Displaying reports 46961-46980 of 87739.Go to page Start 2345 2346 2347 2348 2349 2350 2351 2352 2353 End
Reports until 17:36, Monday 14 May 2018
LHO VE
chandra.romel@LIGO.ORG - posted 17:36, Monday 14 May 2018 - last comment - 17:38, Monday 14 May 2018(41978)
HV1600-10 pressure + RGA

Recording pressures and RGA scans weekly with HV1600-10 activated at EY. H2 reduction is most significant change.

PT-428 = 1.62e-7 Torr (NEG housing hot cathode gauge)

PT-410 = 1.21e-7 Torr (BSC 10 main volume cold cathode gauge)

 

Images attached to this report
Non-image files attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 17:38, Monday 14 May 2018 (41979)

Scan from 4/26, two weeks prior.

Non-image files attached to this comment
H1 PEM (PEM)
marc.pirello@LIGO.ORG - posted 16:37, Monday 14 May 2018 - last comment - 11:57, Tuesday 15 May 2018(41977)
FIBOX issues at vault and MID X

In an effort to complete work at the vault and vault power room prior to the dry season we have been pushing hard to get the readbacks for the Seismic and LEMI channels in the vault operational.  Many issues impede this work, including but not limited to bugs, mice and their biproducts, bees, goat heads, snakes, dirt, weather, spotty communication to the control room, etc...  Currently the seismic reset resides inside of a bees nest.

The FIBOX is a system that can read in an audio signal (seismic and magnetic LEMI signals) and transmit them via multi mode fiber over long distances.  Our system has three Seismic channels, X, Y, and Z, and two LEMI channels X and Y.

Over the past week we have tried resetting the FIBOX's, replacing them with freshly calibrated units, we carried everything back to the lab and tested it, carried everything to MID X and tested the throughput.  After testing the FIBOX's at MID X with a local fiber, I can report that all of the channels are working as designed in this controlled environment.  The ADC inputs also work when a signal is injected into them.

When the FIBOX's are placed in the vault the seismic channels look bad, I assume it is because we cannot reset the seismic system (reset located in bees nest).  The LEMI signals also look bad.  Next step will be to read the signals directly with an oscilloscope and inject signals directly with a function generator out in the vault.

Everything is reconnected in the vault as of 3:00pm PDT.

Comments related to this report
jeff.jones@LIGO.ORG - 11:57, Tuesday 15 May 2018 (41993)
Bubba is aware of and working on a resolution to the bees. 
LHO General
thomas.shaffer@LIGO.ORG - posted 16:01, Monday 14 May 2018 (41976)
Ops Day Shift Summary

TITLE: 05/14 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: Work today including: ISC team in HAM6 investigating AS_C and viewports, EX PCAL checks, ETMX prep for AMDs later in the week, PEM PSL testing. 
LOG: See attached

 

Non-image files attached to this report
H1 SEI
hugh.radkins@LIGO.ORG - posted 14:26, Monday 14 May 2018 (41974)
WHAM4 HEPI Unlocked

HAM4 HEPI is unlocked and the Chamber went to fully isolated with out issue.

Ran Range of Motion tests of 600 micro units on X Y & RX RY.  See attached for the local sensor response:  First is the X & Y.  On this one I've taken the absolute to show the over lap better.  Can't really explain why they don't overlap on the smaller X drive excursions when it can do the larger Y.  This would appear to not be an interference issue but must be some force problem.  Again, can't explain at this point.  The second plot shows the tilting offsets  and suggests the vertical motion of the greater RY excursion starts to run into something, note: I dod not take the absolute value this time.  I'll look into the details to see if it guides me to a particular spot.  Meanwhile, there is plenty of range available for operation.

Images attached to this report
H1 PSL
jeffrey.bartlett@LIGO.ORG - posted 14:05, Monday 14 May 2018 - last comment - 15:29, Monday 14 May 2018(41973)
Add 100ml to Crystal Chiller
   Added 100ml cooling water to PSL crystal chiller. Did not add any water to diode chiller. Both filters are clean and clean. No noted debris or discoloration. 
Comments related to this report
jeffrey.bartlett@LIGO.ORG - 15:29, Monday 14 May 2018 (41975)
  Should read "Both filters are clean and clear" 
H1 TCS
alexei.ciobanu@LIGO.ORG - posted 12:03, Monday 14 May 2018 - last comment - 10:48, Tuesday 15 May 2018(41969)
Measurements of single-bounce OMC mismatch due to SR3 heater

Alexei, TVo

Ran a measurement OMC mismatch from of single-bounce beam (off of ITMX) as a function of SR3 heater temperature.

The power to the SR3 heater was gradually ramped from 0 W to 5 W (corresponding to a temperature range of 25 C to 70 C) over the course of several hours to account for the SR3 time constant (about 15 minutes according to G1501373)

The OMC was scanned by applying a sawtooth ramp voltage to PZT2_EXC with a period of 20 seconds and amplitude of [0,120] counts.
There were also some OMC alignment loops that were closed during the scan (AS_A, and AS_B?) (I'm sure TVo will correct me if I'm wrong).

The mismatch was computed by measuring the ratio of the second order peak to the zeroth order peak. The mismatch data was taken by an OMC scan analyzer tool that I've been developing, which tries to track the zerorth and second order peaks
in time by essentially plotting the PZT2_EXC channel against the AS_DCPD channel. I will upload the tool on gitlab and pypi hopefully sometime soon when it can be used without needing me to watch over it.

The final plot ( m_vs_temp_1_2.png ) is the summary of the measurement, which is a combination of two sets taken about an hour apart. The mean mismatch managed to drop by about a 1% over a 40 C change, with a fluctuation of about 1% for any given temperature. I'm not really sure why the mismatch data is so noisy (I confirmed that the tool was correctly tracking the heights of the peaks). I was also unsure what temperature load the SR3 heater could sustain ( G1501373 says that either 10 W (emitted?) or 87 C is the max).

I will investigate the single-bounce models of the IFO to see if the mismatch change is what we expect.

Images attached to this report
Comments related to this report
alexei.ciobanu@LIGO.ORG - 10:48, Tuesday 15 May 2018 (41987)

Just finished crunching the single bounce model of the SR3 actuator. Plot attached.

Plot was generated from the LHO FINESSE model with the most up to date measured parameters (found here).
The OMC eigenmode of this model was computed then back-propagated to the SRM AR surface.
A sample of beam parameters that are mismatched to the OMC eigenmode by 10% (i.e points that lie on the 10% contour in the plot) were generated following the method in T1800193.
Each beam parameter was then back-propagated to the BS.
The SR3 RoC change was varied between 0 mm and 32 mm and the beams were forward-propagated through the changed SR3 all the way back to the SRM AR surface.

All of the resulting beam parameters from this procedure are shown on the plot.

I've also plotted the most recent measurement I could find on alog of the single bounce beam parameter.

From the plots on the post that I originally posted we can see that the mismatch imporves by about 1% over roughly a full SR3 actuation range. This combined with the information that our initial mismatch is about 10% puts us somewhere in the lower right corner on this plot.

My guess is that the observed astigmatism in the single bounce beam probably makes SR3 heater actuate on the mode differently to what I've modeled. I might look into performing the same analysis but factoring in astigmatism, but right now I don't know how to carry that out. Adding another degree of freedom (the other transverse axis) makes this difficult to conceptualize as a plot.

Images attached to this comment
alexei.ciobanu@LIGO.ORG - 10:48, Tuesday 15 May 2018 (41992)

I've been asked to provide the code for the actuation maps. The notebook for generating the SR3 actuation map is on ligo gitlab linked here.

The only real dependency for this code should be the latest commit of pykat (15/05/18 or later). Let me know if this doesn't work, doesn't make sense, or is somehow wrong.

H1 PSL
edmond.merilh@LIGO.ORG - posted 09:15, Monday 14 May 2018 (41966)
PSL Weekly Report - 10 Day Trends FAMIS #6200
Images attached to this report
LHO General
thomas.shaffer@LIGO.ORG - posted 09:13, Monday 14 May 2018 (41967)
Morning Meeting Minutes

ISC

    - Beam to HAM6, AS AIR check, AS_C, and lock DRMI

    - SRM AWC testing on going. SR3 heater measurements happened over the weekend

PSL

    - "Wrap up" this week

SUS

    - Zero ITM OpLevs and run ITM TFs

VAC

    - MY work continues

    - Ion pump installs not till next week

EX

    - TMS and ETMX work continues

    - AMD install end of the week

    - PCAL baffle install this week

Other

    - HAM6 Door will be coming off this week

    - Access control work will be in LSB today

Tuesday Maintenance

    - RF balun investigation

H1 PSL
thomas.shaffer@LIGO.ORG - posted 08:12, Monday 14 May 2018 (41965)
PSL Weekly Report

FAMIS7490


Laser Status:
SysStat is good
Front End Power is -0.003303W (should be around 30 W)
HPO Output Power is 0.7854W
Front End Watch is GREEN
HPO Watch is RED

PMC:
It has been locked 3 days, 15 hr 28 minutes (should be days/weeks)
Reflected power = 16.46Watts
Transmitted power = 51.93Watts
PowerSum = 68.39Watts.

FSS:
It has been locked for 3 days 15 hr and 28 min (should be days/weeks)
TPD[V] = 1.073V (min 0.9V)

ISS:
The diffracted power is around 1.8% (should be 3-5%)
Last saturation event was 3 days 15 hours and 28 minutes ago (should be days/weeks)

Possible Issues:
Front End Power is Low
ISS diffracted power is Low
LRA out of range, see SYSSTAT.adl

 


 

This script definitely needs to be updated. I will talk to the PSL crew.

H1 AWC
daniel.brown@LIGO.ORG - posted 16:30, Saturday 12 May 2018 - last comment - 10:23, Thursday 31 May 2018(41964)
SRM heater at HAM5

Thomas, Dan Brown

This morning we wheeled out the SRM heater to the north side of HAM5. The CO2 laser cannot be switched on currently until the SOP is complete, the controller for the CO2 is on Thomas' desk. The goal today was to try and align the table to the two steering mirrors and the holes in the SRM baffle. We managed to center on the ZnSe viewport and the first steering mirror. Changing pitch and yaw there we could trace the beam around the edge of the first baffle hole, we were unable to do the same on the output baffle hole. When we believed we were centered correctly the alignment beam could be clearly seen on the baffle on the HR side of the SRM, we're currently unsure whether that should be the case or not. We also do not have a good view of the beam dump from the north side which makes trying to align into it difficult. We still have some alignment work to do here before we are ready.

The north HAM5 door area is now sectioned off with screens between the squeezer table and the clean room, pictures of the area are attached. 

 

Images attached to this report
Comments related to this report
corey.austin@LIGO.ORG - 19:20, Monday 14 May 2018 (41984)

Eddie, Corey

Eddie exported the AWC mirrors and beam dump from the SolidWorks model so that I could add them to the Zemax model. The attached .pdf shows the path of the CO2 beam into HAM5.

Aidan confirmed that most of the power will be absorbed by the optic, so only the beam labeld 'AR Reflection' will be present with the actual CO2 beam. I included the other beams (transmitted, HR reflection) in the model since the alignment laser is not absorbed, and thought it may aid with alignment.

Non-image files attached to this comment
stephen.appert@LIGO.ORG - 09:43, Wednesday 16 May 2018 (42011)

Betsy and Jason conducted the initial alignment as documented in:

LHO aLOG 39669 https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=39669

Is there any reason that this successful initial alignment would not be easily recaptured? Seems that there should be enough adjustment possible to sort this out.

daniel.brown@LIGO.ORG - 10:23, Thursday 31 May 2018 (42261)

Not really any major issues. It's just awkward to check the alignment using the reflections on the SRM baffles: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=41724. We asked Corey to check where we should see spots on the SRM HR baffle so we had a better idea of what we were looking at.

We managed to get the CO2 beam on the SRM and induce a lens using this method yesterday: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=42254

H1 AWC
daniel.brown@LIGO.ORG - posted 12:35, Saturday 12 May 2018 (41963)
SRM heater beam shape

Alexei, Dan Brown

We did some beam profiling measurements of the SRM heater to determine how far away the table should be positioned from the ZnSe viewport and if the beam sizes are correct. To take beam profiles of the CO2 we used a knife edge and a power meter. The measurements were compared to a simple model of the setup which matches up well. The aim was to get around a 5mm radius at the SRM, which we can achieve if we position the table so the top of the periscope is about 1m from viewport.

Measurements and analysis can be found in:

https://git.ligo.org/IFOsim/Finesse_playground/blob/master/daniel_brown/LHO/CO2_knife_edge.ipynb

Images attached to this report
H1 ISC (AWC, ISC)
thomas.vo@LIGO.ORG - posted 16:54, Friday 11 May 2018 - last comment - 17:30, Tuesday 15 May 2018(41962)
AS DC Centering and OMC ASC Loops closed, AS_C missing

Daniel, Jenne, Fil, TVo

In preparation for this weekend's work to try to do an OMC Scan measurement while varying SR3 RoC, I decided to try to make sure our new alignment of the IMC could make it down to HAM6.  I was able to get light on AS_A_DC and AS_B_DC and close the centering loops but I noticed that AS_C had no light on it which is very odd.  

All the electronics were turned back on from our grounding loop searching from April 26-27 however, the attached trend shows that something dramatic happened to that QPD segments around Apr 27 2018 15:53:41 PDT which caused the individual segments to get much noisier and the sum to drop dramatically.  I'm pretty sure we were laser safe at the time so it wasn't like the a beam falling off the diode. So I thought this might be some sort of electronics problem like a disconnected cable in the midst of the madness, but everything in the rack to the chamber feed-through seemed to be connected properly, Fil and Daniel tested the in vacuum QPD chain from the outside with a multi-meter and confirmed that there is a connected diode in chamber.

So maybe we're just not seeing light? Again, this seems strange because we see light on both AS_A and AS_B.

In general, this won't deter our work this weekend but we might want to get this figured out before we open the doors early next week or put it on the task list for the chamber.  One method we haven't tried is looking for AS_AIR and seeing if that comes out of the viewport. Also, there is a picomotor we can actuate to steer the beam onto AS_C, but I'm holding off on this unless we know what is going on.

 

Comments related to this report
daniel.sigg@LIGO.ORG - 10:34, Monday 14 May 2018 (41968)

Made a quick check that the downstream electronics works:

  • Inserted a DB25 breakout board and made sure the 3V bias is present on all segments,
  • Disconnected the QPD and added a 100kOhm resistor between anode and cathode. Check that there is a 0.1 offset at the output of each segment.
daniel.brown@LIGO.ORG - 10:57, Monday 14 May 2018 (41971)

Thomas, Dan

We checked the AS air and OMC transmission beams coming out of the north HAM6 viewports. They were too dim to see with cards but visible with the IR viewer, both are clearing the viewports fine

jenne.driggers@LIGO.ORG - 20:09, Monday 14 May 2018 (41985)

After more looking in the viewport with Keita, Daniel and TVo (including turning the illuminator on/off, and sadly seeing no response on AS_C, although we did see a tiny response on the OMC QPDs which are inside the shroud), I worked on picomotoring the AS_C steering mirror, in a last-ditch effort to see if we could ever see a signal.  The answer so far is no.  Using the largest picomotor steps, I went +/- 6 steps in pitch and +/- 10 steps in yaw from the previous nominal.  I thought I saw a beam briefly, but it turned out to be something upstream, since it affected all of the AS diodes (including the WFS, which aren't affected by this steering mirror).  I did a rough raster scan of the picomotor actuation, mapping out a rectangle.  When I was finished, I put the picomotor back to the place that I started, so even though it won't have gone precisely to the old pointing, it should be close. 

AS_C seems to have a lot of 60 Hz + harmonics noise, more so than the OMC QPDs do, when the IMC is offline (MC2 misaligned).  Daniel points out that this shouldn't affect our ability to see a DC response, and the rest of the electronics chain passed some basic checks, but it does seem like a concern. 

jenne.driggers@LIGO.ORG - 12:56, Tuesday 15 May 2018 (41995)

Daniel pointed out to me that the picomotor to HAM6 likely wasn't connected since ISCT6 isn't really back in it's final position yet.  And, he was right.  So, today I connected the HAM6 picomotor controller using some 10' DB25 extension cables, and then re-did my raster of the AS_C pico.  Step size of "magnum", 10 x 10 grid.  I didn't see anything at all that looked promising.  The picomotor is back nominally where I started, although it's of course not precise. I think we're going to have to pull the north door of HAM6 tomorrow, as we discussed was a possibility at this morning's meeting.

koji.arai@LIGO.ORG - 17:30, Tuesday 15 May 2018 (42008)

In case you find a problem with the QPD diode, the head, or the invac cable:

The cable currently installed for AS_C is D1101654 / S1202409 (40"). It has only one head (Head #29). The diode installed is Q3000 InGaAs QPD #18.
cf. LHO ALOG 12244

There is only one spare InGaAs QPD diode (#15) left as an LHO spare.
The spare 40" cable is D1101654 / S1301546. This cable has no head. Therefore, to use this cable, the head needs to be transplanted from S1202409 or D1000231 S1202412 (36"), which has two heads (#34 and #35) and two diodes (#55 and #76) attached.

See also: E1101174

 

H1 SEI
hugh.radkins@LIGO.ORG - posted 16:53, Friday 11 May 2018 - last comment - 15:59, Tuesday 15 May 2018(41961)
ETMY HEPI Y to RZ Decoupling

The two attached plots show before and after adding the final HEPI Y to RZ Cross Coupling factor.

This was first looked in alog 40106, 40117, & 40150 for ETMX.  I want to look at ETMX again as that was before I looked at the geometric consideration I posted earlier in 41955.

I feel pretty good about the solution here though now.

The optical lever out put during the HEPI length stroke is the sum of actual optic yaw plus the expected apparent yaw due to the OpLev Length to Yaw Cross Coupling: OLOutput = Actual + Expected.

So I want to minimize the Actual = Output - Expected.  Assume in this case the Actual is all caused by the HEPI Cross Coupling.  See the 40106 alog for the conversions and such to get the units, and the amplitudes of the OpLev Cross Coupling factors are from E1200836.  The signs of these corrections are subject to geometric analysis.

Anyway, with a CC factor for HEPI Y to RZ of 0.0065 in H1:HPI-ETMY_IPSALIGN_3_2 of the IPS Alignment Matrix, the residual is pretty much zero'd out as seen in the 2nd plot although I might be able to tweak it a little bit more.

This length drive on the ETMY HEPI is 0.8mm so a huge drive wrt anything we'd ever need to drive but why not get rid of it.

Images attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 10:52, Monday 14 May 2018 (41970)

Re; "I want to look at ETMX again as that was before I looked at the geometric consideration I posted earlier in 41955."  I've looked at that again in light of the geometry and conclude my result is valid for ETMX.  The bottom line for this exercise is that the OpLev Length to Angle CC factor is Positive for ETMX (hence my correctness) and it is negative for ETMY.  This is because the PD is on the opposite side of the beam tube and the beam is displaced in the opposite direction with a positive path length change.  Thank you for your support.

hugh.radkins@LIGO.ORG - 15:59, Tuesday 15 May 2018 (42002)

Went ahead and did the ETMY X to RZ HEPI diagonalization.  A value of -.0064 for H1:HPI-ETMY_IPSALIGN_3_1 does a thorough job of minimizing the cross-coupling.  This has been accepted into SDF.

LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 16:25, Friday 11 May 2018 (41960)
XBM Purge Air Butterfly Valve Replaced

The butterfly valve for the purge air on the X beam manifold was missing its stop pin, allowing it to turn freely (more than a 1/4 of a turn), removed it and replace it with a spare on hand.

Upon further inspection of the bad valve we found the rolled pin was sheared off, also noted one of the two screws missing that fasten the disc to the stem, I was not able to locate the missing screw.

Images attached to this report
H1 General
jeffrey.bartlett@LIGO.ORG - posted 16:04, Friday 11 May 2018 (41959)
Ops Day Shift Summary
Ops Shift Log: 05/11/2018, Day Shift 15:00 – 23:00 (08:00 - 16:00) Time - UTC (PT)
State of H1: Unlocked for upgrades
Intent Bit: Engineering
Support: X
Incoming Operator: X
Shift Summary: Vent closeout activities.  
 
Activity Log: Time - UTC (PT)
14:55 (07:55) Chris – Going into the LVEA to recover some rigging
15:00 (08:00) Start of shift
15:10 (08:10) Chris – Out of the LVEA
15:17 (08:17) APS on site – Working at the staging building
15:27 (08:27) APS on site – Working at the staging building
15:24 (08:24) Filiberto – In MSR working on access control system
16:19 (09:19) Filiberto – Going to End-Y to work on access controls
16:23 (09:23) Richard – Working on E-Stop for Diode room
16:23 (09:23) Dan & Alexei – Going to Squeezer Bay
16:30 (09:30) Filiberto – Transition End-Y to laser hazard
16:52 (09:52) Corey, Keita, & Travis – Going to End-X to work on TMS yaw
16:56 (09:56) Greg – Going into LVEA to work on TCS laser alignment
17:18 (10:18) Dave – Going to Mid-Y to restart computer
17:35 (10:35) Filiberto – Back from End-Y
17:36 (10:36) Dan & Alexei – Out of the Squeezer Bay
17:39 (10:39) Dave – Back from Mid-Y
17:40 (10:40) TVo & Filiberto – Into the LVEA turn on high voltage for HAM fast shutter (WP #7551)
17:44 (10:44) TVo - Out of LVEA
17:45 (10:45) Filiberto – Working on access controls in PSL closet
17:55 (10:55) Chris – Returning rigging to LVEA
17:55 (10:55) Apollo crew – Going to Mid-Y to clean up
18:02 (11:02) Chris – Finished in LVEA – going to Mid-Y
18:28 (11:28) TJ – Restarting the Guardian ISI sensor correction nodes
18:46 (11:46) Keita, Corey, & Travis – Back from End-X
20:30 (13:30) Marc & Filiberto – Going to the vault
20:31 (13:31) Daniel – Going to End-Y to work on ALS laser
20:37 (13:37) Fred – Taking a tour through the LVEA
20:44 (13:44) Daniel & Alexei – Going into the Squeezer Bay
21:06 (14:06) Corey – Bringing panels into the LVEA – May use roll up door
21:13 (14:13) TVo – Going into the HAM6 rack
21:15 (14:15) Daniel – Back from End-Y
21:25 (14:25) Fred – Tour out of the LVEA
21:26 (14:26) Corey – Out of the LVEA
21:17 (14:17) APS – Back on Site
23:00 (16:00) End of shift

 

H1 AOS (AOS, ISC, SUS)
keita.kawabe@LIGO.ORG - posted 13:32, Friday 11 May 2018 - last comment - 11:04, Monday 14 May 2018(41954)
TMSX SUS rotation complete (Corey, Travis, Keita)

Betsy and Travis told us that we can just use the top blade to rotate TMS is we're talking about O(100urad) instead of O(many mrad), so we did just that.

The procedure was: Remove ERM protection cover, adjust EX bias so the optic is centered in oplev, inject green laser, set the TMSX offset to get the retro-reflection on the table. Then loosen the blade (which makes TMS sag so no retro-reflection), turn the adjustment screw, tighten the blade, look where the beam goes, repeat.

It turns out that 1/4 turn of the adjustment screw took out 400-something urad, then Travis tried 1/16 of a turn and that took out the rest.

In the end TMSX alignment sliders were set to [P,Y]=[-74,5] urad, almost perfect for Y, and P is no worse than yesterday where it was [91,-585].

We also adjusted BOSEM depth. For F1, LF and RT we recently measured the open values and set the depth (41675) so didn't bother to remeasure open values but we reset the depth anyway as RT seemed to have drifted out.

For F2, F3 and SD, old and new offset as well as open value as of now are:

  Open today New offset Old offset Reading before adjustment Reading after adjustment
LF NA NA -9350 ~9.9k ~9k
RT NA NA -13475 ~16k ~12k
F1 NA NA -10515 ~10.9k ~10.7k
F2 18.1k -9050 -11164 ~11k ~9k
F3 23.2k -11600 -14150 ~18.5k ~11.3k
SD 22.1k -11050 -14372 ~11k ~11.5k

 

Inventory info: S/N of F3 BOSEM is 296, F2 301.

Comments related to this report
betsy.weaver@LIGO.ORG - 14:09, Friday 11 May 2018 (41957)

Travis and I have taken the 6 DOF transfer function measurements of TMSX.  While nothing says it is rubbing (good), there still seems to be something wrong with the top 2 BOSEMs (LF and RT), see attached.  The TFs that utilize these 2 BOSEMs show a DC offset across the entire measurment.

Will continue forensics later.  Maybe a setting somewhere?  TBC...

Images attached to this comment
Non-image files attached to this comment
keita.kawabe@LIGO.ORG - 11:04, Monday 14 May 2018 (41972)

The changes in the TF look predominantly just a factor of 4-ish increase in sensitivity, and it makes sense to me.

We know that BOSEM LF and RT sensitivity was much smaller before I and Corey repositioned/replaced these on Apr/25. If you look at my alog and Jeff's comment attached (41675),  their physical sensitivity increased by a factor of 2.8 and 3.3 respectively for LF and RT, then Jeff changed the calibration constant for LF from 1.295 to 1.604 (a factor of 1.24) and for RT from 1.146 to 1.113 (a factor of 0.97).

The overall sensitivity of LF and RT increased by 2.8*1.24=3.5 and .97*3.3=3.2, respectively, i.e. roughly the P and V sensitivity should have increased by a factor of ~(3.2+3.5)/2~3.4. And 4/3.4~1.2, that's not a big number.

I assume that the reference in Betsy's plot was taken when the sensitivity was already small.

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