Displaying reports 56941-56960 of 85656.Go to page Start 2844 2845 2846 2847 2848 2849 2850 2851 2852 End
Reports until 15:56, Wednesday 07 September 2016
H1 General
cheryl.vorvick@LIGO.ORG - posted 15:56, Wednesday 07 September 2016 (29519)
Ops Day Summary:

State of H1: locking DRMI1F but not able to get through Engage_DRMI_ASC - Sheila working on alignment by hand to get through this stage

Locking Struggles:

Site Activities:

H1 General (OpsInfo, SEI)
edmond.merilh@LIGO.ORG - posted 14:23, Wednesday 07 September 2016 (29518)
Ops Overview MEDM screen edited

Changes made to the Ops overview medm screen include:

Please refer any other suggestions for changes to me regarding this screen.

H1 SEI
hugh.radkins@LIGO.ORG - posted 12:45, Wednesday 07 September 2016 (29516)
Position of BS HEPI post De-Bias Op & OpLev Drift

RobertS suggested a look at the BS OpLevs for position drifting.  I would say there isn't a lot of drifting looking at three days--First Attachment.

But--HEPI moved BS Optic pitch 3 or 4 urads based on Optical Lever

The first attachment is a 3 days showing the BS HEPI work done yesterday 29495 based on the HEPI Catesian location monitors.  You can see that the HEPI Cartesian positionas are exactly the same as before the work but the YAW and moreso the Pitch are shifted immediately following the work on HEPI.  The second attachment zooms into 9 hours and OpLev change is pretty much immediate with the reisolation of the SEI.  I did a quick scan of a few months of this and see most of the time, the OpLev Pitch and Yaw don't change drastically after a de/re-isolation of HEPI.  So I think the amount of change seen here yesterday is not the norm.

On the third attachment we see the actual change with the local Sesnors.  For the four Horizontal sensors you can see that all shift about positive 4 - 500 counts.  These actuators face opposite directions so these shifts essentially cancel and no YAW or Translation should occur.  For the verticals, with different Actuator positions, it is hard to imagine not actually shifting the tilt of the table even with the same resolved cartesian position.  Certainly the platform strain (in the actuator psoitions) as quantified by the Pringles is different.  This is what we have though with AC couple pringle loops.  I recommend we study the isolation sequence and maybe we can achieve better repeatability.

It is hard to imagine how this can affect the Optic Pitch but...

Images attached to this report
H1 PSL
edmond.merilh@LIGO.ORG - posted 09:48, Wednesday 07 September 2016 (29513)
PSL Weekly 10 Day Trends - FAMIS #6112

In general; Varying levels of higher-than-normal humidity levels in the LASER room and the Osc box and the corresponding temp fluctuations in the xtals are all related to the ongoing chiller issues. The resulting tripping/shutdowns are also evident in these trends as well. The ongoing DB3 issue is addressed here.

Images attached to this report
H1 General
vernon.sandberg@LIGO.ORG - posted 09:29, Wednesday 07 September 2016 (29514)
Maintenance Day Work Permit Summary for 2016 September 6
Work Permit Date Description alog
       
       
6139.html 2016-09-06 12:10 Activity: Vent locally mounted RGA turbo pump while isolated from RGA+Vertex volume via (1) closed 1 1/2" metal valve * Repair turbo vent valve O-ring and confirm with leak detector * Remove turbo from RGA hardware and install with (1) 1 1/2" O-ring valve * Pump to rough vacuum the volume between the newly installed O-ring valve and the adjacent 1 1/2" metal valve 29507
6138.html 2016-09-06 11:20 Activity: Load new debugging builds of daqd on the frame writers. Load h1fw0 & h1fw2 with a new build of daqd to help diagnose issues seen with h1fw0. Two frame writers are needed in order to do a comparison of additional output to be produced by daqd.  
6137.html 2016-09-06 10:31 Activity: swap fw0 and fw1 10GigE fibers to see if retransmission error follows the hardware.  
6136.html 2016-09-06 09:46 Activity: Replace the camera that allows views of the VEA with a functioning camer  
6135.html 2016-09-06 09:33 Activity: Restore IM1-4 alignment to O1 values and use IM4 Trans and ISS2 QPD to evaluate the IMC and IM alignment. This work is best done before ISS2 array is recentered. This investigation is part of an evaluation of changes in H1 alignment since O1, including input pointing already alogged, and continuing on to changes in IMC/IM alignment. 29500
6134.html 2016-09-06 08:15 Activity: Removal, repair and reinstall of demod board. 29502
6133.html 2016-09-02 09:39 Activity: Remove DC Bias on BS HEPI Servo Position: DeIsolate HEPI Loops, adjust length of Payload Springs to bring position closer to servo'd position. Reisolate. Duration 2 hours.
Area of Activity: H1 SEI HEPI BS
29495
6132.html 2016-09-01 09:25 Activity: Update h0vaclx and h0vacly to add input and output beam tube annulus ion pumps. Restart DAQ to add channels.  
6131.html 2016-08-31 10:21 Activity: add all epics diagnostics channels for the frame writers to the DAQ for trending purposes.  
H1 General
cheryl.vorvick@LIGO.ORG - posted 08:43, Wednesday 07 September 2016 (29512)
Morning Meeting:

System Updates:

 

- SEI

- SUS, working, no update

- CDS/Electronics

- TCS, working, no update
- VAC, noise sources turned off yesterday
 
Commissioning last night went well, continues today.
LHO FMCS
bubba.gateley@LIGO.ORG - posted 07:09, Wednesday 07 September 2016 (29511)
Chilled water setpoint change at the corner station
I increased the chilled water set point at the corner station chiller to 40 degrees F. Up from 36 degrees F. 
H1 ISC
stefan.ballmer@LIGO.ORG - posted 00:41, Wednesday 07 September 2016 - last comment - 19:59, Wednesday 07 September 2016(29509)
Stability work at 50W

Jenne, Stefan

- lowered CFSOF gain from 0.5 to 0.2. This avoids an instability due to gain peaking and possible radiation pressure feed-back at 2.15Hz.

- With that the coil driver switching was no longer an issue. In fact we reduced the ramp times all to 1 sec - it worked fine.

- We still keep dropping the sideband recycling gain and lost lock after  ~36min. THus we decided to do some loop gain tracking.

- We added a laser frequency modulation line at 900Hz, and demodulated it in REFL_9_I (blue - LSC-LOCKINM_1_DEMOD_4_I) and REFL_45_I (brown - LSC-LOCKINM_1_DEMOD_3_I in the attached plot).

- Additionally we suspected that the BS ASC controls are going wacko. So we but pitch and yaw dither lines on the BS, and demodulated everything.

- Attached are two plots (with different time axis) of the result during a 50W lock.

Remarks:

- The REFL45 gain INCREASED by more than a factor of 2! This is consistent with less 45 sideband going into the cavity, and thus more being available as reference in REFL.

- The AS36_A gains seem to reflect that - i.e. a slight gain drop due to less 45MHz being available.

- The AS36_B gains initally agree, but then go completely nuts:  AS36_B_Q_P (orange) keeps dropping, while AS36_B_Q_Y (red) turns around.

- Additionally, the AS36_B_Q_Y- Q dither demoduilation is growing significantly (not plotted). Not sure what to make of that. (the Q dither demodulation of all other signals remaind reasonable.)

Conclusion:

- We suspect that our lock losses might be due to the BS ASC signal becoming unsable. In addition, we have to carefully look at loop gains of all WFS that use 45MHz in REFL - their gain is expected to shoot way up.

- At lest for REFL ASC, it might be time to use the dynamic power normalization.

 

LEGEND for plot:

H1:LSC-LOCKIN_1_DEMOD_4_I_OUTPUT         LSC: laser frequency to REFL_9_I  (blue)
H1:LSC-POPAIR_B_RF18_I_NORM_MON          9MHz 2-f in PRC                           (green)
H1:LSC-LOCKIN_1_DEMOD_3_I_OUTPUT         LSC: laser frequency to REFL_45_I (brown)
H1:ASC-ADS_PIT4_DEMOD_I_OUTPUT           ASC: BS pit to AS36_A_Q_P           (cyan)
H1:ASC-ADS_PIT5_DEMOD_I_OUTPUT           ASC: BS pit to AS36_B_Q_P           (orange)
H1:ASC-ADS_YAW4_DEMOD_I_OUTPUT           ASC: BS yaw to AS36_A_Q_Y      (purple)
H1:ASC-ADS_YAW5_DEMOD_I_OUTPUT           ASC: BS yaw to AS36_B_Q_Y      (red)

Images attached to this report
Comments related to this report
peter.fritschel@LIGO.ORG - 07:16, Wednesday 07 September 2016 (29510)

Beamsplitter motion as seen by its Optical Lever:

Over the course of the 40 minutes shown in Stefan's plots, the BS optical lever shows that it is moving:

  • Pitch: moves by 0.1 urad over 12 minutes at the beginning, then more or less stays there
  • Yaw: moves by 0.2 urad over the 40 min; looks like it is still drifting at roughly this rate at the end of the lock
Images attached to this comment
stefan.ballmer@LIGO.ORG - 19:59, Wednesday 07 September 2016 (29522)

I spent sume time lookin g at the signals form the AS36 diodes during this lock.

The 1st quation was whether all the RF from the length signals ios indeed in the I phase.

- Plot 1 shows the I sum and Q sum of AS_A_36. Most of the signal is in the I phase, but a phase change of -12deg (from -140 to -152 deg) would further improve the situation.

- Plot 2 shows the same thing for AS_B_36. It's overall phasing is as good as we can expect.

- Plot 3 shows the signal of all individual quadrants, I and Q (including the extra -12 deg in AS_A_36). Note that most signal is in quadrant 3. This might be an indication that we also have a centering issue, or it might be the result of an unhealthy about of higher order modes at the AS port.

- Plot 4 shows the Q signals that go into the BS error signals - they are a weighted sum of A and B - currently 0.666*A+1.0*B. For A the trace is plotted with (blue) and without (green) the extra -12deg of phase.
  Note that the PIT signals (and to a lesser extend also the YAW signals) show a divergence to opposite direction, because their weighed sum is servod to zero. This is expected if one channel starts seeing more garbage than signal.

- Plot 5: This plot shows the BS dither line strength for PIT and YAW, for both A and B diode. Note that A is well behaved until the end, while B's gain increases significantly for yaw, and drops to almost zero for pit.

Based on plot 4 and 5 I suspect we would be better off using only AS_36_A at 50Watt. THe challenge will be it's offset - we will try this later tonight.

Images attached to this comment
LHO General
patrick.thomas@LIGO.ORG - posted 00:05, Wednesday 07 September 2016 (29508)
Ops Evening Summary
Jenne, Stefan, Terra, Jamie and Sheila commissioning.

Peter and Jason finished work on the PSL at the beginning of the shift. Stefan started and I finished an initial alignment. Jenne and I had to change the fiber polarization in the MSR. We encountered issues with engaging the DRMI ASC loops again. This was mostly dealt with by stopping at LOCK_DRMI_1F and moving the optics to minimize the ASC error signals before engaging the control loops. The striptools for these are in /opt/rtcds/userapps/release/isc/h1/scripts. They are PITCH_ASC_ERROR_SIGNALS.stp and YAW_ASC_ERROR_SIGNALS.stp. There was a 300nm dust alarm in the PSL102 room. I trended the channel back and it appears to have happened a number of times before. I changed the ISI configuration from 'very windy' to 'windy'.

23:12 UTC Jenne to LVEA to measure noise of seismometer
23:18 UTC Jenne back

Jason and Peter done in PSL, Stefan starting initial alignment

23:52 UTC Jenne and I changed polarization in MSR
00:11 UTC Initial alignment done
01:55 UTC PSL102 300NM dust alarm warning
03:16 UTC Changed ISI configuration from 'very windy' to 'windy'
LHO VE
kyle.ryan@LIGO.ORG - posted 17:32, Tuesday 06 September 2016 - last comment - 14:28, Wednesday 07 September 2016(29507)
Vertex RGA in nominal state - IFO impacting noise sources are now off
Friday I had improved by a factor of 2x or so the persistent air leak in the Vertex RGA by torquing the suspect "factory" flange between the analyzer and it's protective nipple.  This leak turned out to be only a small fraction of the total leak rate observed, i.e. there was more than one leak.  Today I again removed all of the heat tapes and aluminum foil to gain access to the CF joints for additional helium leak testing.  Note that all joints had been tested individually at various times prior to this most recent bake exercise as well as collectively via bagging the complete RGA assembly.  Again, the joints tested good today so I decided to do a "fire hose" test and upped the flow of helium to "audible" values.  John W. was physically present this time and his well documented aura was in full effect so we immediately found that the turbo vent valve was the culprit.  This is consistent with all of the previous observations as the Turbo vent valve had not been sprayed in earlier hunts, the reasoning being that it is an O-ring seal with a very small cross section and permeates to the point of being a nuisance when leak hunting (normally!).  Also, the rate at which is was leaking was just smaller than that which would show up on the foreline pressure gauge but just big enough for the portion that reverse flowed through the turbo stages could account for the value of observed leaking at the turbo inlet - Arrgghh!!!!! 

I took scans and decoupled the turbo and pump carts and shut all noise sources off.  

I'll make an entry tomorrow with the scan data.
Comments related to this report
kyle.ryan@LIGO.ORG - 14:28, Wednesday 07 September 2016 (29517)
Attached are the scans taken on 09-06-2016
Non-image files attached to this comment
LHO VE
kyle.ryan@LIGO.ORG - posted 17:05, Tuesday 06 September 2016 - last comment - 10:59, Wednesday 07 September 2016(29506)
Manual over-fill of CP3 not required
No overfill required today as we had an LN2 delivery and I had to reduce the LLCV %open from 21% to 18%.  

~1635 - 1700 hrs. local -> I visually confirmed that CP3's exhaust line was frosted - dewar vapor pressure at 20 psi.  

Next overfill to be Friday, Sept. 9th.
Comments related to this report
kyle.ryan@LIGO.ORG - 10:59, Wednesday 07 September 2016 (29515)
So I screwed up (I used to keep a tally of these occurrences but it has become too impractical)!  It wasn't until after the LN2 delivery was underway (done?) that I realized that I hadn't proactively reduced CP3's LLCV %open value so as to avoid over pressuring CP3's LN2 reservoir.  As I have now demonstrated, we are vulnerable to this on delivery days.  Recall that while CP3 is in "Manual" fill mode, we have defeated any ability for CDS to close the Fill Valve (aka LLCV) as a response to overpressure.  As such, we are completely reliant on Vacuum Personnel awareness.  

Gerardo suggested that I notify he and Chandra when LN2 deliveries get placed to lessen the likelihood of this happening again.  John suggested that we leave open the exhaust check-valve bypass-valve and not rely on "Vacuum Personnel awareness" - that is why he gets paid the big bucks!  I will open the bypass valve the next time I am at the Y-mid - Brilliant!  

Non-image files attached to this comment
H1 General (IOO, ISC, PSL, SEI, VE)
cheryl.vorvick@LIGO.ORG - posted 15:55, Tuesday 06 September 2016 (29505)
Ops Day Summary: Maintenance - PSL plumbing

State of H1:  PSL crew continue to work on plumbing - crystal chiller was filled in preparation for turning it back on

Additional Activities:

Sitewide:

State of systems that might effect H1 locking:

H1 SEI
jim.warner@LIGO.ORG - posted 15:11, Tuesday 06 September 2016 (29504)
Guardian node for Compact BRS created

TJ, Jim

This afternoon TJ walked me through making a guardian node for the Compact BRS in the Biergarten. This BRS is only destined to be used for Newtonian Noise studies, but has been drifting a bit since install. Up to today, the monitoring system has been Krishna watching from off-site, then sending me an email when the PZTs go out of range, if I don't catch it before then. Now there is a guardian that monitors the PZT readouts and recenters them automatically.

This is not a critical node, so if CDS needs to kill the node for any reason, we can do that, but it's nice having BRS babysitting automated. I've added this node to the Guardian Overview, in the top right above the TCS nodes, but that screen is getting pretty busy. I've also added/commit the guardian code to the userapps/isi/h1/guardian repository.

The node has 3 states:

1. INIT which returns to RUN, 

2. RUN which monitors the outputs to the PZTs and

3. RECENTER, which ramps off the damping, then the outputs of the PZTs, clears the histories of the PZT CTRL filters, ramps the CTRL gains on, then restores the damping and returns to RUN.

Images attached to this report
H1 PEM
robert.schofield@LIGO.ORG - posted 14:40, Tuesday 06 September 2016 (29503)
ID of a couple of peaks in DARM

During today’s maintenance, I looked into a couple of peaks in DARM that have been present in recent weeks, even though we have been at low sensitivity. The peak at 56.8 is from the EX HWS. We should power it on a separate 18V supply like EY, or remember to shut it off for the O2 run. The peak at 451.5 was associated with Kyle's RGA bake-out pumping by HAM4, but I think he completed that today, so the peak should go away.

H1 ISC (ISC)
richard.mccarthy@LIGO.ORG - posted 13:52, Tuesday 06 September 2016 (29502)
Common Mode Servo FET Demod Board replaced.
Re-Installed Common Mode Servo Board S1102626 for use with the mode cleaner.  This is the unit that had problems when the filter board was installed 23 Aug.  This unit has the 200kHz filter installed.  
Took advantage of the PSL work to fix the first channel on the DeMod board.  This has been re-installed and the mode clean is again going through the first channel.
H1 General
cheryl.vorvick@LIGO.ORG - posted 13:50, Tuesday 06 September 2016 (29501)
Ops Mid-day Update:

State of H1: PSL crew working on plumbing and flow sensors - taking lunch and will return to the PSL this afternoon

Maintenance Activities: 

Current Activitiy:

H1 IOO (IOO, PSL, SUS)
cheryl.vorvick@LIGO.ORG - posted 13:26, Tuesday 06 September 2016 (29500)
H1 alignment changes in IO optics and in alignment sensors: O1 and post O1

I've collected the alignment changes in the IMC, the IMs (IM1-4), PRM, PR2, RM1, and RM2.

I've also included the senors that see the beams related to these optics, WFSA, WFSB, IM4 Trans, and ISS2 QPD.

WFSA and WFSB are plagued by a mirror in HAM2 that we believe is loose, because the signals ont he WFS jump when there's no indication of IMC mirrors jumping.  Because of this feature in the WFS signals, I subtracted out the jumps from the segments of drift, and combined the drift segments to get a total drift over O1.

I've highlighted two sets of numbers:

I included RM1 and RM2 since they follow the change of the beam.

Most changed optics:

Most changed sensor /  dof:
  • ISS2 yaw at +1.2 normalized qpd units

IMC WFS reflect the O1 input beam change in yaw of +33urad suggested in my alog 29463:

  change in O1
wfsa p 0.055
wfsa y 0.254
wfsb p 0.210
wfsb y 0.359
Non-image files attached to this report
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