Displaying reports 64421-64440 of 83266.Go to page Start 3218 3219 3220 3221 3222 3223 3224 3225 3226 End
Reports until 15:26, Friday 26 June 2015
H1 CDS
david.barker@LIGO.ORG - posted 15:26, Friday 26 June 2015 (19347)
FRS web page inaccessible from CDS workstations

Jeff, Dave, Jonathan, Ryan:

Jeff K noted that the FRS web service was inaccessible from LHO CDS workstations this afternoon. We raised this as FRS-3241. Jonathan H and Ryan B did some analysis on the problem and suspect it is an issue with LLO DNS when clients use  root-DNS. I opened a LLO GC fault ticket  FRS-3242 and closed out FRS-3241 Until a fix has been implemented, I have reconfigured the internal CDS DNS server to resolve the fed.ligo-la.caltech.edu address internally. This is just a short term fix.

H1 SYS (ISC, SEI)
hugh.radkins@LIGO.ORG - posted 15:21, Friday 26 June 2015 - last comment - 16:49, Friday 26 June 2015(19345)
WHAM6 Further Status Update

With purge on and both door covers open 2' outside of -Y door plane:  Dust counts all zeros!

While Matt was prepping to cut glass, Greg & I did the major rebalance of the ISI.

After Matt got the modified OMC shroud pieces reinstalled, Greg and I completed the ISI rebalance--I'll detail next.

Just before recovering the openings, -X of South Door:

100/0/100/0/200/100 counts for 0.3/0.5/0.7/1.0/2/5/ particals

Got the covers secured and free of the Optical Table with the purge turned down.  Jim made quick TFs (will log seperately) and they look fine.

Dan took over next and reports the OMC is still in good shape.

I've completed a thorough visual inspection and as-built of the new mass layout.

Thanks to GregG who spend nearly four hours in chamber.

Comments related to this report
jim.warner@LIGO.ORG - 15:25, Friday 26 June 2015 (19346)

HAM6 ISI looks healthy after a quick l2l  transfer function. See attached spectra. Resonances all look similar to last known good tf's.

Images attached to this comment
hugh.radkins@LIGO.ORG - 16:31, Friday 26 June 2015 (19350)SEI

I've added my as-built for the WHAM6 mass balance to the DCC at D1201388-v4.

hugh.radkins@LIGO.ORG - 16:49, Friday 26 June 2015 (19351)

Here are trends of the vertical CPSs indicating how well re-balanced the ISI is after the shroud install.  The trend is ~15 days and you can read the current CPS readings on the medm.  The ISI is not isolating so this is the free hanging position.  The error is less than 100 counts (a few um,) plenty close.

HEPI remains Locked

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 15:20, Friday 26 June 2015 (19344)
new tables installed in computer users room

Our new tables for the computer users room were installed today. This required the power cycling of several CDS workstations.

H1 AOS
matthew.heintze@LIGO.ORG - posted 13:10, Friday 26 June 2015 - last comment - 17:15, Friday 26 June 2015(19342)
OMC glass black shroud install complete

Matt H, Bubba G, Greg G, Jeff B, Calum T (remotely), Eddie Sanchez (remotely)

 

If you remember from yesterday with all the glass pieces of the OMC shroud in we had a cable interference with the shroud (see pic 2424).
 After playing with the cables the decision was made to pull the two interfering panels out so that the cables would hang free (see pic 2431). This however leaves the to now open and exposed (pic 2459). So after some discussion last night we decided to try to score and snap part of the black glass to stop the interference but also so that we could get the plate back in.

 

By looking side on (pic 2469) we could use the holes that the capture screws go in a s a guide to where the cables interfere with the black glass and how much glass we wanted to remove.

 

We decided to remove around 2.25 " (see plate mod pdf)...so it should hopefully look like "OMC3D" pic

 

With a brand new glass cutter we practiced on some test piece bits of black glass Calum had sent Betsy. The trick is to only do one 'score" with a light but even pressure, and then put the pressure over a raised surface (say a small diameter smooth rod), and then with gentle and even pressure that is spread out, push down and will get it to snap along the score.

 

Once happy with our technique, we went out and did it to the two real pieces. After of course the old carpenters trick of "measuring twice cutting once" :-) Worked like a charm. John W, gave us a small file (diamond tipped I think) to just gently bevel the edges a tiny bit to take off the sharp corners. That also worked really well. We then cleaned it by blowing it down with top gun, and then in area that snapped giving it a methanol rinse.

 

It went back in no problems at all. Its done.

 

Pic 2497.....before pic of one of the glass pieces to be cut

Pic 2498......after its been "modified"

Pic 2504...drying after methanol rinse. Thats the AR coated side you see

Pic 2506 & 2510.....The now complete OMC black glass shroud installed

Images attached to this report
Non-image files attached to this report
Comments related to this report
koji.arai@LIGO.ORG - 15:30, Friday 26 June 2015 (19348)

It was a nice recovery!

It seems that the picture 2506 shows that one of the bosem cables was touching these two white cables.
It's not obvious from the picture 2510. Has this rubbing been fixed between these two pictures?

daniel.hoak@LIGO.ORG - 17:15, Friday 26 June 2015 (19354)

Ahh, I meant to double-check this clearance - thanks for the reminder.  I just went back into the chamber, there was no contact between the white (PZT?) cables and the black BOSEM cable, but I fiddled with the BOSEM cable to provide more clearance.  The attached pictures aren't terribly convincing by there's more than an centimeter of room between the cables now.

Images attached to this comment
H1 General
thomas.shaffer@LIGO.ORG - posted 10:55, Friday 26 June 2015 (19341)
EY ESD power cycled reset

Leonid needed the ESD for some measurments, so Corey and I reset the EX ESD the usual way (toggle H1:ISC-EXTRA_X_BO_4, then click HI on the medm). We couldn't do this with EY since it is the newer low noise ESD, but Jeff showed showed us the SUS_CUST_QUAD_BIO.adl screen and the big reset button.

This worked, kinda, but the driver was railed negative. Richard and I went down the EY to power cycle the driver and this seemed to solve the issue.

H1 AOS
stefan.countryman@LIGO.ORG - posted 10:49, Friday 26 June 2015 (19340)
Added missing leap second to EY IRIG-B, set leap second pending on EY, EX, MSR IRIG-Bs
Dave Barker

The IRIG-B in EY only had 15 leap seconds set as of yesterday. I manually added an extra leap second at around 12:30 PST and set a pending leap second. Dave and I confirmed that all three operational IRIG-Bs have 16 current leap seconds as well as a leap second pending for June 30th.
LHO General
corey.gray@LIGO.ORG - posted 09:25, Friday 26 June 2015 (19337)
Fri Morning Detector Meeting

Morning Meeting Notes

LHO VE
john.worden@LIGO.ORG - posted 09:01, Friday 26 June 2015 (19336)
X2 Beam Tube pressure during washing

The beam tube washers are nearing completion on X2 and are currently near the X end station.

The plot shows 30 days of pt 523.

Images attached to this report
H1 AOS
matthew.heintze@LIGO.ORG - posted 22:26, Thursday 25 June 2015 (19334)
OMC black glass shroud and beam diverter move update

Daniel H, Matt H (and help at various times from Hugh, Greg G, Kiwamu, Sheila, others)

 

Todays events

So a  quick summary of todays work as too tired to write a detailed one sorry.

The in-vacuum cables were connected back onto the OMC and we confirmed we had signals etc. Also had a go at roughly moving the beam diverter to the position Keita/Dan hoped they could sqeeze it so as to not to have to move optics/SEI balance masses. We also had a look at trying to strain relieve the cables on the OMC that touch the OMC black glass shroud. But it looks like these are very touchy and altering these alter the balance.

 

Decided to analyse more with a laser beam.

 

Had troubles locking the mode cleaner. Apparently it was chased down to some whitening problem (something that last appeared around May 2014 I think I overheard). Once input mode cleaner locked and Dan had it set in a single bounce configuration,  The "M8" mirror (near the tiptilt and OMC shroud) was replaced (as was the additional black glass beam dump we had to remove for the OMC shroud install). The septum viewport protector was removed.  Dan was estatic (okay maybe he wasnt estatic but he was happy) that immediately saw signals. Looking at the OMC glass shroud and the beams though it looks like they go through very close to the center. Well done to Eddie Sanchez and the SYS team for all their hard work with the design to make sure they did.

 

We played more with the cables but in the end I decided to pull the trigger on removing the two upper black glass plates that r the cables that go to the glass bench are touching (it pained me to do so after all the hard work putting it in). Playing with the cables more we were able to get it to a point that Dan was "happy" with....(he would like it better if could but we decided we were at the point that perfection was the evil of good enough).

Note: we have it so that no offsets on the OMC like used to have

 

Then checked beam aligment out of OMC. As M8 didnt go back exaclty in the same spot, some of the optics had to be tweaked to re-establish the alignment. Also had to move a beam splitter as part of the beam diverter move. We chacked that both beam diverters still work in air. They did.

 

Also turned down purge air and did some TF's and they all passed (see attached).

 

Below is Dans much more succint summary......

 

Beam diverter was moved succesfully
90-10 BS was moved upstream of the second OMCR pico mirror; power on the QPDs has not changed (when the diverter is open)
Beam dump for 90-10 splitter was moved next to OMC SUS, should be out of the way

Alignment of OMCR path is good
Tested both beam diverters
Alignment into / out of OMC is excellent
Flashed OMC and saw the OMC TRANS beam out of the vacuum

OMC SUS TFs are good!

Purge air is on and OMC PZT HV is off.

 

Going forward tomorrow and still trying to get two bit of black glass back in

However not yet ready to hand over to Hugh for balancing. We are still actively investigating at how we can try to get both plates back in. After talking to Calum tonight he wants me to try putting at least one of the plates back in and taking some measurements to see how we might be able to modify the plates (ie maybe score and snap a bit off.......)

Also we should take TF's of tip tilts at some stage (after doors are on probably though).

 

Oh particle counts were basically all 0 in all locations (if not zero then had a reading of 10). Sorry am usually better at recording these details.

 

Pics:

2403...before pic of the OMC before shroud work started

2426...OMC black glass shroud installed

2424..the two cables on the OMC that interfere with the OMC black glass

2435...The OMC glass shroud with the two upper glass plates removed. It doesnt look as impressive :-(

2431 & 2434..how close the cables are to the peek support with glass removed.

2410 & 2412....beam diverter, V glass beam dumps (both), and beam splitter before move of beam diverter

2441 & 2442....playing wiht cables on OMC and checking alignment of beams into and out of OMC shroud

2445, 2449, 2451 & 2453.....the beam diverter, V balck glass dumps (ne for beam diverter and one for beam splitter) and beam splitter after beam diverter move

2454 & 2455...the "holes" in the OMC black glass shroud that the beams go in and out of

2457, 2460, 2461...the OMC black glass shroud from a different angle (with the two glass panels missing)

Images attached to this report
H1 PEM
robert.schofield@LIGO.ORG - posted 20:35, Thursday 25 June 2015 - last comment - 22:29, Thursday 25 June 2015(19333)
High acoustic coupling likely due to HAM6 ISI blade spring and suspension wire resonances; wire damping demonstrated

Summary: Frequencies excited by tapping HAM6 ISI flexures while it was vented match frequencies excited in DARM by external acoustic and shaker injections.  A prototype damping clamp damped the wire resonances. We suggest development of a permanent damping clamp for the ISI suspension wires and tuned dampers for the blade springs in the 350-450 and 850-1000 Hz bands.

Ambient acoustic sound produces noise in DARM that is only a factor of 2 below our current sensitivity in the 850-1000 Hz band and not much lower in the 350-450 Hz band and several higher frequency bands (Link).  We got a chance to study HAM6 during the vent that started last week.  It turned out to be difficult to excite and monitor the resonances that dominate in vacuum when we were vented. I believe that this is because the dominant vibration coupling path to the ISI table surface during a vent is acoustic and not through the flexures, as it is in vacuum.  External shakers did not produce peaks in the geophone signals that matched the peaks in DARM. I ended up attaching a small shaker magnetically to one of the blade springs, and monitored the frequency with an accelerometer mounted close to where the flexure attached to stage 2 (see photos in Figure1).

I thought at the outset that the high-acoustic coupling bands were likely associated with modes of the ISI flexure because they lined up with ISI resonance bands characteristic of all ISIs, and all external vibration would have to be funneled through these flexures to shake the table. Figure 2 shows that I excited a number of peaks in my in-vacuum accelerometer spectra by flicking one of the 3 ISI suspension wires (number 3). The evidence that it was the wire resonances and not some other resonances that I excited by flicking the wire is strengthened by the fact that these peaks were not evident when I damped the wire by clamping a piece of Viton to it. Since flicking amplitude is not well controlled, Figure 2 shows that I went back and forth several times between clamp-on and clamp-off states. Figure 3 shows that the lowest of the excited wire resonances, 753 Hz, matches the frequency of a peak in DARM that is excited by shaking HAM6 with a shaker. Note that the peak at this frequency is not the largest feature in DARM in this region, the feature between 850-100 Hz is larger, but, resonances of the wires do seem to account for the coupling at higher frequencies.  Figure 4, for example, shows that at least two of the high frequency resonances excited by flicking the wire line up with peaks in DARM that were excited acoustically. 

Figure 5 shows that tapping on the blade spring rather than the wire produces peaks that line up with acoustically excited peaks in DARM, including the largest acoustically excited peaks in the 850-1000 Hz band. I tried clamping a small piece of Viton to the blade spring and it was not nearly as successful as the wire damping (a factor of 2 at most). Possibly a larger piece would help, but I am inclined to suggest a tuned damper like the one for the low frequency blade spring mode.

Thus I would suggest that we develop a wire clamp damper like the prototype that I made to damp the wire modes, and that we develop tuned dampers for the 350-450 Hz band and, most importantly, for the 850-1000 Hz band.

Robert S., Hugh R., Katie Banowetz, Nutsinee K.

Non-image files attached to this report
Comments related to this report
brian.lantz@LIGO.ORG - 22:29, Thursday 25 June 2015 (19335)SEI
just adding the SEI tag so I don't loose the entry.
H1 PEM
robert.schofield@LIGO.ORG - posted 20:03, Thursday 25 June 2015 (19332)
Magnetic coupling at ITMX

I was able to make a couple of PEM injections during ER7, not enough to get a full picture, but because it is of interest, we superimposed magnetic noise prediction points for the ITMX injection onto the plot for coupling at ETMY (figure). The predicted level for ITMX is flatter in frequency (some cable coupling?) but the coupling level near 10 Hz, where the prediction is closest to the DARM noise floor, is lower than for ETMY.

Robert S., Katie Banowetz

Non-image files attached to this report
H1 TCS
nutsinee.kijbunchoo@LIGO.ORG - posted 17:27, Thursday 25 June 2015 (19331)
ITM RH heating/measurement attempt

Elli, Greg, Nutsinee

The ITMY HWS return SLED beam is slightly clipped at the moment so we are testing to see whether or not the HWS sees the similar result to alog14698 before we move on to do CO2Y alignment work. Elli turned on the ITMY HWS camera yesterday morning to let it warm up. We ran the HWS script this afternoon before and after turning on the ITMY ring heater for >30 mins (the ring heater was turned on at 21:42:18 UTC). We didn't see any significant changes in spherical power, prism X, or prism Y. We also tried to run the script on ITMX HWS to see if we could get any result but the return beam was so dim that the script crashed after taking 50 sample of centriods ("Not enough unique sample points specified"). We turned everything off and called it a day. Hopefully we can work on ITMY HWS optics alignment tomorrow.

H1 CDS
patrick.thomas@LIGO.ORG - posted 16:05, Thursday 25 June 2015 - last comment - 10:41, Monday 29 June 2015(19330)
end Y chassis 3 updated
Filiberto, Patrick

I didn't realized it had been removed, and except for communication errors with the missing chassis, the PLCs ran on without apparent incident.

Filiberto made the same modifications as to the one at end X and reinstalled it. I updated the system manager accordingly, checked it into svn and activated it.

This time I didn't restart the PLCs, but I still had to restart the EPICS IOC. I burtrestored to 6:10 this morning.
Comments related to this report
filiberto.clara@LIGO.ORG - 10:41, Monday 29 June 2015 (19360)
Both End Station Controls Chassis 3 were updated to wiring diagram E1400317-v2.

The following beckhoff modules were installed:
QTY 6 : EL3104 Analog Input Terminals
QTY 1: EL9410 Power Supply Terminal for E-Bus

New modules inferface with ALS WFS Demodulators and MCL PZTs.
LHO General
corey.gray@LIGO.ORG - posted 16:02, Thursday 25 June 2015 (19318)
Ops DAY Summary

Day's Activities

H1 SEI
jim.warner@LIGO.ORG - posted 15:59, Thursday 25 June 2015 (19329)
RX FF on ST1 BSC-ISI's

After my work on the HAMS on Wednesday, I thought I would try working on BSC feedforward some more. So far I've just gotten RX FF working on ITMY (I was then promptly distracted by other stuff). First attached plot shows the improvement I've gotten between 10 and 30 hz, red and blue are the FF on and off Y ground, magenta and cyan are the T240 RX with FF on and off. Second plot shows that I managed to not spoily the Y direction anywhere (same color scheme, red/cyan FF on, blue/magenta FF off). Last plot shows my design, blue is the X/Y FF we are currently using, red is the ideal filter, green is the filter I've installed. Black was supposed to be an estimate of the performance, but I haven't quite figured that out yet, I'll post when I've fixed it. It is supposed to be something like 1 - (filter installed) / (ideal filter), but all I get is ~1, which means no subtraction.

Images attached to this report
H1 SUS (SUS)
leonid.prokhorov@LIGO.ORG - posted 15:51, Thursday 25 June 2015 (19328)
OPLEV Charge measurements
Leonid.Prokhorov, Jeffrey.Kissel

We measured ETMY and ETMX charge using optical levers. At both TM the charges are much lower than it was before discharging. Plots of the day and long-term are attached.

Note, that for ETMY we see the other sign of pitch and yaw response than it was in measurements of June, 12. We have not find the reason. We did the couple of measurements with Low-voltage driver instead the Hi-voltage. Sign of respose for Hi and Low voltage drivers agrees even if correlation of measured points for low voltage is very low. Dependencies of pitch and yaw on bias voltage are in attachment. 
Just in case: for all ETMX measurements signs are the same as June, 12. For ETMY the previous measurements of charge was in Jan and it gives us the 3rd combination of signs. 
Images attached to this report
H1 PSL (PSL)
edmond.merilh@LIGO.ORG - posted 15:39, Thursday 25 June 2015 (19327)
PSL Weekly Report - Past 10 day Trends
Images attached to this report
H1 CDS
patrick.thomas@LIGO.ORG - posted 09:56, Thursday 25 June 2015 - last comment - 14:05, Thursday 25 June 2015(19320)
Moved BPG402-SE at end X to output of photodiode chassis, chassis 3 removed
Filiberto, Patrick

Filiberto moved the cable for the gauge and I made the update to the system manger, committed it into svn, and activated it.

Filiberto then removed chassis 3 for his work on it. I disabled that chassis and the one following it in the target system manager, activated and ran that configuration. I have not restarted the PLCs because I am not sure they will run without the missing chassis. The gauge appears to still be operating however, as it does not need a PLC program.

So the end X Beckhoff PLCs are not running while Filiberto works on the chassis.
Comments related to this report
patrick.thomas@LIGO.ORG - 14:05, Thursday 25 June 2015 (19326)
Filiberto reinstalled the modified chassis. I updated the system manager accordingly, committed the change to svn and activated it. I had to reboot the computer in order to get PLC2 to run. I burtrestored to 6:10 this morning.

It is back up and running again.
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