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Reports until 09:14, Friday 25 August 2017
H1 SEI
hugh.radkins@LIGO.ORG - posted 09:14, Friday 25 August 2017 - last comment - 11:47, Friday 25 August 2017(38367)
STS2 Wind/Floor Tilting Measurement now at Roam9

Thursday afternoon we had a brief but strong wind event--See first plot: 2 day's minute trends.  I had moved the roaming STS2 a week or more ago and now resides at position Roam9.  At the corner station the wind average touched on 20mph for maybe 90 minutes with a stable direction of about 170o or ~from EndX toward the corner.  No non-wind seismic evident.

The second attachment shows the usual STS ASD comparisons between the Roaming HAM5 and the Detector used ITMY STSs, see 38184 for the Roam8 comparison and you can follow back from there.  Great news: for the X dof here at Roam9, the HAM5 STS shows several factors less floor tilting than ITMY starting at 30ishmHz; and, the Y dof is maybe no worse--is that band between 10 & 100mHz too much?

So bottom line Roam9 shows promise!

Times: RefTime is low wind, 25 Aug 0930 utc.  High wind is 0130 25 Aug.  XMLs in /ligo/home/hugh.radkins/STS_Seismometer_Studies

Images attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 11:47, Friday 25 August 2017 (38369)

Latest locations.

Non-image files attached to this comment
LHO General
patrick.thomas@LIGO.ORG - posted 08:23, Friday 25 August 2017 (38366)
Ops Day Shift Transition
TITLE: 08/25 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 51Mpc
OUTGOING OPERATOR: Ed
CURRENT ENVIRONMENT:
    Wind: 3mph Gusts, 2mph 5min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.08 μm/s 
QUICK SUMMARY: No issues to report.
H1 General
edmond.merilh@LIGO.ORG - posted 07:55, Friday 25 August 2017 (38365)
Shift Summary -Owl

TITLE: 08/25 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 50Mpc
INCOMING OPERATOR: Patrick (subbing for Cheryl)
SHIFT SUMMARY:
LOG:

 

H1 General
edmond.merilh@LIGO.ORG - posted 05:02, Friday 25 August 2017 (38364)
GRB Alert

12:01UTC Confirmed wit Livingston. Injections node working properly. 1 hour standown in effect.

H1 General (DetChar)
edmond.merilh@LIGO.ORG - posted 00:45, Friday 25 August 2017 (38361)
Livingston informed us of a GRB alert

07:22 Radar, at LLO aclled to confirm a GRB. Verbal Alarms did not report, however the INJ_TRANS node was activated into the 1hr standown mode. That being said, tweaks were in process after a fresh lock.

H1 General
edmond.merilh@LIGO.ORG - posted 00:43, Friday 25 August 2017 - last comment - 00:57, Friday 25 August 2017(38360)
Shift Transition - Owl

TITLE: 08/25 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 48Mpc
OUTGOING OPERATOR: Jeff
CURRENT ENVIRONMENT:
    Wind: 9mph Gusts, 8mph 5min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.10 μm/s
QUICK SUMMARY:

H1 was locking when I arrived. uSEI ws up to .2um/s and winds had been nearing 40mph earlier. OMC had to be massaged a bit before DC readout as it wouldn't lock. The AS90(purple)trace looked like te victim of some kind of offset as it was off scale until power increase where it came back down to familiar amplitudes. I ran a prelim a2l before setting the bit. the range was below 50Mpc as it was after I spoke to Aidan yesterday morning and he had me manually adjust the TCSX LASER power from preheat level (.500W) to .300W (see his aLog). He told me that we would probably go to .350W to claim a bit more of our already weakish range, so I did and it looks as if it may be a good move as our range has crept back up to 50+Mpc. Tweaking PI mode 28 (as usual).

 

Comments related to this report
edmond.merilh@LIGO.ORG - 00:50, Friday 25 August 2017 (38362)

7:50UTC Verbal Alarms is dodgy. Going to restart

edmond.merilh@LIGO.ORG - 00:57, Friday 25 August 2017 (38363)

While trying to quit to restart the missed messages started to cycle out. After restart I got: Could not connect to GRD_ALS_DIFF_ETMY_ESD_ERROR.

Images attached to this comment
H1 General
jeffrey.bartlett@LIGO.ORG - posted 00:01, Friday 25 August 2017 (38359)
Ops Evening Shift Summary
Ops Shift Log: 08/24/2017, Evening Shift 23:00 – 07:00 (16:00 - 00:00) Time - UTC (PT)
State of H1: Relocking
Intent Bit: Commissioning/Locking
Support: Sheila, Jenne, Jeff K.,
Incoming Operator: Ed
 
Shift Summary: After second lockloss and could not relock ran an initial alignment. Had a bit of trouble with the MITCH_DARK stage, but after several tries and an assist from Sheila, completed the initial alignment. Tried relocking. Cannot make it past CHECK_IR. Wind is up, with gusts well into the upper 30mph range. X and Y microseism is up to 0.3um/s. BRS-X RY_INMON is off the charts right now. The winds are forecast to abate around 22:00PT. Going to hold in DOWN until things quiet down before trying to relock.
Getting high dust counts at End-Y. Caused by high winds and heavy forest fire smoke.
Environmental conditions are improving, so will try relocking.
Relocking no go. Rerun initial alignment. Twice initial alignment stuck at SCR_ALIGN LOCKING_SRY; and twice it tripped the SRM WD.  
On third try made it through initial alignment. Trying to relock.   
Slowly working through the relocking steps. Turn over to Ed; perhaps he will have better results.
 
 Activity Log: Time - UTC (PT)
23:00 (16:00) Take over from Patrick
23:10 (16:10) Lockloss – Unknown
23:16 (16:16) HFD - Going to Mid-X to check the alarm panel
23:35 (16:35) Relocked at NLN – Back into Observing
23:36 (16:36) Damp PI Mode-28
23:37 (16:37) Damp PI Mode-27, 19
00:38 (17:38) Lockloss - Unknown
01:40 (18:40) Complete Initial Alignment
01:41 (18:41) Try relocking
02:35 (19:35) Put IFO into DOWN until environmental conditions improve
07:00 (00:00) Turn over to Ed
H1 General
jeffrey.bartlett@LIGO.ORG - posted 19:54, Thursday 24 August 2017 (38357)
Ops Evening Mid-Shift Transition
  Lost lock at start of shift. Relocked quickly and without trouble. Shortly after lost lock a second time; but was unable to relock. Completed initial alignment, after overcoming some difficulty with MITCH_DARK step. Tried relocking but with no success. Breaks on FIND_IR (DIFF) or at CHECK_IR. Also having difficulty with IR DIFF not really found. Can hand tune and get a good spike, but still cannot really find IR with regularity. 

   Winds are up and gusting into the mid-30mph. X and Y microseism is up to 0.3um/s. BRS-X is damping. High winds are forecast until around 22:00PT. Holding the IFO in DOWN until the environment settles before trying relocking. 

   Getting high dust alarms at End-Y. Given the high winds and heavy wildfire smoke, this is not unexpected.      
H1 PSL
patrick.thomas@LIGO.ORG - posted 16:13, Thursday 24 August 2017 (38354)
Weekly PSL Chiller Reservoir Top-Off
FAMIS 6537

Added 100 mL H2O to crystal chiller.
Neither chiller had a fault light lit and both chillers read that the water level was OK.
Both canister filters appear white and free of debris.
H1 General
jeffrey.bartlett@LIGO.ORG - posted 16:10, Thursday 24 August 2017 (38353)
Ops Evening Shift Transition
Ops Shift Transition: 08/24/2017, Evening Shift 23:00 – 07:00 (16:00 - 00:00) - UTC (PT)
State of H1: Locked at NLN, 28.6w, 51.1Mpc
Intent Bit: Observing
Weather: Clear skies; Winds 10 to 18mph, Temps in the mid-80s
Primary 0.03 – 0.1Hz: X & Y Axis at 0.2um/s, Z Axis at 0.02um/s
Secondary 0.1 – 0.3Hz: At 0.1um/s
Quick Summary: IFO Locked and Observing along with LLO and Virgo. A2L looks good. No problems or issues to report.
Outgoing Operator: Patrick
LHO General
patrick.thomas@LIGO.ORG - posted 16:02, Thursday 24 August 2017 (38352)
Ops Day Shift Summary
TITLE: 08/24 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 51Mpc
INCOMING OPERATOR: Jeff B.
SHIFT SUMMARY: Lost lock for unknown reason. Had to make a significant adjustment to PRM in YAW to lock PRMI. Made it to NLN. While running a2l PI mode 27 ran away and I lost lock again. Succeeded in making it back to NLN and did not attempt to run a2l again. Set to observing. Succeeded in damping PI mode 27 early on.
Have transitioned the INJ_TRANS guardian back to INJECT_SUCCESS.
LOG:

14:47 UTC Closed terminal on nuc3 that was obscuring DARM on control room screenshots.
15:35 UTC Noticed DIAG_MAIN message stating that seismon is not updating. The GPS time does appear stuck at 1187621613.
16:10 UTC Betsy to optics lab.
16:26 UTC Lock loss.
16:32 UTC Gave Aidan remote access.
16:37 UTC Filiberto to mid Y.
17:03 UTC Filiberto back.
17:43 UTC NLN.
17:47 UTC Running a2l.
17:59 UTC Richard to CER.
18:05 UTC Lock loss. PI mode 27 ran away and I could not bring it back.
18:08 UTC Richard back.
18:31 UTC Visitor through gate to see Chandra.
18:32 UTC NLN.
18:35 UTC Observing.
Damped PI mode 27
18:59 UTC Nichole W. to mid X to retrieve Pelican cases.
19:09 UTC Nichole W. through main gate.
19:23 UTC Nichole W. back.
20:19 UTC Set INJ_TRANS to INJECT_SUCCESS.
20:51 UTC Elizabeth to mid Y to pick up parts.
21:14 UTC Elizabeth back.
21:26 UTC Travis and Liz to mechanical room (property control).
21:34 UTC Travis and Liz back.
21:50 UTC Jeff B. moving equipment from LSB to staging building.
22:08 UTC TJ to optics lab.
22:10 UTC Jeff B. done, moving yellow cart to OSB.
22:23 UTC TJ back.
LHO General
patrick.thomas@LIGO.ORG - posted 12:45, Thursday 24 August 2017 (38351)
Ops Mid Shift Report
Back to observing after lock loss at 16:26 UTC.
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 11:55, Thursday 24 August 2017 (38350)
CDS O2 restart report: Wednesday 16th - Wednesday 23rd August 2017

model restarts logged for Wed 23/Aug/2017 - Wed 16/Aug/2017 No restarts reported

H1 TCS (TCS)
aidan.brooks@LIGO.ORG - posted 11:04, Thursday 24 August 2017 - last comment - 14:21, Monday 28 August 2017(38349)
Lens change per lock seemed to increase in June - possible change in absorption?

[Aidan]

I've been investigating the apparent increase in range that occurred this morning when CO2X was turned off. This would seem to indicate that either (a) the CO2 laser is somehow misaligned/or deformed and causing a very poor lens, or (b) the present level of lensing (SELF heating + CO2) is too much. It's worth noting that the requested (and delivered) levels of CO2X laser power haven't changed significantly over the last four or five months.

If we assume (b) and also that the better range in the past is partially due to a better thermal state, then the conclusion is that either the effective CO2 lens or the SELF heating lens has increased.

I've gone back and looked at the HWSX spherical power data (H1:TCS-ITMX_HWS_PROBE_SPHERICAL_POWER) from two months around the period of the earthquake. The relevant value here is the spherical power change per lock (the difference between the upper and lower levels that are obvious in the time series which shows the transient lens from SELF heating and CO2 laser changes). There is an interesting period form 22-June to 7-July where this trends upwards by approximately 25 micro-diopters (or about 50%). This indicates that the apparent lens change per lock seen by the HWS is increasing significantly.

Two factors also play into this. (1) the CO2 laser is being turned on and off during this time (to keep the thermal state warm when the IFO has lost lock). However there is no significant change in the CO2 power level behaviour over the corresponding time range. (2) we know there is already a point absorber on ITMX as well as uniform absorption. The spherical power value is fitted to the low spatial-frequency lens. The presence of a known high spatial frequency point in the wavefront complicates this. For example, it's possible that the HWS alignment may be drifting and the point absorber is contributing more to the total spherical power value. This obviously needs to be investigated further by looking at the stored gradient fields.

However, it does seem that there is a real effect going on as the range got much better (~15% better) when the CO2 laser turned off. 

Images attached to this report
Comments related to this report
aidan.brooks@LIGO.ORG - 14:21, Monday 28 August 2017 (38404)

One thing to note is that if the IFO beam is moving across the surface of the optic (specifically, across the point absorber), then we would see a 50% increase in the amount of absorbed power if the IFO beam moved by dr = 7-10mm. This is based upon the estimate of the point absorber at a radius (r_point) of something like 36-44mm from the center of the optic. (see aLOG 35071 and aLOG 34868)

Specifically: dP_abs = exp(-2*[(r_point - dr)/w0]^2) - exp(-2*[(r_point)/w0]^2)

relative_change = dP_abs/exp(-2*[(r_point)/w0]^2)

H1 PSL (PSL)
travis.sadecki@LIGO.ORG - posted 10:04, Thursday 24 August 2017 (38348)
PSL Weekly

Laser Status:
SysStat is good
Front End Power is 33.8W (should be around 30 W)
HPO Output Power is 154.8W
Front End Watch is GREEN
HPO Watch is GREEN

PMC:
It has been locked 9 days, 0 hr 11 minutes (should be days/weeks)
Reflected power = 16.77Watts
Transmitted power = 57.41Watts
PowerSum = 74.17Watts.

FSS:
It has been locked for 0 days 0 hr and 3 min (should be days/weeks)
TPD[V] = 0.9646V (min 0.9V)

ISS:
The diffracted power is around 3.1% (should be 3-5%)
Last saturation event was 0 days 0 hours and 34 minutes ago (should be days/weeks)

Possible Issues:  None
 

H1 General (TCS)
edmond.merilh@LIGO.ORG - posted 03:47, Thursday 24 August 2017 - last comment - 18:36, Thursday 24 August 2017(38336)
TCSX CO2 LASER woes

09:29UTC "TCSX CO2 LASER output off" verbal happened. After a trip into the LVEA to find the FLOW light tripped on the controller I went into the mezzanine to check the chiller which was NOT tripped. I went back down and reset the controller and everything looked ok except for some SDF diffs in TCS_ITMX_CO2_PWR,TCS_ITMX_CO2, and DIAG_SDF nodes. I called Jason on the phone and he didn't have to much to say about some new Guardian stuff that has been added. I accepted te DIFFS that were showing and took a couple of screenshots.

10:32UTC LASER won't stay locked. It keeps dropping/searching/locking...rinse, lather, repeat. When it locks, the ready bit goes GREEN and I set the Intention bit but it just keeps falling out over and over again.

10:35UTC maybe it will hold this time?

10:46UTC nope

Images attached to this report
Comments related to this report
peter.king@LIGO.ORG - 04:10, Thursday 24 August 2017 (38337)
We should look at the TCSX controller as it would seem that the trip point is set
differently from the the TCSY controller.  It might be that there are two resistor
values that may have to be changed.
edmond.merilh@LIGO.ORG - 06:00, Thursday 24 August 2017 (38338)TCS

Here's what the BNS Range plot and the HIFO_RANGE looks like since the TCS issue began. There's an uptick in BNS range and then a drop into the mid-40Mpc range. DARM is also a mess.

Images attached to this comment
aidan.brooks@LIGO.ORG - 07:25, Thursday 24 August 2017 (38342)

[Aidan (remotely), Ed]

I just got off the phone with Ed. It seems that after the TCS CO2X laser reacquired lock, the requested power went to a much higher level (500mW) than that required during steady-state operations (300mW). Given the long recovery time, I advised Ed to drop the request power manually back down to 300mW and then re-enter observing mode if we got kicked out.

Interestingly, the range went UP when the CO2X delivered power was 0.0W. We might try dropping the requested power for the remaining time in O2.

 

 

Images attached to this comment
alastair.heptonstall@LIGO.ORG - 07:41, Thursday 24 August 2017 (38344)

I agree with Peter - we should look at the laser controller first, and the flow meter second.  We have a spare chassis that can be swapped in very quickly.  At the same time it would be useful to double check the settings on the yellow electronic flow meter that's under the beam tube.  If you pop the top off it there is a screen and the current/voltage output range can be checked so we know its output calibration.

Once a laser trips and is turned back on it needs at least 30mins before we try to lock it. Not giving it this time will cause the guardian script to mess around with its thermal state and it will take longer to lock. We should think about whether we should be losing detector time to wait to be able to lock this laser if it does not improve sensitivity.  Maybe we aren't gaining a lot from that. 

sheila.dwyer@LIGO.ORG - 09:43, Thursday 24 August 2017 (38347)

This improved range was due to a reduction in the broadband jitter coupling, which can be seen looking at coherence between the PSL bullseye pit signal and DARM or the IMC WFS B DC PIT coherence, shown in the attached screenshot. (For IMC WFS B there are some peaks from acoustics on the table which are not changed with the TCS settings.)

It not surprising that the this can be improved.  It doesn't seem worth changing settings at this point in the run.  This noise is subtracted by Jenne's weiner filter cleaning of the data; we know that the spot positions also can improve this noise, and after the long vent we will have both a different PSL laser and hopefully less ITMX absorption. 

Images attached to this comment
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 18:36, Thursday 24 August 2017 (38356)
Opened corresponding FRS Ticket 8846.
LHO VE
kyle.ryan@LIGO.ORG - posted 19:22, Tuesday 22 August 2017 - last comment - 10:09, Sunday 27 August 2017(38315)
TMDS training session at X-end
Rai W., Mike Z., Daniel S., Jeff K., Chandra R., Kyle R. 

Today the TMDS Gas Delivery Table was transported to the X-end VEA and set it up for operation.  The actual Surface Discharge Ionizer was mounted on a stand for today's demonstration purposes.  Nominally, it would be mounted to the dedicated TMDS port of BSC9's East Door.  The Vent/Purge air supply was ran and dry air supplied to the TMDS setup.  Prior to exposing the Ionizer to the conditioned air supply, the plumbing connection at the Ionizer was decoupled and connected to a test setup that facilitated the measurement of > 0.3 micron and > 0.5 micron particulate in the conditioned air. The air line was then re-coupled to the Ionizer.  An approximate 50/50 mix of Ethylene Glycol to Alcohol along with "chunks" of dry ice was used as a cold trap to the path.  

Rai W. gave an overview of the theory and a detailed tutorial as to the operation of the setup.  Daniel S. and Jeff K. noted details related to the ion production while Kyle R. and Chandra R. noted detail related to the vacuum related issues.  

The Ionizer setup performed satisfactorily (with caveats) at making comparable amounts of positive and negative ions.  

The plan now is to connect the Ionizer to BSC9 and perform an actual discharge of the ETMx during next Tuesday's maintenance day.  

My notes from today; 

1. Oscillations were noted and attributed to electronics design -> Daniel S. will address.  
2. Rai W. requested that we provide a means of support to take the weight of the Ionizer when mounted to the 1 1/2" valve on the BSC -> Kyle R. will address.  
3. Confirmation of the preferred means to pump to rough vacuum the X-end VE between cycles of discharge gas admission -> Chandra R. will address.  

Non-image files attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 09:53, Wednesday 23 August 2017 (38327)

We will use the QDP80 to pump down the chamber between discharge cycles, with the turbo spun down and, as needed, use purge air to regulate the pump-side pressure to match the chamber pressure as to not break the 10" gate valve rated for 10 Torr differential pressure. Attached is a plot from LLO discharge. They spun up and down the turbo between cycles, but decided later it was not worth the trouble.

Images attached to this comment
jeffrey.kissel@LIGO.ORG - 20:30, Thursday 24 August 2017 (38358)CDS, DetChar, ISC, SUS, SYS, VE
Refer to Figure 1 of T1400713, TMDS design document for elements of setup.

A couple of useful videos of the oscilloscope readouts during the experiment:

Lesson 1: Control and readback of the electrometer from the TMDS inferface chassis, D1500152.
    Rai has set up the readback of the electrometer with the square-wave input shown on the blue trace, and the electrometer readback in yellow. One is looking for an even balance in voltage from the positive and negative ions. The electrometer has a negative voltage bias at the time of recording, so it appears as though we're getting more positive than negative ions, but, rest assured, we're good. 

Lesson 2: Demonstration of ionic discharge against TMDS chamber walls, if HV supply to ion generator is too high.
    The readback of the HV current is shown on the yellow trace. The video starts out with the ion generator discharging, as is evident by the rattiness of the waveform. At the last few seconds of the video, he reduces the VARIAC HV transformer gain, bringing the ion generator back to the desired level.

Lesson 3: Demonstration of electrometer readback once HV voltage is reduced
    Once the HV is tuned with the VARIAC, with the initial max amplitude of the square wave generator, then the square wave amplitude may be reduced to ~ 3 V pkpk (assuming a flow rate of about 30-50 [mL/s ?? not sure about those units]). Once we did this, we saw evidence for a ~3 MHz oscillation on the electrometer readback. Investigating the circuit drawing for the electrometer board (D1500061), Daniel and Mike agreed to replace the readback's output resistors R9 & R10 with ~100 [ohm] resistors. 
This has been done already, and the electrometer has been reinstalled

Lesson 4: Final setup of readback / monitor system, in the "ready to discharge into chamber" configuration.
    Once again, Rai demonstrates the control of the HV VARIAC and the desire to keep the ion generator current readback from any rattiness in its waveform, which is indicative of ionic breakdown discharge against the TMDS chamber walls.

I attach a ton more pictures of the setup as well. Hopefully the filenames are a good enough caption.
Images attached to this comment
kyle.ryan@LIGO.ORG - 10:09, Sunday 27 August 2017 (38386)
Desired gas flow rate 30 - 50 Liters per Minute (LPM)
H1 SUS
jeffrey.kissel@LIGO.ORG - posted 11:37, Tuesday 08 August 2017 - last comment - 18:22, Thursday 24 August 2017(38077)
Single Stage SUSs Checked for Rubbing
J. Kissel

I've checked the last suspensions for any sign of rubbing. Preliminary results look like "Nope." 

The data has been committed to SUS repo here:
/ligo/svncommon/SusSVN/sus/trunk/HAUX/H1/IM1/SAGM1/Data/
2017-08-08_1629_H1SUSIM1_M1_WhiteNoise_L_0p01to50Hz.xml
2017-08-08_1629_H1SUSIM1_M1_WhiteNoise_P_0p01to50Hz.xml
2017-08-08_1629_H1SUSIM1_M1_WhiteNoise_Y_0p01to50Hz.xml

/ligo/svncommon/SusSVN/sus/trunk/HAUX/H1/IM2/SAGM1/Data/
2017-08-08_1714_H1SUSIM2_M1_WhiteNoise_L_0p01to50Hz.xml
2017-08-08_1714_H1SUSIM2_M1_WhiteNoise_P_0p01to50Hz.xml
2017-08-08_1714_H1SUSIM2_M1_WhiteNoise_Y_0p01to50Hz.xml

/ligo/svncommon/SusSVN/sus/trunk/HAUX/H1/IM3/SAGM1/Data/
2017-08-08_1719_H1SUSIM3_M1_WhiteNoise_L_0p01to50Hz.xml
2017-08-08_1719_H1SUSIM3_M1_WhiteNoise_P_0p01to50Hz.xml
2017-08-08_1719_H1SUSIM3_M1_WhiteNoise_Y_0p01to50Hz.xml

/ligo/svncommon/SusSVN/sus/trunk/HAUX/H1/IM4/SAGM1/Data/
2017-08-08_1741_H1SUSIM4_M1_WhiteNoise_L_0p01to50Hz.xml
2017-08-08_1741_H1SUSIM4_M1_WhiteNoise_P_0p01to50Hz.xml
2017-08-08_1741_H1SUSIM4_M1_WhiteNoise_Y_0p01to50Hz.xml

/ligo/svncommon/SusSVN/sus/trunk/HTTS/H1/OM1/SAGM1/Data/
2017-08-08_1544_H1SUSOM1_M1_WhiteNoise_L_0p01to50Hz.xml
2017-08-08_1544_H1SUSOM1_M1_WhiteNoise_P_0p01to50Hz.xml
2017-08-08_1544_H1SUSOM1_M1_WhiteNoise_Y_0p01to50Hz.xml

/ligo/svncommon/SusSVN/sus/trunk/HTTS/H1/OM2/SAGM1/Data/
2017-08-08_1546_H1SUSOM2_M1_WhiteNoise_L_0p01to50Hz.xml
2017-08-08_1546_H1SUSOM2_M1_WhiteNoise_P_0p01to50Hz.xml
2017-08-08_1546_H1SUSOM2_M1_WhiteNoise_Y_0p01to50Hz.xml

/ligo/svncommon/SusSVN/sus/trunk/HTTS/H1/OM3/SAGM1/Data/
2017-08-08_1625_H1SUSOM3_M1_WhiteNoise_L_0p01to50Hz.xml
2017-08-08_1625_H1SUSOM3_M1_WhiteNoise_P_0p01to50Hz.xml
2017-08-08_1625_H1SUSOM3_M1_WhiteNoise_Y_0p01to50Hz.xml

/ligo/svncommon/SusSVN/sus/trunk/HTTS/H1/RM1/SAGM1/Data/
2017-08-08_1516_H1SUSRM1_M1_WhiteNoise_L_0p01to50Hz.xml
2017-08-08_1516_H1SUSRM1_M1_WhiteNoise_P_0p01to50Hz.xml
2017-08-08_1516_H1SUSRM1_M1_WhiteNoise_Y_0p01to50Hz.xml

/ligo/svncommon/SusSVN/sus/trunk/HTTS/H1/RM2/SAGM1/Data/
2017-08-08_1520_H1SUSRM2_M1_WhiteNoise_L_0p01to50Hz.xml
2017-08-08_1520_H1SUSRM2_M1_WhiteNoise_P_0p01to50Hz.xml
2017-08-08_1520_H1SUSRM2_M1_WhiteNoise_Y_0p01to50Hz.xml

Will post results in due time, but my measurement processing / analysis / aLOGging queue is severely backed up.
Comments related to this report
jeffrey.kissel@LIGO.ORG - 14:59, Thursday 17 August 2017 (38253)
J. Kissel

Process the IM1, IM2, and IM3 data from above. Unfortunately, it looks like I didn't actually save an IM4 Yaw transfer function, so I don't have plots for that suspension.

I can confirm that IM1, IM2, and IM3 do not look abnormal from their past measurements other than a scale factor gain. Recall that the IMs had their coil driver range reduced in Nov 2013 (see LHO aLOG 8758), but otherwise I can't explain the electronics gain drift, other than to suspect OSEM LED current decay, as has been seen to a much smaller degree in other larger suspension types.

Will try to get the last DOF of IM4 soon.
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jeffrey.kissel@LIGO.ORG - 17:26, Thursday 17 August 2017 (38260)
All HTTSs are clear of rubbing. 

Attached are
- the individual measurements to show OSEM basis transfer function results,
- each suspensions transfer functions as a function of time
- all suspensions (plus an L1 RM) latest TFs just to show how they're all nicely the same (now)

Strangely, and positively, though RM2 has always shown an extra resonance in YAW (the last measurement was in 2014 after the HAM1 vent work described in LHO aLOG 9211), that extra resonance has now disappeared, and looks like every other HTTS. Weird, but at least a good weird!
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jeffrey.kissel@LIGO.ORG - 18:22, Thursday 24 August 2017 (38355)
J. Kissel

Still playing catch up -- I was finally able to retake IM4 Y. Processed data is attached. Still confused about scale factors, but the SUS is definitely not rubbing, and its frequency dependence looks exactly as it did 3 years ago.
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