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Reports until 08:53, Tuesday 16 September 2014
H1 PSL (PSL)
peter.king@LIGO.ORG - posted 08:53, Tuesday 16 September 2014 (13944)
PSL Diagnostic Breadboard Scan
One thing to note about this week's diagnostic breadboard scans, is that the reference cavity transmission has deteriorated
down to ~1 V.  Although the power reflected by the pre-modecleaner is about the same, at ~ 2.1 W.  For reasons unknown at the
moment, the frequency stabilisation servo had a tendency to lose lock and/or oscillate.  I reduced the common gain from 30 dB
to 27 dB for these measurements to see if that'd make things a little more robust - at least whilst the scans were being
conducted.  The input modecleaner was flashing during this period too, which would partly explain why the reference cavity
was blinking.

The relative power noise measurement looks the same as last week.  Nothing significant to report.

During the frequency noise measurement, the input modecleaner lost lock which caused the reference cavity to lose lock.
The pull on the laser frequency was such that even the pre-modecleaner in the diagnostic breadboard lost lock for a split
second.  Both error and control signals are higher than the reference measurement, most likely because of the problems mentioned.
Both are about a factor of 100 higher than normal.  There is a peak both spectrums at 10 Hz that was not present in prior measurements.
The problems seem to also coincide with a peak in the 1-3 Hz seismic noise region.

A repeat of the frequency noise measurement when things appeared "quieter" still had a peak at 10 Hz.  The measurement was disturbed by
a period of oscillation due to the input modecleaner losing lock and trying to re-acquire.

The beam pointing measurement looks nominal.  Nothing significant to report.

The mode scan looks nominal.  4.3% higher order mode power, higher order mode count 54.

The intensity stabilisation power noise measurement looks good.  Better than the reference measurement everywhere except above ~7 kHz.
Non-image files attached to this report
H1 AOS
sheila.dwyer@LIGO.ORG - posted 00:07, Tuesday 16 September 2014 - last comment - 00:08, Tuesday 16 September 2014(13942)
PRMI sideband

Kiwamu, Dan, Alexa, Rana, Sheila

Today we spent most of the day working on PRMI sideband locked, we had trouble acquiring lock, Kiwamu thinks this is a problem with MICH.

Images attached to this report
Comments related to this report
kiwamu.izumi@LIGO.ORG - 00:08, Tuesday 16 September 2014 (13943)

PRCLloop open loop. The red trace is the new one and the black one is the old one.

Images attached to this comment
H1 AOS (TCS)
alastair.heptonstall@LIGO.ORG - posted 18:17, Monday 15 September 2014 - last comment - 18:45, Monday 15 September 2014(13927)
TCS CO2 projection system Y-arm table is ready

Alastair & Greg

On Saturyday we finished with the alignment on the Y-arm table and made an off-table projection of the beam to check the size and shape.  Photo of the bench is attached.  The visible laser was aligned to the CP and the CO2 laser coaligned to the visible laser.  It should all be ready for testing on the CP now.

Some notes:

There are a few things still not in their final configuration.  Firstly we need to fab a housing for the FLIR camera to match the X-arm one.  Then the camera needs installed on the bench.  We also need to install the IR sensor on the viewport before the system is run long-term unattended.  The laser had a problem with its RF driver and we swapped in a spare but were missing power connectors (5pin 40A connec) so at the moment the laser is running on a Sorensen next to the table.  The connectors are ordered.  The mask is mounted in its flipper mirror but the flipper is not connected up yet.  The flipper also needs the up/down sensor.  And we still need to put in the second flipper with the annular heating mask.

Data from this table:  Will add this once I locate my notebook, but the following was measured:

Polarizers 2 & 3 extinction ratios measured: 

Power meter used to calibrate output power to CP as a function of rotation stage (1/2 wave plate) angle :

QPDs are installed and aligned.  Each quadrant calibrated for power and center position measured.  We'll need to decide if we want to calibrate for position or use the values from the X-table where the QPDs are mounted on translation stages.  Calibration data: 

Images attached to this report
Comments related to this report
greg.grabeel@LIGO.ORG - 18:45, Monday 15 September 2014 (13940)TCS

Here is the result of the ITMy projection. The image was taken with the FLIR PM695 pointed at our target (a black piece of construction paper) 14m away from the periscope. Attached on the left is a 12" ruler for scale. Here you can see the heat profiles taken from a horizintal and vertical line across the projection. 

 
Images attached to this comment
H1 ISC
keita.kawabe@LIGO.ORG - posted 17:53, Monday 15 September 2014 - last comment - 18:25, Monday 15 September 2014(13939)
Crude output matrix to walk the beam on PR2

Since it seems like a cumbersome job to walk the beam on PR2, I calculated the necessary combination of optics to walk the beam on PR2 without affecting the beam position and angle on BS and ITMs. I put this combination in INP2 of the WFS output matrix (as INP1 is being experimented for WFS).

You should be able to, say, give INP2 WFS filter an offset to manually walk the beam, and/or you should be able to route one of the POP sled QPD signal to it to servo the beam position on PR2.

Images attached to this report
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keita.kawabe@LIGO.ORG - 18:25, Monday 15 September 2014 (13941)

Calculations

IM4:

You turn IM4 by theta0 and the beam is deflected by 2*theta0.

PRM rotation:

Assume that the beam was perpendicular to both AR and HR before IM4 was rotated.

After IM4 rotation, in order for the PRM to retro-reflect the beam,  you tilt the PRM by theta1 so the incident angle becomes 2*theta0-theta1.

The beam angle inside the PRM relative to the AR face is therefore (2*theta0-theta1)/n.

The beam position on PRM is L1*2*theta0 where L1 is the IM4-PRM distance (ignore the thickness of the PRM).

In order for HR side to retroreflect, the beam angle should match the HR side angle:

(2*theta0-theta1)/n = L1*2*theta0/R

where R is the ROC of PRM HR.

theta1=2*theta0*(1-n*L1/R).

PR2 and PR3 rotation:

M0=ABCD matrix from IM4 output to PR3 output.

M1=from PR2 output to PR3 output.

input vector at IM4 output is inV=[0; 2*theta0]. 

PR2/PR3 rotation of theta2/theta3 is represented as [0; 2*theta2] and [0; 2*theta3] at the output of PR2/PR3.

theta2 and theta3 are determined by the following equation:

M0*inV + M1*[0, 2*theta2] + [0, 2*theta3]=0.

Parameters used:

ROC were taken from nebula web page (-10.948m, -4.543m and 36.021m for PRM, PR2 and PR3).

IM4-PRC distance was roughly eyeballed to be 20inches from D0901083.

PRM-PR2 and PR2-PR3 were taken from T0900043, i.e. 16.6037m and 16.1558m respectively.

I flipped the sign of PR2 component for PIT (but not for YAW) due to the way the local coordinate is defined for SUS.

H1 CDS
james.batch@LIGO.ORG - posted 17:38, Monday 15 September 2014 (13938)
Changed default print driver for matlab
Changed default print driver for matlab to psc2 to enable color printing on the control room printer.  Was originally ps2.
H1 SEI
hugh.radkins@LIGO.ORG - posted 17:19, Monday 15 September 2014 (13937)
ISI TFs Set to start on WHAMs 2 & 4 ~Midnight pdt

I'm attempting two jobs on opsws3.  Please take it easy on this work station but I won't say don't use it.

Please reenable any watchdog trips on the HEPI, ISI, and SUS.

H1 SEI
jim.warner@LIGO.ORG - posted 16:18, Monday 15 September 2014 (13936)
TFs set to run on I/ETMX ISI's
My tf on Sat at ITMX went poorly, so I will be taking a new tf ITMX, starting at midnight tonight. Re-taking tf's on ETMX, because I have the opportunity, and I haven't taken good data there since the last time we opened.
H1 General
jeffrey.bartlett@LIGO.ORG - posted 16:03, Monday 15 September 2014 (13935)
Ops Summary
LVEA is Laser Hazard

09:49 Hugh – Recycling HAM5 HEPI
10:04 Aaron – Installing illuminater chassis at HAM2 and HAM5
10:18 Betsy & Travis – Working in west bay on 3IFO Quads
10:40 Dave – Cabling at the HAM6 bay
13:12 Karen – At Mid-Y
14:20 Besty & Travis – Working in LVEA west bay on 3IFO Quads
14:37 Peter – Going to Diode room to reset PSL watchdog

H1 AOS
jason.oberling@LIGO.ORG - posted 14:12, Monday 15 September 2014 - last comment - 14:33, Monday 15 September 2014(13932)
ITMy Optical Lever - Solved!

Jason, Rana, John

Credit for this one goes to John Worden.  He noticed the sawtooth pattern seen by the ITMy optical lever was very similar to that produced by the instrument air system re-pressurizing itself.  Sure enough, we go out and the copper instrument air line is touching the north end of the ITMy transmitter pier, so we moved it.  As can be seen on the attached graph, after the move the sawtooth pattern was gone.  I'll keep an eye on this over the next couple days to make sure this is actually fixed.

Images attached to this report
Comments related to this report
jason.oberling@LIGO.ORG - 14:31, Monday 15 September 2014 (13933)

Picture of the fix, taken by Rana.  We need to keep an eye on this, and come up with a more permanent fix (right now it would be very easy for someone to mistakenly bump the line right back against the pylon, thereby re-introducing the sawtooth).

Images attached to this comment
rana.adhikari@LIGO.ORG - 14:33, Monday 15 September 2014 (13934)

In the trend plot above, the calibration of the pit/yaw channels is in units of microradians. Also, during searches for the problem, we have adjusted the laser diode drive current to a higher power. We need to scribe/tape the laser diode knobs to keep the diode current stable.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 13:26, Monday 15 September 2014 (13931)
PSL Status
PSL Status: 
SysStat: Green 
Output power: 33.7w  
Frontend Watch: Red
HPO Watch: Red  

PMC:
Locked: 3 days, 14 hours, 33 minutes
Reflected power:    2.0w
Power Transmitted: 22.9w 
Total Power:       24.8w 

FSS:
Locked: 0 days, 1 hours, 40 minutes
Trans PD: 0.586v

ISS:
Diffracted power: 11.206%
Last saturation event: 3 days, 14 hours, 24 minutes  
H1 CDS
david.barker@LIGO.ORG - posted 10:50, Monday 15 September 2014 (13930)
summary of DAC lock out events

Frequency of DAC lock out events (requiring IOP model restart to fix). Two more events since my last summary alog Link

9/11 2014 h1seih45

9/10 2014 h1seih23

8/11 2014 h1susb123

8/9 2014 h1seih23

4/21 2014 h1sush2a

3/18 2014 h1sush2a

2/27 2014 h1seih23

12/16 2013 h1seih23

11/7 2013 h1sush2a

11/7 2013 h2sush34

8/8 2013 h1seih23

H1 SEI
hugh.radkins@LIGO.ORG - posted 10:07, Monday 15 September 2014 (13929)
WHAM5 HEPI Controllers now 2hz ugf generic rather than 5hz generic

Like HAM4, no problem taking HEPI down with Guardian, loading the new filters and bringing the loops back on with Guardian all while the ISI remains isolating.  Checked DTT and it looks better but I really need the full TF-hopefully tonight.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 09:30, Monday 15 September 2014 (13928)
08:30 Meeting Minutes
SEI – Working on TFs on HAM2 and HEPI commissioning

OpLev – Working on ITMY sawtooth laser glitch. 
	       Swapping BeamSplitter laser due to glitch

TCS – Laser alignment of TCS-X table

Test Mass Charging experiment is making measurements in the LVEA west bay cleanroom
H1 SEI
hugh.radkins@LIGO.ORG - posted 08:26, Monday 15 September 2014 (13926)
WHAM2 ISI TFs only partial completed. Change in HEPI resonances consistent.

The HAM2 TF data after the 1st couple of sections got corrupted so this needs to be run again.  Still, we can see that again the sharpe peaks between 10 & 40 hz, believed to be HEPI structures, are lowered in frequency and Q.  Also, the H3 CPS response does not develop into the deep zero around 6-7hz.  The lower UGF of 2hz on the HEPI position controller is believed to be the reason.  The attached plot compares the HEPI locked to closed HEPI Position loops ISI TFs.

Images attached to this report
H1 PSL (PSL)
peter.king@LIGO.ORG - posted 08:15, Monday 15 September 2014 (13925)
PSL chiller water level top up
Heard the chiller alarm this morning.  Found the water level to be a little below minimum.  Added about 400 milliliters.
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