Displaying reports 70361-70380 of 85418.Go to page Start 3515 3516 3517 3518 3519 3520 3521 3522 3523 End
Reports until 08:01, Saturday 06 December 2014
H1 COC (COC)
richard.savage@LIGO.ORG - posted 08:01, Saturday 06 December 2014 - last comment - 17:38, Monday 15 December 2014(15479)
ETM high-resolution images with Green and IR light resonating
SudarshanK, TravisS, EvanH, AlexaS, RickS

Using the Pcal beam localization cameras at both end stations, we took images of the ETM surfaces under three conditions: IR and Green resonating; IR only resonating, and Green only resonating.

Attached below are two composite images composed of four separate images taken with the same camera settings:
Upper Left: Xarm Green
Lower Left: Xarm IR
Upper Right: Yarm Green
Lower Right: Yarm IR

The images in the first composite were taken with the following camera settings: F8, ISO 200, 30 second exposure, WB-cloudy.

For the second composite image the aperture was F29 (~13 times less light)

The Yend camera was re-focused for the IR-only images, but the Xend camera was not re-focused.
Images attached to this report
Comments related to this report
richard.savage@LIGO.ORG - 21:51, Monday 08 December 2014 (15502)
Thomas Abbott at LLO applied the Pcal beam localization analysis the the LHO ETMY image to calculate the position of the center of the optic in the image from last Friday.

The image below contains lines that indicate the center of the optic using the Pcal image analysis.
Images attached to this comment
betsy.weaver@LIGO.ORG - 12:19, Wednesday 10 December 2014 (15536)

Attached is a picture of the original FirstContact (FC) sheet, circa ~Jan 2014, showing the "IAS window" which is a thinner film of FC in the central 3" of the larger sheet.  To me, the shape of the FC window looks similar to the 3" ring showing up in green on the recent optic photo above.  SYS is working with us to get our cleaning game plan together in order to remove the ring.  As well, they are investigating other possible scenarios of where the ring came from if not the window.  Note, there was a full FC sheet re-cleaning in March that apparently did not remove all of the ring that was left behind apon the removal of the first sheet.  To be continued...

Images attached to this comment
dennis.coyne@LIGO.ORG - 17:38, Monday 15 December 2014 (15631)COC, SYS
I've attached an overlay of (a) the SolidWorks CAD view of ETMy along the PCal camera path and (b) the PCal camera image of H1 ETMy (scaled and rotated). Since SolidWorks does not diffract the image viewed through the ETM optic, I indicate the shift in the ETM Telescope Baffle aperture as well. Three of the 4 bright areas are along the ETM Telescope Input aperture/baffle edge (a coincidence?). (The upper one is red.) One of the 4 bright spots does not correspond to any feature in the CAD image and is likely a spot of residual First Contact.
As subsequently shown by the zoomed in PCal image using the Green Lantern flashlight (green LED) after venting (see entry #15635), it is simply a coincidence that the two prominent bright areas appeared to be along the ETM Telescope baffle aperture edge.
Non-image files attached to this comment
H1 COC (COC, ISC)
evan.hall@LIGO.ORG - posted 18:20, Friday 05 December 2014 - last comment - 15:29, Monday 08 December 2014(15476)
ETMY loss scan

Dave, Alexa, Evan

Summary

We’ve now completed a scan of the equivalent ETMY loss as a function of spot position on the Y optics.

  • We locked the Y arm in IR.
  • We turned on the REFL WFS loops in which actuate on IM4 and PR2. This keeps the pointing into the Y arm maximized.
  • Then, using a spiral pattern, we adjusted the pitch and yaw of ETMY and ITMY in such a way so as to move the spot on ETMY (but not in ITMY). The total amount of excursion was about 4 urad in each direction.
  • For each position, we let the configuration settle for 60 s (to let the WFSs catch up), and then recorded the counts on ASAIR using a 5 s cdsutils.avg.
  • Afterward, we unlocked the arm and then recorded the power on ASAIR; it equals 1351(15) ct.
  • With the above information, we can infer the total loss via the formulas in LHO#15470, again ignoring mode-matching.

Loss vs. alignment is given in the attached plot. The attached zip contains the data and the code used to perform the measurement. The measurement uncertainty is about 45 ppm, and comes from the uncertainty in the number of ASAIR counts with the cavity unlocked. Note that this plot is equivalent ETMY loss; i.e., all the observed loss (including power in the rf sidebands and mode-mismatched light) is assigned to the ETM.

Details

  • In order to move the spot on only the ETM, we scaled the angle steps θE and θI so that θE = θI × (4 km − ROCE) / ROCE, where ROCE = 2.24 km.
  • For pitch, we stepped the ETM and the ITM with the same sign. For yaw, we stepped them with opposite signs. We think this gives the required soft-mode angular motion in pitch and yaw.
  • As for the convention in the plot for the displacement on the face of the ETM: the displacement is found by multiplying the ITM angle by the cavity length. When we push positive in ITM yaw, we simultaneously push negative in ETM yaw. This pushes the cavity mode toward the left when looking at the ETM face-on. When we push positive on the ITM and ETM in pitch, this tilts the optics forward (the tops of each optic approach each other, and the bottoms recede), and thereby pushes the cavity mode downward.
Non-image files attached to this report
Comments related to this report
evan.hall@LIGO.ORG - 19:53, Friday 05 December 2014 (15478)

We are repeating the measurement for the ITM. Then the script will try to get a bigger spiral on the ETM.

Please do not unlock the Y arm for the next 200 minutes.

evan.hall@LIGO.ORG - 23:29, Sunday 07 December 2014 (15484)

I’ve attached the results of Friday night’s ITM scan data (first attachment). The arm unlocked shortly into the ETM scan, so there is no data there. Note that the axes indicate the ITMY spot position, but the quantity plotted is the equivalent ETMY loss (for the sake of consistency with the previous measurement).

First, the data indicate that the spiral is centered around an especially lossy spot for the arm. Second, it seems that sweeping the spot on the ITM can change the measured arm loss by several hundred ppm. That magnitude seems comparable to the effect of sweeping the spot on the ETM, as we measured on Friday. There are several possible things we might conclude from this:

  • The ITMY coating also has anisotropic loss.

  • Moving the spot on ITMY is causing clipping somewhere (e.g., the edge of the optic).

  • The scan strategy is also moving the spot on ETMY. Since the ROCs of the ETM and ITM are similar (2.2 km and 1.9 km, respectively), we require the alignment sliders to be calibrated to better than 7 % of each other in order for this to work [since (4 km - ROC_I) / ROC_I = 1.07].

  • The unlocked value of ASAIR is changing with alignment.

To test the last of these, I locked the Y arm, turned on the WFS loops, and looked at the locked vs. unlocked values of ASAIR for several different arm alignments (separated from each other by 2 urad in pitch/yaw). I first measured ASAIR while locked. Then I held the outputs of the WFS loops, unlocked the arm, and measured the ASAIR value again. I found consistently that the unlocked value was 1370(15) ct. So it seems this is not the issue.

To test the idea that the spot location on ITMY is causing clipping, I adjusted the arm alignment to give lower loss. I ran the ITM sweep again (second attachment). Here the overall loss values are much lower (as low as 550 ppm), but again we find a variation of 100 ppm or so.

Non-image files attached to this comment
daniel.sigg@LIGO.ORG - 07:15, Monday 08 December 2014 (15485)

The limiting aperture for an ITM scan is probably the BS baffle. Not sure we can (yet) conclude that these losses come from the ITMY.

paul.fulda@LIGO.ORG - 15:29, Monday 08 December 2014 (15493)

Here are the expected clipping losses as a function of offset from the mirror center. This assumes a 62mm radius beam on a 326mm radius optic coating. The pdf shows the clipping loss as a function of offset, and the other attachment is an animation showing the intensity spilled over the edge as the offset is increased (since gifs are all the rage these days).

Images attached to this comment
Non-image files attached to this comment
H1 PEM (PEM)
dale.ingram@LIGO.ORG - posted 16:16, Friday 05 December 2014 (15475)
Friday seismic forecast
Hanford hauling has been running on day shift today (12/5) and they will operate on swing shift tonight also.  We've received no indication that they'll do weekend work.
H1 General
jeffrey.bartlett@LIGO.ORG - posted 16:07, Friday 05 December 2014 (15474)
Ops Day Shift Summary
LVEA: Laser Hazard
Observation Bit: Commissioning  

07:15 Karen & Cris – Cleaning in the LVEA
09:00 Tweaked the ISS Reference Signal voltage to raise Diffracted Power up to 7.5% 
09:00 Peter – Working in the Diode Room
09:00 Travis & Sudarshan – Going to End-Y to work on PCal cameras
09:19 Andres – Working in the 3IFO Storage Container cleanroom & looking for TCS parts
09:28 Filiberto & Aaron – Cabling work in the HAM3 area
09:43 Mitch – Going into the LVEA to work on Elliptical baffle
10:11 Rick S. – Going to End-Y
10:20 Dave – Going to End-Y to work on camera
10:35 Mitch – Out of LVEA
10:37 Karen – Going to End-Y for cleaning
10:57 Dave – Back from End-Y
11:00 Kyle – Going to End-Y
11:01 Travis – Going to End-X
11:07 Platt Electric on site to deliver electrical parts. Richard will escort
11:00 Turn off sensor correction while Travis is at End-X
11:14 Sudarshan – Back from End-Y
11:20 Kyle – Back from End-Y
11:45 Andres – Out of LVEA
11:48 Gerardo – Turn on cleanroom fans at HAM1/2 
11:51 Rick, Travis, & Sudarshan – At End-Y installing camera 
12:12 Filiberto & Aaron – Out of the LVEA
12:30 Filiberto & Manny – Going to End-Y & End-X for PCal camera work
12:59 Aaron – Measuring power output at HAM3 area
13:28 Corey – Out of H2/Squeezer bay
13:40 Andres – Going into the LVEA looking for parts
13:40 Bubba – Going to Mids and Ends to drop off filters
14:16 Andres – Out of LVEA
14:55 Travis & Sudarshan – Going to End-X to work on PCal camera 
15:19 Rick – Going to End-Y to work on PCal cameras
LHO General
gerardo.moreno@LIGO.ORG - posted 15:31, Friday 05 December 2014 - last comment - 15:51, Friday 05 December 2014(15472)
Residue On Cleanroom Curtains

(Jeff B, Gerardo M)

Found some goop on the cleanroom curtains, yes the cleanroom over HAM1-HAM2.

The goop appears to be generated from a reaction between the glue of the tape and the vinyl of the curtain, so far the reaction does not appear to take place on "ameristat", we will look further into that.

Note: on photos attached only look at curtain content.

Images attached to this report
Comments related to this report
kyle.ryan@LIGO.ORG - 15:51, Friday 05 December 2014 (15473)
Years ago, the cleaning crew were wiping down these curtains with some sort of solvent (Acetone?) which caused similar issues.  Could this be happening again?  
LHO General
gerardo.moreno@LIGO.ORG - posted 12:06, Friday 05 December 2014 (15469)
Cleanroom over HAM1 and HAM2 is ON

(Filiberto, Gerardo)

We turned ON the cleanroom that is on top of HAM1 and HAM2, time 11:48 am.

H1 SEI
jim.warner@LIGO.ORG - posted 10:14, Friday 05 December 2014 (15464)
HAM2 HAM3 ISI Sensor correction/ STS issue

I've been trying to turn on Sensor correction at HAM2 & HAM3 on the ISI's. HAM2 works as expected, but HAM3 gets almost nothing from turning it on. So far I've look at the the input filters (HAM3 was looking at the wrong STS originally, and the cal filter had a pole and zero at 1), the Hua filters (which all look the same) the input and output spectra at various places on the STS signal path (which all look the same, that I've found) and the chambers isolation filters (which, again, look very similar). Not sure what's going on.

H1 INJ
jeffrey.bartlett@LIGO.ORG - posted 09:54, Friday 05 December 2014 (15463)
08:30 Meeting Minutes
Seismic:Installing Guardian changes for commissioning group
	Testing sensor corrections HAM2 and HAM3
CDS:	Cabling work at the HAM3 area
PCal:	Camera work at End-Y and End-X
FMP:	Trenching/road work between H2 enclosure and VPW
GC:	Monday 06:00 to 07:00 ISP outage, limited INet access. 
H1 CDS (PEM)
james.batch@LIGO.ORG - posted 09:01, Friday 05 December 2014 (15461)
Display of Seismic FOM's restored on projector0
The display of seismic FOM's on projector0 in the control room is now accurate.  This follows a change of operating systems for the dmt computers performed yesterday.  
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 08:26, Friday 05 December 2014 (15460)
CDS model and DAQ restart report, Thursday 4th December 2014

model restarts logged for Thu 04/Dec/2014
2014_12_04 17:42 h1fw0

unexpected restart of fw0. Conlog frequently changing channels list attached.

Non-image files attached to this report
H1 ISC (COC, ISC)
evan.hall@LIGO.ORG - posted 18:31, Thursday 04 December 2014 - last comment - 13:32, Friday 05 December 2014(15456)
Y arm loss measurements

 

Dave, Elli, Alexa, Evan

We are trying to decrease the observed loss in the Y arm by changing the position where the cavity mode falls on the test masses.

We have done the following things:

  • We locked the Y arm in IR.
  • We set up ASC loops which take REFL WFSs signals and actuate on IM4 and PR2. This keeps the input pointing to the arm maximized.
  • We move the alignments of ITMY and ETMY and monitor the dc signals on the TRY and ASAIR_A diodes.
  • The unlocked reflected power as seen by ASAIR is 1180. While locked, Dave has been able to increase the ASAIR signal by hand from ~960 ct to ~1020 ct by adjusting the ETMY and ITMY pointings.
  • I’ve written a python script that will adjust the test mass alignments in a spiral pattern in order to map out the cavity loss. It is currently running.

 

Please leave the Y arm locked for the next 100 minutes.

Comments related to this report
evan.hall@LIGO.ORG - 00:43, Friday 05 December 2014 (15458)

Dave, Evan

We found a sign error in the script, but it doesn’t matter because the Y arm broke lock soon after we started the script so there is no data.

We have tried to relock the Y arm, but have not been able to. Maxium buildup on the TRY PD is about 3 cts (I expect we should se flashes of 6 cts or so). We've left the Y arm test masses "aligned" as determined by their saved guardian values.

It seems there is no green light anywhere in the arm. The ALS Y camera is completely dark, the REFL PD is completely dark, and I cannot move the TMS (either by hand or with the baffle script) to put light on the ITMY baffle PDs. Perhaps there is an issue with how the green light is being launched into the TMS, but I cannot diagnose it.

evan.hall@LIGO.ORG - 01:01, Friday 05 December 2014 (15459)

Ryan called and walked me through unsticking the green QPD loops at the Y end, which had become railed.

We're leaving the rest of the work for the morning.

keita.kawabe@LIGO.ORG - 10:21, Friday 05 December 2014 (15462)

I and Alexa looked at the video image of ETMY and ITMY.

We confirmed that the green and the IR are on top of each other on ITMY when the alignment was good-ish for green and IR. There's no particularly bright spot.

We couldn't tell if the green and the IR are on top of each other on ETMY. But there are two bright spots on the ETMY camera that only appear when the arm is locked. See attached images (green was misaligned for these images so you only see IR).

The ETMY camera is looking at the ETMY from HR side. These spots could be something on the HR coating itself, or could be an image of something else (e.g. some scattering and ACB or some unknown ghost beam hitting near by structure?) reflected by the HR coating. This cannot be behind the HR coating, but it's still not impossible that these are some ghost beams from TMS structure taking strange path and coming into the camera at a large angle.

While Dave was walking the beam in PIT, the high spot became brighter or weaker but the lower spot didn't change much (the first three images).

When the beam was moved in YAW the lower spots got brighter (the 4th image).

Update:

This morning I locked green to Y arm without IR, and I can see bright spots on the same position (5th picture), so now it seems more likely that they are on the HR of the mirror.

The sixth picture is taken with green and IR both locked.

If these are on the mirror, the low spot is somewhat low and somewhat to the right  left  to the center of the HR.

Images attached to this comment
keita.kawabe@LIGO.ORG - 11:18, Friday 05 December 2014 (15466)

Update 2: Is the loss by shmutz big?

To see if the loss caused by the shmutz is significant, Alexa and I moved the beam about +-3cm in YAW on the ETMY without moving ITMY position: (ITMY, ETMY)= (-7.5, +5.88) urad in YAW moves the beam on ETMX to the right, flip the sign to move to the left.

We saw an improvement in both of the cases but it was better when we moved to the left. This is probably because the shmutz is to the right to the center of the mirror.

Alexa will post the StripTools plot, Dave is working on the loss number.

In the attached picure, the first one is when the beam was moved to the right, the next one is when it was moved to the left. Ignore the bright thing at the center of the shmutz as that's just green, look at the halo, and you can see that the IR is indeed dimmer than the last picture from my previous entry.

Images attached to this comment
alexan.staley@LIGO.ORG - 10:09, Friday 05 December 2014 (15465)

Keita and I had intentionally misaligned the green PZTs to examine the ETMY and ITMY camera with only the IR beam, and we never realigned it. This is why Evan found the EY green QPDs railed.

Also I found that one of the two IR input pointing WFS had not been cleared, which also explains why the IR beam was not flashing in the cavity.

alexan.staley@LIGO.ORG - 11:34, Friday 05 December 2014 (15467)
  ITMY YAW ITMY PITCH ETMY YAW ETMY PITCH ASAIR
Original -152.9 209.5 -58.7 93.93 1068 cnts
Right 3cm -160.4 209.5 -52.82 93.3 1117 cnts
Left 3 cm -145.4 209.5 -64.58 93.3 1129 cnts

The above tables lists the positions and the counts on ASAIR. When the IR is not resonanting in the arm, ASAIR reads about 1360 cnts.

 

In the StripTool I have shown ASAIR_LF_OUTPUT which we are using to measure the power loss, and LSC-Y_TR_A_LF_OUT which measures the IR transmitted power.

At -75 min the IR is flashing in the arm cavity, and ASAIR is about 1360 cnts. Shortly after the IR locks, and then the input pointing WFS engage, as seen by the power build up in IR.

At -70 min we have full IR buildup (TR is about 11 counts), meanwhile ASAIR has dropped to about 1068 cnts. 

At -45 min I begin to move the beam to the right; this is completed at about -40 min. At this point the transmitted power has remained the same and ASAIR is now up to around 1117 cnts

Shortly after we lose lock, and I recover the lock.

At -30 min I begin to move to the left; this is completed at about -20min. Again the tranmistted power has stayed the same, and now ASAIR is at 1129 cnts. Eventually we lose lock again.

Images attached to this comment
keita.kawabe@LIGO.ORG - 11:53, Friday 05 December 2014 (15468)

Mirror cage outline and guesstimated mirror center line.

Note that we are looking the mirror from the left at a big-ish angle.

Blue lines are inner edges of the cage.

Images attached to this comment
evan.hall@LIGO.ORG - 12:14, Friday 05 December 2014 (15470)

Using the ASAIR data in LHO#15467, the loss 850 ppm for original, 690 ppm for left 3 cm, and 655 ppm for right 3 cm, again ignoring mode-matching issues.
The formula I’m using is as follows:
[ 1 - L_E = left[frac{A - r_I}{A r_I - 1} 
ight]^2,]
where A = sqrt{P_{
m{ASAIR}}^{
m{on res}} / P_{
m{ASAIR}}^{
m{off res}}}, and r^2 = 1 - 0.014.

keita.kawabe@LIGO.ORG - 13:32, Friday 05 December 2014 (15471)

Rick sent us this picture of Pcal camera. We can clearly see bright spots, which I assume is caused by the IR.

Note that pcal camera is looking at the optic from the right.

Images attached to this comment
H1 ISC
evan.hall@LIGO.ORG - posted 22:51, Wednesday 03 December 2014 - last comment - 19:19, Friday 05 December 2014(15432)
Y arm lossy ?

Dave O. Elli, Daniel, Kiwamu,

We briefly checked how lossy our arm cavities are by locking the individual arm without recycling.

For the X arm:

ASAIR_A_LF = 1180 cnts when unlocked.

ASAIR_A_LF = 1155 cnts when locked.

 

For the Y arm:

ASAIR_A_LF = 1180 cnts when unlocked.

ASAIR_A_LF = 970 cnts when locked.

 

We made a corase estimation of intra cavity loss (or a.k.a round trip loss) for the y arm, which is estimated to be about 750 ppm (!). In the calculation, we did not take a mode-mismatch or RF sidebands into accout. We need a closer look at this arm cavity to see why it is so lossy.

Comments related to this report
paul.fulda@LIGO.ORG - 09:28, Thursday 04 December 2014 (15439)

If beam mis-centering on the TMs is the cause of all the extra loss, it will have to be quite a big mis-centering. I did a quick calculation, and to get 750ppm loss at the ETM, the beam has to be offset from the center by about 6cm (roughly one beam size). The attached plots show the intensity spill over for a 62mm radius beam on a 163mm radius coating, with no offset and with a 6cm offset. The proportions of beam power outside the coating, with no offset and 6cm offset, are 0.991ppm and 762ppm respectively.

Non-image files attached to this comment
alexan.staley@LIGO.ORG - 15:38, Thursday 04 December 2014 (15448)

Just in case someone wants a plot ...

Images attached to this comment
evan.hall@LIGO.ORG - 19:19, Friday 05 December 2014 (15477)

Dave has a calculation which makes some assumptions about mode-mismatch and sideband power for the X arm.

Suppose the power in the sidebands is 6% of the incident beam, and 15% of the incident carrier doesn't enter the cavity because of mode matching issues; i.e., about 20% of the light is nonresonant. Then the equivalent power reflection is (1155 - 236) / (1180 - 236) = 0.974. This gives a loss of 108 ppm in the X arm.

Displaying reports 70361-70380 of 85418.Go to page Start 3515 3516 3517 3518 3519 3520 3521 3522 3523 End