IFO broke lock at 16:16 (08:16). Cause at this time is unknown. 

During relocking could not move past DRMI_1F. Consulted with Kiwamu and decided to run an initial alignment. IFO was relocked at NLN at 17:47 (09:47). Ran A2L script. There were SDF notifications for both ETMs and ITMs. Could not find a SUS person, so took screenshots and accepted all. Set intent bit to Observing at 18:25.    

Spoke with Hugh about the BSC ST2 Guardian notifications.  

Pursuant to a discussion on the PSL call this morning, I'm posting trends of the humidity and temperature in the Laser Room, Laser Diode Room, and Chiller Room over the past 365 days.

The humidity sensors are coupled with the temperature sensors.  We have more temperature sensors, but we decided not to record their coupled humidity sensor signals.

Attached is a plot of the NPRO output power and the output power of the two pump diodes for the past 4 years.
One can see that the diode current was increased around 8/16/2013 and 6/5/2014.  The first increase in pump
current was about 200 mA; the second about 50 mA.

This NPRO is very close to its "maximum" diode current.

O1 days 46,47

model restarts logged for Mon 02/Nov/2015 No restarts reported

model restarts logged for Tue 03/Nov/2015
2015_11_03 09:30 h1hpiitmy
2015_11_03 09:30 h1iopseib1
2015_11_03 09:30 h1isiitmy
2015_11_03 10:16 h1isibs
2015_11_03 10:18 h1isiitmx
2015_11_03 10:26 h1isietmx
2015_11_03 10:31 h1isietmy

Maintenance day. Power cycle of h1seib1, new BSC ISI models with reduced sensitivity to coil driver temp status bit when triggering watchdog.

Title:  11/04/2015, Day Shift 16:00 – 00:00 (08:00 – 16:00) All times in UTC (PT)
	
State of H1: 16:00 (08:00), The IFO is locked at NOMINAL_LOW_NOISE, in Observing mode 

Outgoing Operator: Jim

Quick Summary:  IFO locked in Observing for the past 9 hours. Winds are calm to light (0 – 3mph), seismic activity is quiet; microseism is centered around 0.3 um/s.   

     


A

Apologizes for the late entry.

Yesterday all site supply fans were lubricated per the quarterly schedule.

We also took the maintenance period opportunity to change some extremely dirty air filters which are located in the supply fan areas.

TITLE: 11/03 Owl: 8:00-16:00 UTC 
STATE Of H1: Observing @ ~75 MPc.
SHIFT SUMMARY: 
SUPPORT:
ACTIVITY LOG:

H1 was locked when I arrived, RF45 was acting up occasionally, though. Otherwise quiet shift.

15:00 UTC Started receiving CS temp notifications, Bubba notified/working on it.

This morning about 15:00 UTC, I got a couple notifications that temps were low in the LVEA. I let Bubba know, but he was already working on it. I haven't heard any notifications since, Bubba said he will keep an eye on it.

TITLE: 11/03 [EVE Shift]: 00:00-08:00 UTC (16:00-00:00 PDT), all times posted in UTC
STATE Of H1: Observing @ ~75 MPc.
SHIFT SUMMARY: Initial lock impeded by bounce and roll modes. Lost lock during earthquake in East Timor. Seismic stayed abnormally high for almost 2 hours. Recovered and back to observing.
SUPPORT: Evan, Jenne
INCOMING OPERATOR: Jim

ACTIVITY LOG:

00:13 UTC Kyle and Gerardo back from X28 (near end X)
01:25 UTC Towing truck through gate
04:36 UTC Nutsinee leaving, driving up bridge before heading out
04:40 UTC Jenne driving to end stations to turn card readers on
04:49 UTC Turned power off to speaker in control room
05:06 UTC Jenne back
05:45 UTC Restarted video2, Ops overview frozen

Seismic took about 2 hours to ring down to the point that we could relock. The 0.03 - 0.1 Hz seismic band is between ~ .02 and .1 um/s. The microseism is between ~ .1 and .2 um/s. The winds are around 10 mph.

Violin mode damping for ITMX and ITMY is off.

ISI blends are at Quite_90.

Jenne turned the card readers on at end X, end Y and the LVEA.

Range is around 78 MPc.

[Jenne, Miquel, Patrick]

The card readers providing access to the VEAs were turned off during maintenence today.  Since we're unlocked due to an earthquake anyway, they have now been turned back on (EX, EY and vertex).

SUS I_T_M_Y saturating (Nov 4 04:14:41 UTC)
DRMI Unlocked (Nov 4 04:14:41 UTC)
Intention Bit: Commissioning (Nov 4 04:14:41 UTC)
ISC_LOCK state: DOWN (Nov 4 04:14:48 UTC)

From USGS:
6.3 77km WNW of Dili, East Timor 2015-11-04 03:44:15 UTC 14.3 km deep

Spike to ~ .3 um/s in 0.03 - 0.1 Hz seismic band

Have remained in observing. No changes to report.

I have turned off the violin mode damping filters for IX and IY by zeroing their gains. Patrick accepted these into SDF so that we can go to observing.

This is meant to be temporary, i.e., for this one lock only.

The next time the interferometer comes into lock, the Guardian will turn on the normal violin mode damping settings. These settings will appear as SDF diffs (two on IX, and six on IY). These should be accepted into SDF.

We do not expect these modes to ring up during the course of the lock. However, if the mode height on the control room DARM spectrum around 500 Hz rises above 10⁻¹⁶ m/rtHz, the damping should be turned back on:

1. Make sure the ramp times for the damping filter modules are at least a few seconds (currently they seem to be set to 10 s).
2. The filters should already be configured to provide the right damping phase, so changing the filters should not be necessary.
3. Start typing in gain settings. Refer to the values listed below. If the violin mode amplitude is much much higher than usual (e.g., it's off the scale on the control room DARM spectrum), it is wise to start with a small gain (e.g, gain of ±1) in order to make sure the suspension drive does not saturate. Then you can increase the gain in several steps, until the nominal setting is achieved.

A screenshot of the nominal IY damping settings is attached (I didn't take one for IX).

ITMX:

• MODE3 gain: −100
• MODE6 gain: +200
• all others zero

ITMY

• MODE1 gain: −200
• MODE2 gain: −200
• MODE3 gain: +100
• MODE4 gain: −50
• MODE5 gain: +400
• MODE6 gain: +50
• all others zero

TITLE: 11/03 [EVE Shift]: 00:00-08:00 UTC (16:00-00:00 PDT), all times posted in UTC
STATE Of H1: Lock acquisition
OUTGOING OPERATOR: Jeff
QUICK SUMMARY:
Lights appear off in the LVEA, PSL enclosure, end X, end Y and mid X. I can not tell from the camera if they are off at mid Y.
Winds are less than 10 mph. Appear to be increasing.
ISI blends are at Quite_90.
Earthquake seismic band is between 0.01 and 0.02 um/s. Microseism is between 0.1 and 0.3 um/s.

Jeff has been having trouble with ITMY bounce and roll modes. Has been stopping at REDUCE_CARM_OFFSET_MORE to allow Jenne and Evan to investigate.

The DTT template for showing the MICH spectrum on the control room wall is suffering from leakage,  preventing us from seeing some features in the 8 to 11 Hz range. The current parameters and window are:

Window: Hanning

Start/end frequencies: 0/74444Hz 

BW: 0.1Hz 

Overlap: 70% 

Avarages: 3

Resulting BW: 0.18Hz

After playing with the available windows (but keeping all other parameters fixed so it will refresh with the same latency), I have found that Flat-Top reduces the resulting BW to 0.24Hz but also reduces the leakage problem. This would allow us to see features over the problematic range. The first two attached figures correspond to 2015-10-28 14:48:24 ; they show how the Hanning window suffers from a real leakage problem while Flat-top maintains it’s performance. The feature over 8Hz corresponds to a problem solved by Bubba on log (22939). 

We have a few piece of evidence that suggest that anthropegenic noise (probably trucks going to ERDF) couples to DARM through scattered light which is most likely hitting something that is attached to the ground in the corner station.

1. Our spectrum is more non-stationary between 100-200 Hz durring times of high anthropegenic noise. Nairwita noted this by looking through summary pages (these glitches only seem to appear on weekdays between 7 am and 4pm local (14-23UTC), and not on Hanford Fridays when anthropegenic noise is low), and Jordan confirmed this by making a few comparisons of high/low anthropegenic noise within lock stretches.  (alog 22594)
2. Corner station ground sensors are a good witness of these glitches.  HVETO shows this clearly (see page for October 14th for example).  Also, comparison of bandpassed DARM to several corner ground motion sensors and accelerometers show that glitches in DARM coincide with ground motion (for example see nutsinee's alog 22527)
3. The DARM spectragram at the time of these glitches show what looks like scattering arches from 1 Hz motion and a velocity of around 40 um second total path length change. alog 22523  Both this high velocity and the fact that the seismometers on the tables don't seem to witness this motion well suggest that something bolted to the ground is involved in the scattering. This velocity is probably too high for something bolted to the ground.
4. The scattering amplitude ratio (ration of scattered amplitude to DC readout light on DCPDs) we would estimate bassed on the fringes in DARM 1e-5, similar to what we got in April  Using the ISCT6 accelerometer to predict the velocity of the motion doesn't quite work out.
5. Annamaria and Roert did some PEM injections in the east bay, which showed a linear coupling to DARM.  Annamaria is still working on the data and trying to disentangle downconverion from the linear coupling, but if we assume that scattered light is responsible for the linear coupling the amplitude ratio is fairly consistent with what we got from the fringe wrapping when trucks go by.

On monday, Evan and I went to ISCT6 and listened to DARM and watched a spectrum while tapping and knocking on various things.  We couldn't get a response in DARM by tapping around ISCT6.  We tried knocking fairly hard on the table, the enclosure, tapping aggresively on all the periscope top mirrors, and several mounts on the table and nothing showed up.  We did see something in DARM at around 100 Hz when I tapped loudly on the light pipe, but this seemed like an excitation that is much louder than anything that would normaly happen.  Lastly we tried knocking on the chamber walls on the side of HAM6 near ISCT6, and this did make some low frequency noise in DARM.  Evan has the times of our tapping.

It might be worth revisiting the fringe wrapping measurements we made in April by driving the ISI, the OMC sus, and the OMs.  It may also be worth looking at some of the things done at LLO to look accoustic coupling through the HAM5 bellow (19450 and 

19846)

Now that we've cleaned up all of our systematics from the DARM model and released the O1 version (see LHO aLOG 22056, I've updated the diagram that explains how the actuation path clock cycle delay is derived, and also shows that the current value of 7 [clock cycles] or 427.3 [us] that was recently installed at both sites (LHO aLOG 21788) still does a fine job at approximating the total delay between the inverse sensing and actuation chains.