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Reports until 11:18, Tuesday 05 July 2016
H1 SEI (GRD)
hugh.radkins@LIGO.ORG - posted 11:18, Tuesday 05 July 2016 - last comment - 13:32, Tuesday 05 July 2016(28151)
LHO HEPI Guardians Restarted w/corrected code

WP 5984--Addressing a couple month old bug, see SEI log 989 for details.  Summary: We had added a condition to turn off Damping if a platform trips but this code is common for HEPI and the ISI and the HEPI does not have a damping state so there was an error.  This was reverted and Friday Arnaud added a conditional to the code that excluded the HEPI from this action; it was tested at LLO.  I've updated the python code and restarted all the HPI nodes--no impact to the platforms.  See attached for keystrokes.  WP closed.

Images attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 13:32, Tuesday 05 July 2016 (28159)

Duh, of course since the code is common, I actually need to restart all the SEI and ISI guardians as well.  This has been done and the platforms were not affected--thanks guardian programmers!  And thanks to Arnaud for pointing this out to me.  The txt file attached has the restart record.

Non-image files attached to this comment
H1 General (OpsInfo)
cheryl.vorvick@LIGO.ORG - posted 10:02, Tuesday 05 July 2016 - last comment - 11:26, Tuesday 05 July 2016(28149)
Maintenance as of 9:24PT, 16:24UTC - laser is down
microphones Vincent calibration
LVEA Joe batteries
CR Dale tours at noon
all buildings Christina-Karen cleaning
all buildings Fil electorinics inventory
all buildings Joe-Sprague spraying
LVEA Kyle energizing turbo pumps
all buildings Huge checking HEPI pumps
EX and EY JeffK charge measurements
EX and EY Kyle energise RGA filaments
laser Peter-Jason take PSL offline
LVEA DavidM physical measurements
LVEA Nutsinee

swap TCS sled and drain AOM

Comments related to this report
cheryl.vorvick@LIGO.ORG - 11:26, Tuesday 05 July 2016 (28153)

Since last alog:

  • EX-EY - Vincent - microphone-calibration
  • LVEA - Fil - electronicsInv
  • all platforms - Huge - modify HEPI guardians
  • LVEA - Christina/Karen - cleaning
  • Ex-EY - JeffK - EX/EY model restart
  • all buildings - pest control is complete, they checked in as they left

Current:

in LVEA:

  • Nutsinee, TCS
  • Christna, cleaning
  • Fil, inventory
  • David McManus, physical measurements

In end stations:

  • Vincent, microphone calibrations

coming up:

  • DAQ restart
  • small tour to LVEA around 11:30
  • large tour of children at noon
  • restarting laser, H1 recovery
H1 General
cheryl.vorvick@LIGO.ORG - posted 09:18, Tuesday 05 July 2016 (28146)
Morning update: Maintenance is underway - light pipe from LVEA being closed for work on TCS table
H1 PSL
peter.king@LIGO.ORG - posted 09:15, Tuesday 05 July 2016 - last comment - 09:55, Tuesday 05 July 2016(28145)
Front end laser is hobbled
Diodes 3/4 are seemingly kaput.
Comments related to this report
jason.oberling@LIGO.ORG - 09:55, Tuesday 05 July 2016 (28147)

Filed FRS 5822.

H1 PSL (PSL)
peter.king@LIGO.ORG - posted 07:09, Tuesday 05 July 2016 - last comment - 09:11, Tuesday 05 July 2016(28142)
Laser down
Came in to find the laser was off due to the power watchdog being tripped.
Both chillers were still running.

I have turned the laser back on but it hasn't returned to where it normally
returns to.  Looking into what happened.
Comments related to this report
peter.king@LIGO.ORG - 07:12, Tuesday 05 July 2016 (28143)
The laser tripped around 4:15 this morning.
peter.king@LIGO.ORG - 09:11, Tuesday 05 July 2016 (28144)
Looks like the NPRO tripped out.  Maybe due to a minor power surge due to the start of the
week?

    Pre-modecleaner had some problems locking irrespective of the reference level.  Found
that a small tweak to the horizontal alignment brought things back right away.

    Note in passing: with no light the output of the locking photodiode was ~ +29 mV.
Unlocked (ie with light incident on the pre-modecleaner) the output was ~ -230 mV.
Which is sort of low, which might be consistent with a small mis-alignment.  The
locking photodiode is a 1 mm InGaAs photodiode after all.
H1 ISC
marie.kasprzack@LIGO.ORG - posted 15:06, Monday 04 July 2016 (28139)
Beam position on the test masses

The beam position on the test masses is estimated from the a2l gains from the last minimization (method explained in alog 22426)

The gains values before and after the mimization are attached in a2l_gains_1151366417.mat.
The corresponding beam positions are reported in each suspension base in the Fig.1 attached. We can see that the beam is not more off-centered than previously.

However, we can observe that the beam hits the ITM and ETM in differents vertical places now in each cavity, suggesting an increase of the beam tilts in PIT with respect to the optical axes (HARD PIT).
That is what I tried to represent with the projection in Fig. 2, where you can imagine the cavities facing you: the figure axis orientation is the ETMs coordinates orientation.
The YAW tilts are reduced in both cavities. But their directions were opposite before the a2l minimization whereas now both cavity axes have a negative YAW tilt (in the ETM coordinates).

I don't know when the script was run for the last time before that, but it could give an indication that the beam is now more tilted in HARD PIT at 40W, and it enters the cavities from the lower area of the ITMs. 

 

Arm Before a2l After a2l
X

 D pit  = 1.3 mm

D yaw = 9.4 mm

D pit  = 7.8 mm

D yaw = 2.4 mm

Y

D pit  = 2.3 mm

D yaw = 6.5 mm

D pit = 8.0 mm

D yaw = 6.3 mm

Images attached to this report
Non-image files attached to this report
H1 ISC (ISC)
haocun.yu@LIGO.ORG - posted 14:30, Monday 04 July 2016 (28140)
HARD Yaw Loop Low Noise Measurements

Sheila, Jenne, Haocun

We took measurements on the C/DHARD yaw Loops with low bandwidth last Friday.

We firstly turned on the new filter to move compensation peaks for C/DHARD Yaw, then turn off the boost to win more phase. The gain was then lowered to ~half (CHARD_Y: -0.7 ---> -0.3, DHARD_Y: 40 ---> 19), and the new cutoff filters can be turned on.

These steps has been added in the Guardian, and we took measurements with the low noise loop, as attached below.

Both of the UGF are about 3.5Hz at 40 W now, which were ~5Hz before.

Images attached to this report
Non-image files attached to this report
H1 General
vernon.sandberg@LIGO.ORG - posted 14:06, Monday 04 July 2016 (28141)
Details on ER9

Engineering Run 9 (ER9) will begin next Wednesday. Here are some important details for operations:

Please see https://wiki.ligo.org/LSC/JRPComm/ER9 for more details.

LHO VE
john.worden@LIGO.ORG - posted 19:04, Sunday 03 July 2016 - last comment - 10:21, Monday 04 July 2016(28137)
CP3 Fill

Filled CP3 at ~ 1:50 UTC , 6:50 PM LOCAL Time Sunday.

Opened valve 1/2 turn and observed liquid after 5 minutes, 15 seconds. Windy on site.

Comments related to this report
chandra.romel@LIGO.ORG - 10:21, Monday 04 July 2016 (28138)
Thanks, John!
H1 ISC
stefan.ballmer@LIGO.ORG - posted 01:36, Saturday 02 July 2016 (28135)
PRC1 offsets do similar things as soft offsets

Tried to use PRC1 input offsets in pitch and yaw ro recover recycling gain, instead of SOFT imput offsets. While the carrier recycling gain responds to PRC1 input offsets similarl to soft offsets, the POP_18 couldnt care less. Thus I suspect none of these offsets is able to tackle the core issue.

 

The next thing to do is to verify that the POP18 signal is actually trustable, and not saturating,  If trustable, it will be the best indication of recycling cavity losses.

 

LHO General
thomas.shaffer@LIGO.ORG - posted 00:00, Saturday 02 July 2016 (28134)
Ops Eve Shift Summary

TITLE: 07/02 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: None
SHIFT SUMMARY: Commissioning continues. We have been sitting at NOMINAL_LOW_NOISE now for  1.5+ hours.
LOG:
fw1 has had at least a couple of restarts

Lost about 9.5hours on all DMT monitors.

23:40 - Gerardo to CP3

00:04 - Gerardo back.

H1 ISC
stefan.ballmer@LIGO.ORG - posted 23:28, Friday 01 July 2016 (28133)
8 Watt Missing Power - looks like it was lost in the power recycling cavity

Spent some time pulling together calibration numbers for AS, REFL and POP diodes, and makeing a total power budget.

Bottom line:

- The missing 20% power (8Watts!) is not coming out of any port, and thus must be absorbed in the interferometer.
- The way to distinguish loss in the recycling cavity and (280 times smaller) loss in the arms is to look at the sideband recycling gains.

Attached is a plot of power at each port, plus the power in the recycling cavity cast into cumulative arm loss (by multiplying with 279 power buildup and 95ppm round trip losses). Note that there is virtually no increase in AS power, and even a decrease in REFL power. the 8 missing Watts are absorbed in the interferometer.

Note that it is very difficult to distinguish arm losses from PRC losses using the carrier. However the two cenarios are very different for the sidebands - for arm losses both sideband hardly see anything. However, for PRC losses, the 9MHz sideband responds quickest, since it starts off with a hight recycling gain. The 2nd attached plot illustrats this. My money is on PRC losses.

The signals I picked for calibration are:

'H1:LSC-REFL_A_LF_OUTPUT':
0.1*0.5^3*(1-800e-6)^3*1000 = 12.47  mWatt REFL (=cts) / Watt from IFO
10% beam spplitter
two 50% beam splitter
three 800ppm loss mirrors
50% beam splitter
1000mW/W

'H1:LSC-POP_A_LF_OUTPUT':
229e-6*0.1*1e6 = 22.9 uWatt POP (=cts) / Watt in PRC
229 ppm of PR2
10% beam splitter
1e6uW/W

'H1:ASC-AS_C_SUM_OUTPUT':
0.965*800e-6*0.48*0.8*997*10^(36/20)*1638.4 = 3.0554e+04 cts / Watt from SRM
0.965 Faraday transmission
800ppm transmission mirror
48% beam splitter
0.8 Quantum Efficiency
997 Ohm transimpedance
36dB whitening gain
1638.4 cts/V ADC
Note: This calibration has the most estimate factors in it. I don't rust it better than ~25%.

'H1:OMC-DCPD_A_OUTPUT' & 'H1:OMC-DCPD_B_OUTPUT':
0.965*(1-800e-6)^2*0.99*0.93*0.5*0.85817*0.9*1000 = 343 mA / Watt carrier 00 mode from SRM
0.965 Faraday transmission
two 800ppm loss mirrors
1% loss mirrir
93% OMC transmission
50% splitter
0.85817 A/Watt ideal
90% Quantum Efficiency (is this right?)
1000mA/A

Images attached to this report
H1 AOS
carl.blair@LIGO.ORG - posted 21:16, Friday 01 July 2016 (28132)
SUS_PI ETMX damping now in LOWNOISE_ESD_ETMY gaurdian state

I broke lock turning the ETMX ESD low pass filters on.  I put them on as I had a feeling that this help PI damping yesterday and the ETMX 15541Hz mode was out of control and would broken lock.
We have now put this change into the LOWNOISE_ESD_ETMY gaurdian state along with the request for the ETMX_PI_DAMPING state from the SUS_PI gaurdian. 

H1 SUS
betsy.weaver@LIGO.ORG - posted 15:59, Thursday 30 June 2016 - last comment - 14:46, Wednesday 04 April 2018(28090)
ETM15 Ears bonded

Between yesterday and today, Gerardo and I successfully bonded the ears to core optic mass ETM15, destined for LLO for post-O1 eventual replacement. 

Ear s/n 195 bonded to S3 flat of mass June 29, 2016

Ear s/n 196 bonded to S4 flat of mass June 30, 2016

The first ear (s/n 195) has a series of bubbles along it's edge, but the surface area of these do not add up to more than the allowed amount as per E1000277, so it passes, see pix attached.

The second ear (s/n 196) has no bubbles and is nice full bond. 

Images attached to this report
Comments related to this report
betsy.weaver@LIGO.ORG - 11:54, Friday 01 July 2016 (28118)

Inspection of the bonds this morning showed no change to the nice S4/Ear surface bond.

The small edge bubbles along the S3 Ear have migrated a bit (not worse, just moved a bit).  Therefore, we decided to rewet the edge with solution to see if it would wick in and close some of the bubbles.  This worked to close one of the larger bubbles, but one bubble continued to morph so we'll reinspect Monday.  Note, none of the sizes of the bubbles got bigger, so the surface area of the bubble total remains the same and below spec.

Images attached to this comment
betsy.weaver@LIGO.ORG - 10:02, Tuesday 05 July 2016 (28148)

Attached is a picture of what the bubbles in the ETM15 S3 Ear bond look like today (recall, it was bonded last Wed so it has now been over 5 days since initial bond).  Apparently over the weekend, the bubbles ran inbound a bit further.  I estimate the surface are of the bubbles to be near 20mm sq., still under the 50mm sq. spec. E1000278, although it isn't pretty.  I measured the longest streaks to be almost 3mm long, with a width of 0.4mm.  There are no bubbles inward from the edge near the center - anything shown in the picture is a camera reflection.

 

The S4 Ear bond looks unchanged from inspection last week, very good bond, very little bubbles.

Images attached to this comment
betsy.weaver@LIGO.ORG - 14:46, Wednesday 04 April 2018 (41291)

Pictures of this ear bond taken by Danny at LLO just before use at LLO, indicate that the bubbles have not changed shape or size since the picture attached July 2016.  Phew, said both Gerardo and I.

Images attached to this comment
H1 SUS (DetChar)
betsy.weaver@LIGO.ORG - posted 15:15, Tuesday 21 June 2016 - last comment - 23:54, Saturday 02 July 2016(27893)
TUESDAY Maintenance SUS OSEM noise hunt - SAT AMP Power Cycles

Richard, Filiberto, Ed, Betsy

Following on from Andy's probing alog 27841 regarding funny looking OSEM spectra, today we looked into a few fishy signals.  Based on spectra he took from before and after the early June power outage which show signal changes, he and Jenne identified the following set of problematic OSEM signals.  I've annotated the list with status as to what we found or fixed today:

 

ITMY L2 LR - Fixed after power cycling the Satallite Amp box (see alog below)

ITMY R0 RT - Signal looks funny before power outage, old problem, TBC...

MC1 M3 UL - Signal looks funny before power outage, old problem, TBC...

PRM M2 UR - Fixed after power cycling the Satallite Amp box (see alog below)

PR2 M1 T2 - TBC...

PR2 M3 UL - Giant nominal YAW Bias which has been on this SUS for over a year - very little signal on OSEM - mechanical fix when vent

PR2 M3 LL - Giant nominal YAW Bias which has been on this SUS for over a year - very little signal on OSEM - mechanical fix when vent

SR2 M1 LF - Funny comb feature, TBC...

SR2 M1 T1 - Funny comb feature, TBC...

SR2 M1 T3 - Funny comb feature, TBC... 

ETMX L2 LL - 50Hz turn up noise, TBC... Turn up is due to LOCK ACQ PUSHING, turn up not present during nominal SUS damping, no LOCK ACQ, see below plot

ETMX L2 LR - 50Hz turn up noise, TBC... Turn up is due to LOCK ACQ PUSHING, turn up not present during nominal SUS damping, no LOCK ACQ, see below plot

ETMX L2 UR - 50Hz turn up noise, TBC... Turn up is due to LOCK ACQ PUSHING, turn up not present during nominal SUS damping, no LOCK ACQ, see below plot

 

ETMY L2 UR - 50Hz turn up noise, TBC... Turn up is due to LOCK ACQ PUSHING, turn up not present during nominal SUS damping, no LOCK ACQ, see below plot

IM3 M1 LL - TBC...

 

We plan to pursue ITMy R0 and SR2 this week at next opportunity.

Comments related to this report
betsy.weaver@LIGO.ORG - 15:43, Tuesday 21 June 2016 (27894)

Before doing the sat amp power cycle, we first tried a coil driver power cycle on a few of our funny OSEM sets.  This did not appear to clear the errant noise in any of the 4 cases.  We then embarked on the sat amp power cycle which cured the 2 shown in the above list.  Tomorrow we hope to revisit ITMY R0 RT and SR2 M1 which we have left off troubleshooting today with only coil driver OFF spectra.  (Betsy, tomorrow you should use the attached spectra as a jump off point.) 

TBC...  Note the wildly different looking symptoms both of which were seen by Lundgren in 20675 AUG 2015.

Images attached to this comment
betsy.weaver@LIGO.ORG - 15:45, Tuesday 21 June 2016 (27896)

Attached is the ITMY L2 OSEM signal spectra shown from before and after today's fix.  The PRM M2 OSEM before and after-fix spectra are very similar to this.

Images attached to this comment
betsy.weaver@LIGO.ORG - 09:58, Wednesday 22 June 2016 (27911)

ETMX High freq turn up during LOCK ACQ, not a stand alone OSEM signal feature.

Images attached to this comment
betsy.weaver@LIGO.ORG - 10:03, Wednesday 22 June 2016 (27912)

ITMy R0 RT investigation - this morning Richard and Fil performed another round of tests on the ITMy R0 RT (shared cable and electronics with R0 LF, M0 RT, M0 LF).  After power cycling the SAT box, other SAT box cable reseating, and reseating of the main cable to the chamber, the noise on this channel still exists.

SR2 M1 bouncy noise on 3 of 4 TOP investigation - Richard and Fil powert cycled the Sat AMp box for this set of 4 OSEMs, but the noise is still there.

TBC...

andrew.lundgren@LIGO.ORG - 23:54, Saturday 02 July 2016 (28136)DetChar, ISC, SUS
As requested by Betsy, I've made another set of spectra of the OSEMs. The green line is July 1 10:18 UTC. The reference time (black) is a time near the Boxing Day event (Dec 26 2015 4:30 UTC). This is because the OSEMINF channels are only stored in the commissioning frames, and those aren't stored for very long. But we did store them around events in O1.

If we need to do these checks often, then we will need to 1) Store the OSEMINF channels in raw frames. 2) Occasionally save commissioning frames for some time in known-good states 3) Write some code to dump spectra to a file occasionally.
Non-image files attached to this comment
Displaying reports 58441-58460 of 85824.Go to page Start 2919 2920 2921 2922 2923 2924 2925 2926 2927 End