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Reports until 19:57, Friday 13 November 2015
LHO General
corey.gray@LIGO.ORG - posted 19:57, Friday 13 November 2015 (23382)
Mid Shift Summary

useism is still hight 0.5-1.0 um/s & winds are still averaging over 20mph.

TCSX laser tripped this evening as well.  Nutsinee has been talking with Alastair & Mike about this.  I am going to go out on the floor with her as her "buddy" as she inspects and does work on table.  With this laser off, it takes an hour or two for the TCS to heat up ITMX once we get it back... so we'll be down for a while due to this (but we were already down due to obvious environmental issues.

H1 PSL (PSL)
corey.gray@LIGO.ORG - posted 17:31, Friday 13 November 2015 (23381)
PSL Crystal Chiller Topped Off

While checking doors and turning off lights, I went ahead and topped off the Chiller.  I put in 170mL (NOTE:  Jeff topped it off yesterday to 250mL).

LHO General
corey.gray@LIGO.ORG - posted 17:08, Friday 13 November 2015 (23379)
Transition To EVE Shift Update

TITLE:  11/13 OWL Shift:  00:00-08:00UTC (16:00-00:00PDT), all times posted in UTC     

STATE of H1:  H1 is DOWN due to elevated winds & useism since last night's OWL shift.

Outgoing Operator:  TJ

Support:  

Quick Summary

Gusts up to 50+mph.  useism hovering around 0.7 um/s (must be atleast 0.5 to even think about locking...and this isn't even factoring wind.); useism has been at this value or higher for the last 22hrs!

While we are down, Nutsinee is doing Hartman Wavefront Sensor alignment out on the floor (TJ mentioned Landry approved this earlier).  I see that HAM2, HAM5, & HAM6 ISIs are in the DAMPED state.  Will transition back to ISOLATED when Nutsinee work complete.

LHO General
thomas.shaffer@LIGO.ORG - posted 16:18, Friday 13 November 2015 (23378)
Ops Day Shift Summary
LHO General
thomas.shaffer@LIGO.ORG - posted 12:08, Friday 13 November 2015 - last comment - 12:58, Friday 13 November 2015(23375)
Ops Day Mid Shift Report

I managed to get an initial alignment done when the winds were around 30mph, though it probably isn't a very good alignment because I could not let the WFS wait to converge too long or it would get knocked out of lock. After the IA, the winds have picked up to gusts of 50mph according to our Striptool. Keeping ALS locked is proving impossible.

The good news: useism may be trending down slightly. Maybe it's just an illusion from DMT, but I'd rather be optimistic.

Comments related to this report
thomas.shaffer@LIGO.ORG - 12:58, Friday 13 November 2015 (23377)

Now we are getting gusts into the 60's. I even saw one 70mph gust.

H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 11:34, Friday 13 November 2015 (23374)
CDS model and DAQ restart report, Wednesday - Thursday 11th-12th November 2015

model restarts logged for Thu 12/Nov/2015 No restarts reported

model restarts logged for Wed 11/Nov/2015 No restarts reported

LHO General
thomas.shaffer@LIGO.ORG - posted 09:46, Friday 13 November 2015 - last comment - 10:09, Friday 13 November 2015(23372)
Environment Update

Wanted to post some screenshots to show what we have going on.

1st attachment - Wind Striptool

2nd - NOAA Wave height

3rd - Seismic DMT in control room

Images attached to this report
Comments related to this report
john.worden@LIGO.ORG - 10:09, Friday 13 November 2015 (23373)

Thanks for posting those - I was looking at wave heights earlier this morning and noticed the >10M waves off of British Columbia. 

LHO General
thomas.shaffer@LIGO.ORG - posted 08:16, Friday 13 November 2015 (23370)
Ops Day Transition
H1 PEM (DetChar)
dale.ingram@LIGO.ORG - posted 07:57, Friday 13 November 2015 (23369)
Outreach activity report
A large group of middle school students participated in a field trip at LHO on the morning of 11/12.  Arrival time at LSB = 9:00 AM.  Departure time = 11:30 AM.  Group size = ~100 middle school students; ~10 adults.  Vehicles at the LSB = ~3 school buses.  The group was in the control room near 11:15 AM.  
H1 General
cheryl.vorvick@LIGO.ORG - posted 07:09, Friday 13 November 2015 (23368)
Ops Owl Summary:

Title: Owl Shift  08:00-16:00UTC (00:00-08:00PT)

State of H1:  can lock arms in green, cannot go any further

Shift Summary: H1 has been unlocked all night due to high winds and useism.

Currently: No hope of locking even the X arm in IR (I tried, it's not yet possible because of the ground motion)

- useism is around 0.7

- winds are 0-30mph

- guardian state left on Locking Arms Green

With no hope of locking, Richard gave me to ok to head out a bit early.

Patrick is watching the Control Room/phones.

H1 SEI (Lockloss, SEI)
cheryl.vorvick@LIGO.ORG - posted 05:38, Friday 13 November 2015 (23367)
lock loss and ETMY ISI

Three plots attached

Plot 1:  ETMY ISI right before lock loss.  Clear to see motion increasing, and Z positoin rings ups about 45 seconds before lockloss.

Plot 2: ETMY ISI after lock loss.  The ringing in the CPS_X sensor

- at 7:14UTC ISO RX output sees something and the signal grows to 4x it's previous size - red oval

- at 8:10UTC CPS X Location Mon rings up, Jeff and I disable FM8 Boost3, signal quiets around 8:55UTC

- later, with no locking, I disable and enable again to measure a power spectrum (X and Y)

Plot 3: power spectrum comparing ISO X in

--- 2:49UTC (ref6 ,7) - baseline

--- 7:50UTC (ref8, 9) - ISO RX has run up a bit, but ISO X isn't yet

--- 8:45UTC (ref10, 11) - Boost3 turned off on ISO X

--- 10:27UTC (ref22, 23) - as a test I turned off ISO Y Boost3, and yes, it's noticable (bottom plot)

--- 12:22UTC (ref24, 25) - current state, Boost3 filters have been back on since around 11UTC, winds are between 15mph and 40mph, useism is around 0.8 (slightly better than 1.5 hours ago)

Images attached to this report
H1 General
cheryl.vorvick@LIGO.ORG - posted 04:29, Friday 13 November 2015 (23366)
Ops Owl Mid-Shift Update 12:20UTC

Title: Owl Shift 08:00UTC-16:00UTC (midnight to 08:00AM PT)

State of H1: unlocked for 6+ hours due to useism and wind.

Details:

- max wind speed this shift 60mph

- windspeed sitewide about 2 hours ago across all wind stations was between 18mph and 45mph

Currently:

--- useism is around 0.9 and apears to be rising in the last hour

--- wind is between 5mph and 40mph across the site

--- winds at EY have just spiked to 45mph as I wrote this

H1 General
jeffrey.bartlett@LIGO.ORG - posted 00:12, Friday 13 November 2015 (23365)
Ops Evening Shift Summary
Activity Log: All Times in UTC (PT)

00:00 (16:00) Take over from TJ
01:50 (17:50) Jeff – Add 250ml water to TCS-Y chiller. TCS-X OK
06:03 (22:03) Lockloss – Environmental, high winds and microseism.
07:15 (23:15) Put IFO into DOWN to wait for conditions to improve
08:00 (00:00) Turn over to Cheryl


End of Shift Summary:

Title: 11/12/2015, Evening Shift 00:00 – 08:00 (16:00 – 00:00) All times in UTC (PT)

Support: Jim W., Nutsinee,
 
Incoming Operator: Cheryl

Shift Summary: Lockloss at 06:03 (22:02) – Probably due to high winds (in the high 20s to mid 30s with gusts over 40mph) and increasing microseism (centered at 0.8um/s with high at plus 1.0um/s). Attempting to relock. 

The wind has dropped a bit, but microseism is increasing. Switched the ETM-X Y and ETM-Y X dof from Quite90 to 45mHz to see if this will help with locking. ETM ISI CPSs are not rung up.  

Relocking seldom making it past LOCKING_ALS and ETM-X ISI CPS starting to ring up. Put the IFO into a DOWN state and reset the ETM X & Y blends back to original settings. ETM-X ISI CPS has settled back down to a normal state. When wind and microseism calm down will work on relocking.  


H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 23:52, Thursday 12 November 2015 (23364)
Added BP filters to the violin RMS monitor

I added BP filters to:

H1:SUS-ITMX_L2_DAMP_MODE6_BL

H1:SUS-ITMX_L2_DAMP_MODE7_BL

H1:SUS-ITMX_L2_DAMP_MODE8_BL

H1:SUS-ITMX_L2_DAMP_MODE9_BL

H1:SUS-ITMY_L2_DAMP_MODE6_BL

H1:SUS-ITMY_L2_DAMP_MODE7_BL

H1:SUS-ITMY_L2_DAMP_MODE8_BL

H1:SUS-ITMY_L2_DAMP_MODE9_BL

H1:SUS-ETMY_L2_DAMP_MODE5_BL (broad BP)

The filters have been switched on and will be used in monitoring the violin mode second harmonics. I accepted all the changes in OAF SDF.

The space in ETMX violin RMS monitor has run out. If some of the filters are yours and you aren't currently using it please let me know if you could spare one so I can at least make a broad band filter for the ETMX second harmonics.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 23:03, Thursday 12 November 2015 - last comment - 23:27, Thursday 12 November 2015(23362)
Lockloss - Environmental
   Lockloss at 06:03 (22:02) – Probably due to high winds (in the high 20s to mid 30s with gusts over 40mph) and increasing microseism (centered at 0.8um/s with high at plus 1.0um/s). Attempting to relock. 

   The wind has dropped a bit, but microseism is increasing. Switched the ETM-X Y and ETM-Y X dof from Quite90 to 45mHz to see if this will help with locking. ETM ISI CPSs are not rung up.   

Comments related to this report
jeffrey.bartlett@LIGO.ORG - 23:27, Thursday 12 November 2015 (23363)
   The wind has come back up and microseism has risen to be centered at 1.0um/s. Could rarely move past LOCKING_ALS and never past DRMI_1F. The ETM-X ST1 CPS had also started to ring up. 

   Put the IFO into DOWN to wait for conditions to improve. I returned the ETM-X and ETM-Y blends back to Jim's Odd Blends, and the ETM-X ST1 CPS quickly returned to a quite state. Will leave these set as they are.   
Images attached to this comment
H1 ISC
evan.hall@LIGO.ORG - posted 13:14, Thursday 12 November 2015 - last comment - 08:56, Friday 13 November 2015(23350)
Zoomed-in noise budget from 2015-10-24

GWINC quantum noise curve is replaced with dynamically-generated shot noise curve. Radiation pressure will be included later.

The null stream spectrum shows 8×10−8 mA/rtHz shot noise, which seems to imply 17 mA of dc photocurrent on the sum, rather than the expected 20 mA.

Non-image files attached to this report
Comments related to this report
evan.hall@LIGO.ORG - 08:56, Friday 13 November 2015 (23371)

Matt, Evan

The attachment shows two simple power-law curves (1/f2 and 1/f2.5) superimposed by eye on the residual. At first glance it is not clear which fits better.

In the case of 1/f2, we are looking for something that makes a white force noise on the bottom stage of a suspension (e.g., white electronics noise).

In the case of 1/f2.5, we are potentially looking at something less mundane; e.g., a force noise that goes like 1/f0.5, or potentially elevated structural loss on some suspension.

Non-image files attached to this comment
H1 INJ (INJ)
keith.riles@LIGO.ORG - posted 21:28, Wednesday 11 November 2015 - last comment - 13:11, Friday 13 November 2015(23334)
A look at the CW injection swept sine measurements
I took a quick look at the swept sine measurements Chris made earlier today, in order
to derive a transfer function from H1:CAL-INJ_CW_OUT to H1:GDS-CALIB_STRAIN,
using the same matlab script written recently to analyze L1 measurements>.

Attached are spectrograms of H1:CAL-INJ_CW_OUT and H1:GDS-CALIB_STRAIN for
the period of the measurements, along with the derived transfer function
(see LLO alog entry above for explanation of graphs). Although there is an
odd bump in magnitude response at 610 Hz (due to compensating for a notch 
at a BS 2nd violin harmonic?), things are otherwise smooth between 200 and 1400 Hz,
albeit with phase wrapping at a bit more than 1000 Hz. This measurement seems
at odds with Matt Pitkin's CW hardware injections recoveries (summary plot attached), as is
the case for the recent L1 measurements. 

On the one hand, one could wonder if perhaps the swept sine just isn't sampling the frequency range
finely enough to catch everything that affects the particular frequencies where CW injections
are made, especially given the complexity of the inverse actuation filter Jeff posted here. 

On the other hand, the swept sine points were chosen to coincide almost exactly with
CW injection frequencies (575 and 849 Hz) for which discrepancies between injection 
recovery and the transfer function measurements seem to occur. 

Matt has double-checked and triple-checked the phase definitions he uses in 
injection recovery. So the discrepancies in phase for pulsar 1 and 2 phase remain
mysteries (for both H1 and L1). 

As discussed elsewhere, these lingering discrepancies suggest (to me, anyway) that we 
should simplify CW injections either by using PCAL with its considerably simpler IAF
or by dispensing entirely with an IAF in the current ESD injection mode (i.e., rescale
each CW injection amplitude by the point value of the inverse of the measured
actuation function).

Figure 1 - Spectrogram of H1:CAL-INJ_CW_OUT
Figure 2 - Spectrogram of  H1:GDS-CALIB_STRAIN
Figure 3 - Derived transfer function from H1:CAL-INJ_CW_OUT tp H1:GDS-CALIB_STRAIN
Figure 4 - Summary of CW hardware injection recoveries
Images attached to this report
Comments related to this report
keith.riles@LIGO.ORG - 13:11, Friday 13 November 2015 (23376)INJ
It occurred to me belatedly that looking at the intermediate injection
channel H1:CAL-INJ_HARDWARE_OUT might yield some insight into
the above transfer structure in the 500-1000 Hz range, where 
it's hard to reconcile the measurements with CW hardware injections. 

Figure 1 shows the spectrogram during the sweep sine for the channel.

Figure 2 shows the derived transfer function from CW_OUT to HARDWARE_OUT,
which should follow the shape of the inverse actuation filter.

Figure 3 shows the transfer function from HARDWARE_OUT to CALIB_STRAIN.

More detailed information on all three transfer function measurements
can be found on these web pages:

H1:CAL-INJ_CW_OUT --> H1:CAL-INJ_HARDWARE_OUT

H1:CAL-INJ_HARDWARE_OUT --> H1:GDS-CALIB_STRAIN

H1:CAL-INJ_CW_OUT --> H!:GDS-CALIB_STRAIN

Bottom line: there is non-trivial structure in the 500-1000 Hz band
that the swept sine may not be capturing adequately to allow reliable
comparison with injection recoveries.

Bottom bottom line: it's time to try moving CW injections to PCAL with
its simpler inverse actuation filter, as tentatively decided at yesterday's 
injections team telecon.
Images attached to this comment
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