Displaying reports 64201-64220 of 77217.Go to page Start 3207 3208 3209 3210 3211 3212 3213 3214 3215 End
Reports until 14:39, Wednesday 13 August 2014
H1 TCS (TCS)
greg.grabeel@LIGO.ORG - posted 14:39, Wednesday 13 August 2014 (13392)
Polarizer Window Bonding

The polarizers were retested today after #015 was redone by Alastair and the silicon had some time to cure. I remeasured the offset of all the polarizer windows, where ↑ is right side up for the label and ↓ is upside down with the label. Nominal height is 4" but it looks like there was a slight upward angle from the mirror.

015 4 1/32" 0.3 mrad
4 3/32" 0.9 mrad
011 4 1/16" 0.6 mrad
4 1/32" 0.3 mrad
009 4 1/16" 0.6 mrad
4 1/16" 0.6 mrad
008 4 9/32" 2.8 mrad
3 5/8" 3.1 mrad
001 3 13/16" 1.3 mrad
4 1/4" 2.5 mrad
The requirement is 7 mrad so all of the new polarizer windows look good.
H1 ISC
alexan.staley@LIGO.ORG - posted 14:22, Wednesday 13 August 2014 - last comment - 11:49, Friday 15 August 2014(13391)
Beam Path in HAM6

(Koji, Alexa, Dan)

 

We examined the beam path in HAM6 to OM1 in order to figure out the angle of the beam. We made measurements at four different points. Using an (x, y, z) coordinate system with z = up, y = East, x = South, we find at (all in mm):

Edge of table: (20.32, 0, 98)

Intermediate point 1: (0, 552.72, 95)

Intermediate point 2: (-25.4, 1219.2, 93)

OM1: (-40.64, 1574.8, 91)

The error of the measurement in height is ±1mm, and the error along the x, y axis is ±2.5mm. The attached layout shows the original (red) beam path and the new (green) beam path. From this layout, one can see the actual vs. measured angle deviation in height and along the hoirzontal plane.  Using the points above, we made a linear regression and determined the vertical angle of the beam to be 4.3 mrad. The attached plot shows the data with error bars and the linear fit. 

Images attached to this report
Non-image files attached to this report
Comments related to this report
keita.kawabe@LIGO.ORG - 17:27, Wednesday 13 August 2014 (13399)

So the situation now is this:

  angle of the beam [mrad] position of the beam at OM1 design center [mm]
PIT (positive=up) -4.3 -10.6
YAW (positive=North) (-39.7, though the absolute number is not that important here.) -50.8mm

Because of this, Koji had to tilt the OM1 up by about 4.3mrad, which is big, and I'd say that there's a high chance we will want to fix the beam angle some time in the future (e.g. larger bounce to alignment coupling).  YAW is not that much of a problem because there's enough space to absorb -50.8mm.

We've been discussing how to alleviate this, and the simple hack is to rotate the septum window, which is supposed to have a 0.75deg horizontal wedge which causes 5.9mrad deflection.

According to ICS (via Joe), we should have D1101092 S/N assembly, which should have D1101005 window S/N15, which has dimension measurement that suggests 0.745deg wedge.

However, Koji measured the wedge using laser pointer and got 0.89deg which should cause 7.0mrad deflection. His measurement also suggests that the thickest side is facing south.

Now, when we rotate the septum window by X (positive=clockwise), PIT deflection was zero before but now the beam is deflected vertically by sin(X)*5.9mrad (or 7.3mrad).

Horizontally,   the deflection is -5.9mrad (or -7.3) before rotation, and -cos(X)*5.9mrad (or 7.3) after, so the change in the angle would be 5.9mrad*(1-cos(X)).

If we optimize the septum rotation (which only changes by 30deg steps) for 0.75deg septum we need to rotate the septum by 120 deg clockwise.

For 0.89deg septum wedge, it would be 150deg clockwise. See below.

(The beam position change at OM1 is calculated by using 1.93m as the distance from OM1 to the septum.)

Septum rotation (deg) Septum wedge (deg),
and deflection (mrad)
PIT deflection change (mrad) PIT beam pos at OM1 (mm) PIT beam angle (mrad) YAW deflection change (mrad) YAW pos at OM1 (mm)
120

0.75, and 5.9

+5.1

-10.6+5.1mrad*1930mm
= -0.8mm

5.1-4.3=+0.8mrad

+5.9+2.95

=8.85

-50.8+8.85mrad*1930mm
=-50.8+17.1mm

0.89, and 7.0

+6.1

-10.6+6.1mrad*1930
= +1.2mm

+6.1-4.3=+1.8mrad

+7.0+3.5
=+10.5

-50.8+20.3mm

150 0.75, and 5.9 +2.95 -10.6+2.95mrad*1930
= -4.9mm
+2.95-4.3=-1.35mrad +5.9+5.1
= +11.0
-50.8+21.2mm
0.89, and 7.0 +3.5 -10.6+3.5mrad*1930
= -3.8mm
+3.5-4.3=-0.8mrad +7.0+6.1
= +13.1
-50.8+25.3mm

Anyway, there's not much difference, but since the ICS says 0.745deg wedge, we need to rotate it by 120 deg clockwise if we decide to do it.

koji.arai@LIGO.ORG - 07:27, Friday 15 August 2014 (13419)

Keita and I concerned about the AR reflection from the septum. We thought we should at least check where the AR reflection goes.
This required to make a 3D version of the ray tracing. The result is, in short, the rotation of the wedged window(by 120 or 150deg)
makes the returning beams closer to the arrangement with the nominal beams. They fly about 30-40mm North of the aperture on Faraday.


In this entry, the wedge angle of 0.75 deg is assumed.

The "nominal" beam means: "Use the HAM6 dawing. Assume this incorporates the wedging effect by the septum window."

The "actual" beam means: "Use the measured beam geometry in HAM6."

The "actual+120" and "actual+150" means: "The beams expected by rotating the septum by 120 or 150 deg in CW. The "actual" beam used for the calculation.


1st attachment is an example view of the ray tracing result.


2nd attachment shows the spot positions on OM1 viewed from the back side of OM1.
Rotation of the septum by 120 deg makes the spot close to the "nominal" beam position.
"+120deg" gives us better result than "+150deg".

Note that the result I obtained here are consistent wth Keita's handwriting calculation for the OM1 spots.


3rd attachment

The beam was back-traced to HAM5. We expect that there is a 20mm aperture (iris) at 315mm from the septum window.
It is assumed that the apertue is located at the beam properly. The primary and secondary reflections are located about 35~40mm North of the aperture.
According to D0900623, these beams might be hitting the beam dump for the PBS, but not so clear.

4th attachment

This time, the actual beam was traced-back. Without rotation, the secondary beam definetely hits the apeture structure.
The primary reflction is ~30mm away from the aperture. The rotation moves the secondary reflection further away to North.
Vertical displacement is 5~10mm. So, we can say that the rotation makes the spots close to the original positions.

Images attached to this comment
keita.kawabe@LIGO.ORG - 11:49, Friday 15 August 2014 (13431)

In all of these cases, it seems like all ghost beams will fall on the Faraday Isolator Refl Baffle which is mounted on the suspension cage.

https://dcc.ligo.org/LIGO-D0900136 (Output Faraday Assy)

https://dcc.ligo.org/D0902845-v5 (Faraday Isolator Refl Baffle)

H1 CDS (PEM)
david.barker@LIGO.ORG - posted 13:54, Wednesday 13 August 2014 (13390)
h1oaf0 rebooted to clear zero'ed ADC channels

Robert, Christina, Dave

Robert and Christina reported some corner station PEM channels with ADC values of zero. I power cycled the h1oaf0 front end computer and its IO Chassis and these channels are now non-zero.

Sequence was:

LHO VE
kyle.ryan@LIGO.ORG - posted 13:05, Wednesday 13 August 2014 - last comment - 15:41, Wednesday 13 August 2014(13389)
UPDATE: Corner Station pumpdown
Investigation reveals that all (3) running turbos on site (YBM, XBM and X-end) shut down simultaneously at 1603 hrs. local time yesterday -> Coincidentally, this was only a few minutes prior to my opening of GV2 -> As such, my earlier theory of the XBM turbo tripping off on its safety valve pressure setpoint turned out not to be the case -> This is confirmed also by the fact that PT170A never came on scale.

Today at ~1230 hrs. local -> I spun-up to 100% rpm the troublesome XBM turbo by employing the technique of "loading" the rotor.  To do this, I maintained the turbo inlet pressure at ~ 0.2 torr by adjusting the "up-to-air" needle valve at the turbo's inlet while it spun-up -> Once at full speed, I shut off the air and eventually valved-in the turbo to the XBM volume.  


ERRORS in PRESSURE GAUGES
Also, the LHO vacuum equipment is beginning to show its age as we have been experiencing an increase in the failure rate of the site cold-cathode gauges (lifetime maturation) -> most noticeably PT180B, PT120B and PT170B are reading bogus values now for portions of their nominal range.  As of this writing, both the YBM and XBM turbo inlet CC gauges are reading 1.8 x 10-6 torr which is what I would expect for the recent history -> I would then guess the pressure at BSC2 to be 5-7 x 10-6 torr
Comments related to this report
john.worden@LIGO.ORG - 15:41, Wednesday 13 August 2014 (13395)

Photos of the violent dust storm approaching are here:

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=13366

and here:

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=13365

H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 12:33, Wednesday 13 August 2014 (13388)
CDS model and DAQ restart report, Tuesday 12th August 2014

There were 167 restarts due to storm related power glitching. Also some unexpected restarts of h1fw1. I have attached the list to spare the casual reader the gory details.

Non-image files attached to this report
H1 TCS (TCS)
greg.grabeel@LIGO.ORG - posted 12:01, Wednesday 13 August 2014 (13344)
A Tale of 3 Lasers

It was the best of lasing. It was the worst of lasing. It was the best of shipments (although still bad). It was the worst of shipments. It was the season of single mode. It was the season of no modes. TCS has now received back the lasers that were sent to Access for repairs. Unfortunately the first shipment containing Lasy-50 20510-208160 and RF50 208160-20510 was sent to Caltech (an oversight in shipping) and then to Hanford. It was worse for the wear and the RF driver was busted, it was blowing fuses. Using the RF50 210040 to drive the laser proved more fruitful, while RF50 208160-20510 will be sent back to Access for repairs. Here are the laser/RF driver pairs and their outputs (running at 99% duty cycle) as tested:

Laser RF Driver Watts Notes
20510-208160                  210040                            ~53           RF50 208160-20510 Broken
20708-208100 20708-208100 ~53 RF50 water inlets bent
210020-20710 20710-210020 ~52 RF50 broken water inlet, replaced. Break in wire sheath, fixed.

Attached are some of the photos from the process, including the beam on an IR card.

Images attached to this report
H1 AOS (AOS)
filiberto.clara@LIGO.ORG - posted 11:43, Wednesday 13 August 2014 (13387)
OP Lev Whitening Chassis EX / EY
Replaced insulating film used to isolate the -15V regulators to the chassis metal wall for OP Lev Whitening chassis at end stations.

EY - S1101539
EX - S1101552

Filiberto Clara
H1 DAQ
james.batch@LIGO.ORG - posted 10:50, Wednesday 13 August 2014 (13385)
Restarted daqd on h1nds1 to test copied raw minute files.
The daqd process was restarted on h1nds1 to test the copied raw minute files.  WP 4790.
X1 DTS
james.batch@LIGO.ORG - posted 10:08, Wednesday 13 August 2014 (13383)
The x1work computer is down on the DAQ test stand.
The x1work computer won't boot to Ubuntu 12.04.  It is up temporarily in Ubuntu 10.04 to allow access to user's home directories.  Don't do anything serious on it, it will be rebuilt after the power fail scheduled for tomorrow.  Home directories and /ligo will be preserved since they are on separate disks.
H1 General
jim.warner@LIGO.ORG - posted 09:21, Wednesday 13 August 2014 (13382)
Morning meeting minutes
HAM6 alignment work ongoing
IMC ring down measurements
PR3 oplev almost done
ISS arrays being finished up
Power cabling for PEM chassis
Pulling cables for UW tilt meter
EX tilt meter testing ongoing
EY charging measurements ongoing

Safety Meeting this aft

H1 SUS
borja.sorazu@LIGO.ORG - posted 22:18, Tuesday 12 August 2014 (13380)
ETMY charge repeated measurement and chronology of previous measurements and discharge runs

(Borja)

First of all let us compile the chronological time information of the measurements and the discharge runs:

* Measurement 1 (before any discharge): took  place between UTC (2014-08-07 07:00:00) and UTC (2014-08-07 08:25:00).

* Discharge run 1: between UTC (2014-08-07 19:15:00) and UTC (2014-08-07 19:44:00).

* Measurement 2 (after 1st discharge run): between UTC (2014-08-8 18:00:00) and UTC (2014-08-8 19:30:00)

* Discharge run 2: between UTC (2014-08-08 20:48:00) and UTC (2014-08-08 21:38:00).

* Measurement 3 (after 2nd discharge run): between UTC (2014-08-10 00:00:00) and UTC (2014-08-11 02:00:00)

* Ion pumps in ETMY station was turned ON at UTC 2014-08-11 16:44:00. Notice from this entry that the ion pumps were OFF between discharge 1 and discharge 2 maybe that is why we see a charge reduction after each of these discharges. However the first charge measurement done above (before any discharge run) was done after several days of having the ion pumps on so why the ETMY had not bigger charge?

* Measurement 4 (2nd measurement after 2nd discharge run): between UTC (2014-08-11 20:31:17) and UTC (2014-08-11 23:00:00)

* Measurement 5 (3rd measurement after 2nd discharge run, this measurement is reported in this entry below): between UTC (2014-08-12 17:17:00) and UTC (2014-08-12 19:09:00)

Yesterday ETMY charge results (Measurement 3) were telling us that the ETMY was charging again since the 2nd discharge took place. What is charging the ETMY then? There are 6 mechanisms (that we can think of at the moment) that would cause ETMY charging and that they are different to the original MIT charging measurements, these are:

1)       Green light (through 2 photon process). MIT measurements did not include green light tests. But the green light is not on at the moment.

2)       The rubber stops on the reaction mass (seismic stoppers) with silica tips through silica to silica friction. The MIT tests did include these rubber stops and they did not observe any noticeable effect on the charging. Certainly they are installed in the ETMY reaction mass so they could be playing a role in the ETMY charging but it is hard to believe they would charge the mass so much in only 1 day.

3)       LED illuminators that were turned on from the first discharge run to see effect on the ETMY surface. They have not been turned off since (although there is no reason to keep them on at the moment apart of testing the current charging hypothesis). Again it is hard to believe that a broad angle not extremely bright LED can charge so much a mass in only 1 day.

4)       First contact. For the original MIT tests the masses were not covered with first contact. It is not secret that then removing the first contact layer the mass is charged. But no first contact has been applied or removed for the length of the discharging measurements.

5)        Discharge gage (aka 'cold cathod') this is the very low pressure sensor at the ETMY tank (BSC10). It operates in a similar fashion to an ion pump in which uses ion to pump out some air to sense the pressure. The amount of ions this one uses is considerably smaller than the ion pump (see below) however it is much closer to the ETMY mass.

6)       Ion pumps. This is a new game player. The MIT ion pumps were not used during their tests, so there is not measurement of their effect on the mass charge. Torsion experiments with fused silica fibres indicate that ion pumps do cause considerable charging. As I have describe above this is consisten with what we have seen. The ion pumps were OFF between discharge runs and in both cases we measured charge reduction on the ETMY, however after they were turned on they ETMY started to charge again (notice that the LED iluminators were ON during the 2nd discharge and never turned OFF yet so if it was the iluminator charging the ETMY then why we saw charge reduction one day after the discharge?). The only think that may  not agree with the ion pump being the charger is why the first measurement (Measurement 1) shows such small charging levels while the ion pumps were ON for days before that measurement took place?

However let's see now the results of today's measurement (nothing was changed respect to yesterday's measurement) there is only 1 day different in the measurement, see notes with the measurement values attached here as well as the plots of Normalized pitch and yaw deflection vs. VBIAS comparing measurements of today (identified in the legend as ending with 23) with the ones from yesterday (identified in the legend as ending with 22), I have also plotted a zoom version looking at the Veff (or zero crossing of the deflections. I show next the table summary with red for yesterday's results and green for today's. It is clear that the EMTY has charged considerably, which again seems to confirm the ion pump charger hypothesis.

 

UL after22

UL after23

UR after22

UR after23

LL after22

LL after23

LR after22

LR after23

Veff PITCH [V]

123

228

65

-169

61

-130

85

153

PITCH slope [10-7 µrad/V]

-2.565

-2.606

2.1605

2.305

2.154

2.053

-2.612

-2.635

Veff YAW [V]

177

320

70

-11

54

-39

100

227

YAW slope [10-7  µrad/V]

-2.178

-2.226

2.428

2.489

-2.271

-2.215

2.374

2.308

Still there is one more variable in all this charging measurement game. Remember that one of the ESD quadrants could not be driven (quadrant LL) because its driving signal was going through the ESD low pass filter box, designed to filter the ESD BIAS frequencies above 1Hz, and the driving signal for these measurements is at 4Hz. This was solved before yesterday’s measurements, however are we sure that this change has not caused a different electric field configuration on the ETMY therefore making it incomparable with any other previous measurement? I had tried to run another measurement by bringing the cable configuration to the original case however between some power glitches bring the CDS down and affecting the suspensions controls at end station together with the higher seismic noise due to the sand storm has so far made this measurement impossible as the SNR is too low.

At the moment the ESD cables are as per the old configuration.

Images attached to this report
Non-image files attached to this report
H1 ISC
alexan.staley@LIGO.ORG - posted 20:40, Tuesday 12 August 2014 - last comment - 10:21, Wednesday 13 August 2014(13378)
IMC Length Measurement

(Dan, Alexa)

Since the MC cavity length was adjusted, we repeated the MC cavity length measurement as described in alog 9679.

Data_refl9_short.txt is the data collected using REFL9. ArmCavityLength_v2.m is the script that determines the length given the zero crossing of the projection. The attached plot show the results with a linear regression included.

 

The cavity length is determined to  be L = 16.471698m ± 4um assuming 2 Hz accuracy. The 2 Hz accuracy comes from the accuracy of the IFR plus the extreme rattyness of the transfer function.

Compared to the previous measurement the delta L = L_old - L_new =  0.001914 ± 6um. This is very close to the expected 2mm reduction in length as mentioned in alog 12654.

 

If desired, we can repeat the measurement and include a zero crossing for REFL45 as well. However, we just wanted to make a measurement and get the result public...

Non-image files attached to this report
Comments related to this report
daniel.sigg@LIGO.ORG - 10:21, Wednesday 13 August 2014 (13384)

Looking at the PRC length measurement from alog 10642, we can reevaluate the relative length mismatch:

Parameter Value Unit
FSRPRC 2.600075 MHz
LPRC 57.6508 m
FSRMC 9.100229 MHz
LMC 16.471698 m
FSRMC / 3.5 - FSRPRC -5 Hz
(1 - FSRMC / 3.5 FSRPRC) LPRC 0.1 mm
(1 - 3.5 FSRPRC / FSRMC) LMC -0.03 mm

Right on target! 9.100230 MHz should become the new modulation frequency.

Non-image files attached to this comment
H1 SEI (DetChar)
krishna.venkateswara@LIGO.ORG - posted 20:23, Tuesday 12 August 2014 (13377)
H1 EX BRS Installation, Day 6: Transfer function measurement and tilt from dust storm
Jeff K., Krishna V.

The pressure at the Turbo was 1.2E-6 torr this morning. The transfer function measurements have been less than convincing today. For now, I think d may be (+12.5 +/- 5) microns. I think cross-couplings (twist to tilt) may be introducing larger errors in this measurement than what I'm used to in the lab, where I have a much sturdier platform. The above value of d gives a displacement rejection of (9E-5 +/- 4E-5) rad/m. 

I have attached an ASD plot of 10k seconds of data from late last night/early morning, showing a very quiet ground, at the level of 0.1 nrad/rt(Hz). The blue curve, labeled tilmeter, is the measured tilt and the reference mirror curve is a ~ proxy for the autocollimator noise. We were hit with a dust storm around 4 PM this afternoon which produced lots of tilt noise, shown in the second graph, which was taken from ~5:25-6:30 PM. The noise near 0.1-0.5 Hz appears to be a factor of 10-100 worse. Wind speeds in that time frame were in the 30-40 mph range.

The pump has been turned off and I'm doing another overnight measurement. Tomorrow we will decide how much mass to add to try and reduce d as much as possible.
Images attached to this report
H1 ISC
alexan.staley@LIGO.ORG - posted 20:07, Tuesday 12 August 2014 - last comment - 17:56, Wednesday 13 August 2014(13375)
HAM6 Septum Angle Measurement

(Dan, Koji, Masayuki, Alexa)

We measured the HAM6 septum angle using a laser pointer. We confirmed that there was no observable vertical component to the wedge angle, and then proceeded to measure the horizontal angle. We pointed the laser pointer such that the retro-reflected beam off the surface of the septum returned approximately directly back. Then we measured the distance from the second reflection to this point. This distance was 17mm. The distance from the laser pointer to the septum was measured to be 360mm.

This gives: wedge horizontal angle: 17/360 * 180/pi /2 /1.45 = 0.93 deg

In the equation above the factor of 2 comes from the optical lever effect. Meanwhile the factor of 1.45 comes from applying snells law with the index of refraction for glass and assuming the small angle approximation (see attached drawing).

This measurement was not extremely precise, but was close enough to the expected value of 0.75 deg.

In the attached picture, you will see the retro-reflected beam, which is almost ontop of the outgoing beam, and the second reflected beam. We used the ruler below to measure the separation.

Images attached to this report
Comments related to this report
koji.arai@LIGO.ORG - 17:56, Wednesday 13 August 2014 (13400)

Koji

As the things are getting more precise, I pulled out my old raytracing calculation for an wedged angle.
This gave me the wedge angle of 0.91deg.

This includes the new effect of
- Refractive index of fused silica at 632.8nm (n=1.457)
- Average thickness of the window ((0.948+0.870)/2 = 0.909" = 23.1mm)
- Non-orthogonal input angle

The primary beam is distant from the laser diode by -8mm while the secondary beam from the backsurface is at +9mm.
This condition was fullfilled when the wedge angle is 0.91deg.

The attached plots are:
Attachment1: The overview of the rays
Attachment2: Zoomed view of the optic part
Attachment3: Zoomed view of around the source

Images attached to this comment
H1 ISC
koji.arai@LIGO.ORG - posted 19:54, Tuesday 12 August 2014 - last comment - 20:53, Tuesday 12 August 2014(13363)
HAM6 alignment work progress

[Alexa, Masayuki, Dan, and Koji]

A beam found on one of the OMC QPDs. The fast shutter beam dump elevated.

- We went into the cavity and spent some time to align OM2 and OM3 to have a beam aligned to the OMC.

- We confirmed the beam is hitting the QPDA (short arm one).

- The beam is still misaligned (mainly in yaw) at QPDB.

- We want decent damping of OM1. OM1 has too much tilt and requires adjustment on OSEMs. We are working on this.

 

- The beam dump for the fast shutter need to be raised by an inch. Betsy provided us a set of suspension addon masses
to make the post longer. Using one of them, We successfullt elevated the height of the beam dump by 20mm. This was
enough to accommodate the beam including the possible wobbling of the mirror on the fast shutter.

Images attached to this report
Comments related to this report
daniel.hoak@LIGO.ORG - 20:53, Tuesday 12 August 2014 (13379)ISC, SUS

In trying to re-center the BOSEMs for OM1 (which were off thanks to the large pitch necessary to center the beam on OM2), we found that the flag of LL was contacting the inside of the BOSEM (either the LED or the PD barrel, can't tell which).  This is the same problem that was observed previously on OM2 in alog:12352 and alog:12382.  We managed to twist the LL BOSEM by turning one of the PEEK adjustment nuts in, and turning the other out; this appeared to free the mirror, but the power glitches struck before we could check if the flag was appropriately centered in the PD/LED path.  Checks from the control room after CDS was recovered were not promising.  Probably the pitch correction is so large that we'll need to make some adjustments to the balance of this mirror.  To be continuted tomorrow.

H1 SUS
arnaud.pele@LIGO.ORG - posted 18:17, Monday 11 August 2014 - last comment - 21:05, Tuesday 12 August 2014(13305)
MC2 top mass dc coupling

Gains to decouple bottom mass (pitch and yaw) angular motion from top mass longitudinal drive at DC were implemented in L2P and L2Y components of the top mass drivealign matrix of MC2 using the dc magnitude of the top to bottom L2P (urad/Force cts) and P2P (urad/Torque cts) for length to pitch decoupling and L2Y, Y2Y for length to yaw decoupling. This should be tested.

  alpha
[urad/Force cts]
beta
[urad/Torque cts]
alpha/beta [Torque cts/Force cts]
in pitch -3.90E-03 5.37E-01 -7.26E-03
in yaw 2.20E-03 4.11E-01 5.35E-03


 

Images attached to this report
Comments related to this report
arnaud.pele@LIGO.ORG - 21:05, Tuesday 12 August 2014 (13376)

Attached are the plots of the undamped top to bottom TFs with cross couplings terms. The data cursor shows where I get the numbers from the table above from. The minus sign for Presp/Ldrive comes from the -180 degrees phase.

Non-image files attached to this comment
H1 AOS
filiberto.clara@LIGO.ORG - posted 14:50, Monday 11 August 2014 - last comment - 14:26, Wednesday 13 August 2014(13337)
ETMY and ETMX ESD
Added the ESD Bias Path Filter Box (D1400192) to both ETMY and ETMX.
Units filter voltage noise present on the ETM bias path of the ESD HV drive.

Due to wiring differences inside the chamber, the filter units were connected as follows:
ETMY connected to pin 1 (Flange F2-3)
ETMX connected to pin 3 (Flange F2-3)

Filiberto Clara
Comments related to this report
filiberto.clara@LIGO.ORG - 14:26, Wednesday 13 August 2014 (13393)
EX
Current Limit Box D1201288      SN S1400223
ESD Bias Path Filter D1400192 SN S1400403

EY
Current Limit Box D1201288      SN S1400224
ESD Bias Path Filter D1400192 SN S1400405
H1 INS
jim.warner@LIGO.ORG - posted 16:14, Friday 01 August 2014 - last comment - 19:39, Tuesday 12 August 2014(13165)
TF set to run on ETMX ISI, from opsws8


			
			
Comments related to this report
arnaud.pele@LIGO.ORG - 19:39, Tuesday 12 August 2014 (13374)

restarted it at 7:38pm since it crashed after the first power glitch

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