jenne.driggers@LIGO.ORG - posted 13:59, Tuesday 26 January 2016 (25164)
Some ISI SDFs accepted last night - may be reverted if desired

In anticipation of going to Observe last night (which didn't happen due to a lockloss sometime just before 1am), I had accepted some ISI SDF diffs while JimW was still here to approve them. I'm sure he'll look at his data more, and make a final decision on whether we should keep the sensor correction changes or not, but for now the Guardian will probably put the EY ISI back in its old nominal state, so we'll see a bunch of SDF diffs when we get to NomLowNoise.  Anyhow, I attach a screenshot of what I accepted, and we can re-accept the old values later today, until Team SEI decides to change the Guardian.

Images attached to this report
H1 SYS
daniel.sigg@LIGO.ORG - posted 13:24, Tuesday 26 January 2016 - last comment - 10:39, Thursday 28 January 2016(25162)
Corner TwinCat System updated

Updated the corner TwinCAT system to the most recent svn. This includes the changes needed for adding the ASC-AS_A/B.RF90 channels.

The new AS_B.RF90 demod channels won't be active until the corner 4 chassis is upgraded. The AS_A.RF90 demod channels have been taken over from the old (now deleted) AS_D. Whitening channels for both AS_A and AS_B are working.

Comments related to this report
daniel.sigg@LIGO.ORG - 10:39, Thursday 28 January 2016 (25224)

Added whitening screens for AS_A/B_RF90 to ISC-CUST_WHITENING_OVERVIEW.adl

Added related screen buttons for AS_A/B_RF90 to ASC_OVERVIEW.adl

H1 CDS
james.batch@LIGO.ORG - posted 09:35, Tuesday 26 January 2016 (25156)
Install new GDS software for control room
WP 5696, ECR 1500402

The version of GDS software for the control room has been updated to branch gds-2.17.1.3.  This release addresses several Bugzilla bugs regarding data access, especially NDS2 data access.  

A new NDS2 input section has been added which will allow the user to specify an epoch start and end time, which will limit the channel list to those that existed during the epoch.  For those channels whose data rate was changed without changing the name, it will be possible to specify an epoch where only a single data rate exists.  (This assumes the user knows the time that the data rate changed.)  If multiple channel rates for a channel exist during the chosen epoch, those rates will be displayed when channels are selected.  Because of the way NDS2 returns data, it is still possible to get incorrect data if you choose a data rate for a time when the data really doesn't exist, so it's best to narrow the epoch to display only a single data rate for the channel.

Diaggui now warns you if you don't have a kerberos ticket when attempting to use the NDS2 input.

A release note document has been generated for the GDS tools, see T1600007.
H1 General
cheryl.vorvick@LIGO.ORG - posted 09:10, Tuesday 26 January 2016 (25155)
Maintenace Day: started a bit before 8AM, ongoing now, expected to be about 8 hours

Current activities:

 1           h1psl             PSL.team                 HPO optic exam                 x113   00:04:57
 2        HAM4/TCS         Filiberto/Ed               cables 4 hartman                  202   00:03:14
 3          CPS/PI              Richard     cabling for CPS, status PI                  202   00:03:17
 4            HEPI                 Hugh       CS HEPI check - all down                  202   00:03:24
 5         Sprague                  Joe            check all buildings                  202   00:03:26
 6   dust monitors                JeffB                   modify pumps                  202   00:03:32
 7      ISC/IO/ALS              Richard      add sensors to all tables                  202   00:03:33
 8            TCSY             Alistair             startup TCSY laser                  202   00:03:33
 9      LVEA crane                Bubba     shim rails - requires lift                  202   00:03:54

Alarm Test:

H1 DetChar (DetChar, ISC, PEM)
andrew.lundgren@LIGO.ORG - posted 21:50, Sunday 24 January 2016 - last comment - 14:49, Tuesday 26 January 2016(25134)
Small glitches on second boundaries
There are small glitches very close to each second boundary in the ETMY drive signal and the ETMY SUS ad SEI rack magnetometers.

In order to investigate the half-Hz combs in DARM (see alog 20790), I took an hour of data and folded it with a four-second period. If there is a repeated glitch at any multiple of this period, it should become far more visible. The result is that in several channels, there are glitches very near the boundary of each GPS second. The peak time of these glitches seems to be about 10 milliseconds after the start of the second. The glitch does not repeat identically every second. There is one shape in the first second, then one with an opposite polarity in the next second.

The first two attached plots are for the SUS and SEI racks, which are shown with a 40-Hz zero-phase lowpass. The SUS has a narrow spike, and the negative spike is larger than the positive one. The SEI signal is more complicated. The ETMY L3 MASTER signal, which is the DARM output to the ESD, is shown with a 10 to 50 Hz bandpass. These glitches are more like sine-Gaussians, but the even and odd seconds still seem to have opposite polarities.

There are more channels with similar glitches. We can make a more thorough investigation, and use more data and more times, to try to track down the origin of these glitches. Hopefully these glitches are responsible for the 0.5 Hz combs such that removing them will improve those.
Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 12:27, Tuesday 26 January 2016 (25160)CDS, DetChar
J. Kissel

Tagging CDS in this entry. 

I'd recently taken a look at the requested output of the ETMY L1 stage,
${IFO}:SUS-ETMY_L1_MASTER_OUT_*_DQ
and was interested to find ~1 [Hz] combs in the requested output. Though this isn't the 0.5 [Hz] combs that Andy mentions above, I think it's an excellent place to take the investigation further in a more focused manner -- with the point being that even the SUS's *requested* signal has a comb.

Attached is a 100-sec FFT ASD, of a typical, 1000 [sec] stretch of observation-ready data during the run (2016-01-04 04:00 UTC). Here, to give a feel for the physical amplitude of these signals: at 30 [Hz] the noise amplitude of one of these comb peaks is roughly 1e-3 [ct/rtHz] of requested DAC output, which corresponds to 
1e-3 [ct/rtHz] * (20.0 [V] /2**18 [ct]) = 7.6e-8 [V/rtHz] @ 30 Hz ( * sqrt(2 * 0.01) = 1.1e-08 [V_pk])

Potentially verifiable / refutable Crack-pot Theories / Wild guesses:
- Perhaps there is some of this glitching in the inter-process communication (IPC) on the reflected memory (RFM) data transfer from the corner to the end station, that's only exposed for requested drives that have such a huge dynamic range? For whatever channels in the signal chain that are stored, can you reproduce the same combs by filtering those channels offline?
- Recall that the power supplies for the Hartmann Wavefront Sensor (HWS) were replaced some time ago, see Integration Issue 1062. Has anyone made a before-and-after comparison on this searched other sources for such combs in auxiliary channels? Perhaps forming a BruCo-like search where this UIM / L1 stage control signal is the response instead of DARM?
- Keith has already done a long-term study of the analog-to-digital converters (ADCs), looking for combs: see, eg. pg 44-49 (yeah!) of G1300997. He found no-such combs. Perhaps we should do a similar study on the digital-to-analog convert (DAC) side of things? I could also imagine a similar set up for a set of RFM channels that make the 4km journey along the arms.
Images attached to this comment
andrew.lundgren@LIGO.ORG - 14:49, Tuesday 26 January 2016 (25170)CDS, DetChar, ISC, PEM
In response to Jeff: The SUS-ETMY MASTER signal is just a filtered version of DARM, so if DARM has the comb so do the drive signals. I don't think that tells us where in the loop they originate. But you're right, this could be a digital problem or an electronics one involving something synched to GPS.

Keith T. and Annamaria both suggested that the power supply of the timing fanout might be involved. That of course can be perfectly synched to the GPS second. Annamaria showed me an ADC in the L1 corner station being used as a temporary monitor of one of these power supplies. That signal (attached) jumps downward one second and upward the next, matching what we see in the magnetometers and DARM. Could we check if there's such an effect at the H1 Y-end?
david.shoemaker@LIGO.ORG - 13:59, Tuesday 26 January 2016 (25166)
Note that the small glitches in Andy's post are exactly synchronized to GPS; this makes coupling to many power supply glitches (HWS, or trickle chargers for magnetometers, etc.) an unlikely source.
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