Displaying reports 55941-55960 of 87440.Go to page Start 2794 2795 2796 2797 2798 2799 2800 2801 2802 End
Reports until 04:35, Friday 09 December 2016
H1 ISC
jim.warner@LIGO.ORG - posted 04:35, Friday 09 December 2016 - last comment - 07:10, Friday 09 December 2016(32382)
PI modes being difficult tonight

Getting to NLN tonight hasn't been a problem so far, but there seem to be a forest of features at 18khz that are upset, and I don't see any filters to handle them. Attached spectra are from the current lock stretch (blue) and the 2 hour lock from 23 hours ago. The features around 18040 hz have been the most problematic, maybe the current bandpasses are good for some of the peaks in that region, but not others? The peak at 18038.5 has been the worst, none of the  filters seem to do any good. So far I've had the best luck using a gain of 1000 on Mode 27, but .....

And before I could hit post 18038.5 rang up and broke the lock.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 06:05, Friday 09 December 2016 (32383)

Just got done talking to Terra and Keita. With Keita's approval (because it seems to be required to get the IFO running stably), Terra walked me through making a new bandpass filter for this mode:

cheby2("BandPass",4,40,237,240)butter("BandPass",2,237,240)notch(238.5,20,30)gain(31.6228)

This is installed as 18038p5Hz in FM5 on Mode 27 (Terra suspects this mode is also on ETMY). Turning it on created SDF diffs that I've accepted, and I hit the intent bit 20 seconds before 6:00 local.

terra.hardwick@LIGO.ORG - 07:10, Friday 09 December 2016 (32385)

Jim is awesome and mode seems to be holding stable.

This one was a bit confusing because we have two ETMY modes close to one another, one at 18038ish Hz and one at 18042ish, Hz as seen in Jim's spectum. This is probably the source of TJs problems last night (sorry TJ), though when I checked earlier today the peak I trended from his shift was within the BP so I didn't suspect that to be the problem. Jim scooted over the BP and PLL set frequency to be over the 18038 Hz mode. Next day I'm in, I will create a new mode so that the two can be differentiated. Note though that the 18042 Hz mode did not go unstable just now even though we weren't damping it. I'll look into the last several locks and see which seems to be the regularly problematic one. We also weren't driving quite hard enough; Jim increased the damping gain which worked much better.

For now: If Mode27 seems unresponsive, open PI DTT and check if the growing peak is at 18038 or 18042 Hz. Then check the following:

  • Open Mode27 in the PI medm screen.
  • Open the BandPass filter bank
  • Change the mode27 Bandpass filter if necessary (filters for both options now exist) to cover the correct peak frequency 
  • Open the PLL screen for that mode
  • Set the PLL 'set frequency' to 238 (if the peak is at 18038) or 242 (if the peak is at 18042) 
H1 General
travis.sadecki@LIGO.ORG - posted 00:03, Friday 09 December 2016 (32381)
OPS Eve Shift Summary

TITLE: 12/09 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Jim
SHIFT SUMMARY:  A bit of an extended recovery from the EQs led to a late shift lock.  Lost lock just before the shift ended due to PI modes ringing up while I was using the facilities.
LOG:

See previous logs for most of the story.

7:57 Lock loss.

 

H1 DetChar
corey.gray@LIGO.ORG - posted 23:54, Thursday 08 December 2016 (32380)
H1 DetChar Summary Pages Went Down at 2:10UTC (6:10pmPST)

I sent an email to detchar@sympa.ligo.org this time (vs. detchar@ligo.org).

H1 General
travis.sadecki@LIGO.ORG - posted 23:31, Thursday 08 December 2016 (32379)
Observing at 7:29 UTC

After a bit of a battle with bounce/roll modes, we have made it back to NLN and Observing.

H1 INJ (CAL, INJ)
richard.savage@LIGO.ORG - posted 22:49, Thursday 08 December 2016 - last comment - 23:30, Thursday 08 December 2016(32376)
HW injection schedule file and Inspiral directory updated, Xend Pcal line stopped in anticipation of HW injections

EvanG, RickS

The HWinj schedule file on h1hwinj1 was updated as well as the Inspiral directory.

The Schedule file was loaded in the Guardian. (by Travis in the control room).

The HF Pcal line at Xend was stopped at 6:41 UTC (by Travis in the control room).

Six CBC injections are schedule to go in tomorrow morning, starting at 6 AM PST and separated by 70 minutes.

We will want to restart the Pcal line at Xend when the injections are finished, around noon tomorrow (Friday).

Comments related to this report
travis.sadecki@LIGO.ORG - 22:59, Thursday 08 December 2016 (32377)

Screenshot of PCal X line prior to being turned off.

Images attached to this comment
travis.sadecki@LIGO.ORG - 23:30, Thursday 08 December 2016 (32378)

I also had to accept the SDF diffs for turning this line off in order to go to Observing.  See screenshot.

Images attached to this comment
H1 AOS
travis.sadecki@LIGO.ORG - posted 21:25, Thursday 08 December 2016 (32375)
Back to locking

I ran through IA twice because by the time I finished the first round, the arms had drifted off enough that ALS wouldn't lock.  The second time seems to have gone better as we are now past DRMI.

H1 General
travis.sadecki@LIGO.ORG - posted 19:55, Thursday 08 December 2016 (32373)
Ops Eve Mid-shift Summary

The earth has calmed down enough to start relocking finally.  I am struggling through IA since everything was way out of whack following the EQs.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 16:04, Thursday 08 December 2016 - last comment - 16:36, Thursday 08 December 2016(32371)
Ops Day Shift Summary
Ops Shift Log:12/08/2016, Day Shift 16:00 – 00:00 (08:00 - 16:00) Time -  UTC (PT)
State of H1: IFO is DOWN due to EQs.
Intent Bit: Environment
Support: N/A
Incoming Operator: Travis
Shift Summary: The IFO has been down all shift down to strong and continuous earthquake activity throughout the Pacific. 
 
Activity Log:Time - UTC (PT)
16:00 (08:00) Take over from TJ
17:09 (09:09) Karen – Going to Mid-Y for cleaning
17:18 (09:18) Christina – Going to Mid-X for cleaning
17:50 (09:50) Chris – Moving stuff from OSB multipurpose room to the LSB
18:00 (10:00) Put IFO into DOWN due to Mag8.0 EQ near the Solomon
18:11 (10:11) Karen – finished at Mid-Y coming back to the corner
18:20 (10:20) Christina – Finished at Mid-X coming back to the corner
18:21 (10:21) Kyle – Going to Mid-Y
18:40 (10:40) Kyle – Back from Mid-Y
19:32 (11:32) Richard – Going into LVEA to get temperature monitor labels
19:45 (11:45) Richard – Out of the LVEA
00:00 (16:00) Turn over to Travis
Comments related to this report
jenne.driggers@LIGO.ORG - 16:36, Thursday 08 December 2016 (32372)

Yeah, it's been one of *those* days...

Images attached to this comment
H1 DetChar (DetChar)
beverly.berger@LIGO.ORG - posted 14:57, Thursday 08 December 2016 (32370)
DQ Shift: Monday 5 Dec 00:00 UTC - Wednesday 7 Dec 23:59 UTC

Beverly, Terra, Young-Kim

 

Full results from the DQ shift may be found here.

 

H1 AOS
jeffrey.bartlett@LIGO.ORG - posted 14:56, Thursday 08 December 2016 - last comment - 14:29, Friday 09 December 2016(32368)
CPS Sensor Spectra (FAMIS #6875)
   Posted are the plots for the CPS Sensor Spectra. 
Images attached to this report
Comments related to this report
richard.mittleman@LIGO.ORG - 06:49, Friday 09 December 2016 (32384)

HAM 2 needs a second look

jeffrey.bartlett@LIGO.ORG - 14:29, Friday 09 December 2016 (32400)

Reran the HAM2 HAM3 CPS Sensor Spectra. New plot is posted below. Between 20 ans 60Hz, HAM2 looks a bit better. 

Images attached to this comment
LHO VE (DetChar)
kyle.ryan@LIGO.ORG - posted 14:15, Thursday 08 December 2016 - last comment - 09:50, Friday 09 December 2016(32367)
Need DetChar to scrutinize data

We have a diagnostic setup at BSC8 that we need to run for several consecutive days.  This setup utilizes rotating shaft vacuum pumps that have the potential of effecting the IFO data.  Prior to the start of O2, we had Robert S. monitor the IFO signal(s) while it was locked and in "Low Noise" both with the pumps on and also off, i.e. we did "on/off" tests (see alog entry 31802).  Additionally, and on more than one occasion, we had ran these for several consecutive days during which the IFO experienced long lock stretches at good sensitivity.  As such, we were hoping that someone could examine the pertinent IFO data during the following two time segments to look for any evidence of these pumps running.  In both cases, the pumps in question were running continuously:  


November 24th, 0230 UTC to November 29th, 1800 UTC and

December 5th, 1900 UTC to December 7th, 0035 UTC.  

Comments related to this report
keith.riles@LIGO.ORG - 20:48, Thursday 08 December 2016 (32374)DetChar
Attached is a zipped tar file of spectral comparisons for the two pump-on periods cited
and for an intervening pump-off period. Since I don't know what the pump frequency
is supposed to be, I'm not sure where to focus attention, but I'm not seeing gross differences
other than higher 60-Hz harmonics in both pump-on periods (is that expected from
the pumps?), along with the overall greater excitation / upconversion of violin modes and
the presence of  "silent" calibration lines at 22.3 and 30.1 Hz in the first pump-on period. 

Here are the FScanned data intervals used:

pumpon-1 -- 23.5 hours of SFTs collected between Nov24th, 0230 UTC and Nov 29th, 1800 UTC
pumpon-2 -- 11.5 hours between Dec 5th, 1900 UTC and Dec 7th, 0035 UTC
pumpoff -- 78 hours between Nov 30, 14:00 UTC and Dec 5th, 14:00 UTC

If there are particular frequencies where I should be expecting disturbances,
let me know and I'll do some zooming. 
Non-image files attached to this comment
keith.riles@LIGO.ORG - 09:50, Friday 09 December 2016 (32390)
Kyle informed me offline that the pumps run at 1720 RPM (28.667 Hz) 
with small turbos running at 90,000 RPM (1500 Hz). Attached are zooms
of bands around the first four harmonics 28.667 Hz (band sizes increase
linearly with harmonic number) and around 1500 Hz. I don't see anything
jumping out at me in any of the low-frequency bands that indicates an 
artifact restricted to pump-on times. 

The region around 1500 Hz is harder to interpret because of different average 
quad violin mode excitations and associated up-conversion.

Fig 1 - 28.5-28.8 Hz
Fig 2 - 57.0-57.6 Hz
Fig 3 - 85.5-86.4 Hz
Fig 4 - 114.0-115.2 Hz
Fig 5 - 1480-1520 Hz
Images attached to this comment
H1 General
jeffrey.bartlett@LIGO.ORG - posted 13:40, Thursday 08 December 2016 (32366)
Ops Day Mid-Shift Summary

Earthquakes continue to occur throughout the Pacific. Latest are a 5.2 off Chile, and two more 5.2 off the Solomon’s. Microseism had dropped below 1.0um/s but is now back up to over 8.0um/s. Continue to hold the IFO in DOWN until things settle down.   

H1 General
jeffrey.bartlett@LIGO.ORG - posted 10:49, Thursday 08 December 2016 (32362)
IFO Down - Earthquake Activity

After things started to settle down from the California eaethquake, we were hit by another mag 7.8 earthquake in the Solomon Islands. Put the SEI_CONF to LARGE_EQ_NOBRSXY. All ISI and several SUS have tripped many times. Microseism is over 300um/s.

IFO in down while we ride through the rumbling earth.  

H1 SUS
thomas.shaffer@LIGO.ORG - posted 05:15, Thursday 08 December 2016 - last comment - 15:31, Friday 09 December 2016(32354)
PI slightly rung up modes that we are not damping

It seems like there are some PI modes that we are no longer damping that are slightly run up according to the dtt. I also wonder if the peaks at around 13000hz are modes that we had not had issues with before, or maybe something else entirely? I don't see any mention of them on the PI medm and they are currently the highest. I will try to damp some of the other ones if they get any higher.

The attached shows the PI dtt just after reaching low noise.

Images attached to this report
Comments related to this report
thomas.shaffer@LIGO.ORG - 06:01, Thursday 08 December 2016 (32356)

Well I think things are stable now. I ended up flipping the sign for the both the phase and gain on mode 27. Mode 26 also came up and changing the phase got it to, very slowly, go down. I took some screen shots of the dtt template at 20min, 26min, and 32min into the lock. The modes that the Striptools said were ringing up, didnt necessarily agree with the dtt. I dont remember how much the modes can shift in frequency, but it seems like some of them were off by a couple of hz. 

Images attached to this comment
terra.hardwick@LIGO.ORG - 11:58, Thursday 08 December 2016 (32364)OpsInfo

A couple things:

  • I'm not sure what you're referencing that seems 'a couple Hz off', could you elaborate? I checked the band pass filters against the frequency of the peaks at the times you listed and the most I found was Mode28 was off by 1 Hz. I have since changed the BP filter to account for this shift. 
  • Remember that if a peak's frequency in DTT is different than the bandpass filter frequency, you should switch to a different band pass. There are explicit directions in the PI Wiki (which you can open from the PI medm screen and which I just updated to make more clear) and I've walked through this process individually with each operator. If something is still unclear, you can always still call me at anytime (number on the whiteboard). This shouldn't be much of an issue these days but is worth checking if you're having damping problems.
  • Modes 27 and 29 have to be carefully watched during the first hour of lock. These have been successfully damped for weeks now but must be reacted to immediately. 
  • Again, if you lose lock from a PI, you must wait in DC readout to give that mode time to ring down. You can watch the ringdown in DTT. If you try locking again, the mode will still be rung up.
  • There are some modes that always have higher amp, such as the 13kHz modes TJ noted, that are not unstable - TJ that DTT from low noise you first posted is totally normal. You can always look at a reference from an eariler stable lock time to compare the amplitudes. I will add a good reference to the PI DTT in the background so it's easy to see what's 'good'
  • Regarding DTT and StripTool not seeming to match - we use different error signals for different modes, while the DTT is just looking at one of those signals. The result is that Modes 27,28 look very rung up on the StripTool but their peaks in the DTT dont look so high. This is done on purpose, because those modes need to be damped faster. 

Please any operator contact me at any time if help/explanations/etc is needed.

thomas.shaffer@LIGO.ORG - 15:31, Friday 09 December 2016 (32401)

For the couple hz off thing, I was mainly refering to the frequencies listed on the medm above the modes. I'm not sure how accurate these are suppose to be, but like mode 27 says 18041, and the dtt was saying that 18038 seemed to be more rung up (see second attached). I didn't remember how much they shifted, and I did not look at the actual filters themselves at the time.

I was able to make it work (on the second try) with just changing phase and gain so I didn't look into it too much after that. But, yes, following your instructions and changing the BP would have been next on the list.

In alog32385 you mention that you will put a reference trace to show what is normal and what is not. I would love this because I looked at the dtt picture that is on the wiki and saw that it was much different. Either way, it was a good learnign process for me since I have only ever had to change phases for PI modes.

H1 ISC
evan.hall@LIGO.ORG - posted 14:41, Tuesday 06 December 2016 - last comment - 11:36, Thursday 08 December 2016(32257)
CPY ghost beams on the SRM

Keita, Rana, Evan

After refocusing the HAM5 camera, we see in full lock that there are at least two ghost beams hitting the SRM composite mass. These ghost beams move when CPY (but not CPX) is moved.

The attached plots show the DARM spectrum for different CPY alignments. There is no obvious sweet spot, but perhaps we will find one by looking at some long-term DARM BLRMS.

This image shows the HAM5 camera with the nominal CPY alignment (-150 µrad in pitch, 0 µrad in yaw). The two bright, vertically aligned spots on the left-hand side are the CPY ghost beams.

Images attached to this report
Non-image files attached to this report
Comments related to this report
evan.hall@LIGO.ORG - 14:42, Tuesday 06 December 2016 (32258)

Also, the take snapshot button for camera 17 just saves blank images.

 

sheila.dwyer@LIGO.ORG - 15:23, Tuesday 06 December 2016 (32263)PEM

Here are 2 other old alogs that are relevant if you are worried about scatter from CPs:

Robert saw scattering from CPY in the PR2 camera:  31243

I saw that 6 times higher drive was needed on CPX than CPY to make noise show up in DARM, and the noise that did show up was clear fringe wrapping shelves for CPX and a broad shelf for CPY.  30979

CPY scattering seemed like it is not an immediate problem since the drive reuiqred to see noise in DARM was 100 um at the error point of the damping loop at 0.1 Hz.  I don't know the gain of the damping loop, but assume that it is not less than -20 dB at 0.1 Hz, so that we are pushing the mass at least 10 um, probably more. This should be larger than the normal path length modulation.  It would be good to look at what the gain of the damping loop actually is to see if this is really a much larger path length modulation than what we would normally expect.  

denis.martynov@LIGO.ORG - 11:36, Thursday 08 December 2016 (32365)

SRC model shows that CPY is installed parallel to HR surface of ITMY (misalignment angle of 0.07 degrees). This number gives a vertical offset of the ghost beam on SR2 of 2 cm and on SRM of 10 cm. This is how I read the camera image. One might also suggest that the plate is misaligned even further from the nominal position — by 0.14 degrees. In this case ghost beams swap and we can’t tell a difference.

H1 CAL (CAL)
craig.cahillane@LIGO.ORG - posted 17:42, Sunday 04 December 2016 - last comment - 10:25, Thursday 08 December 2016(32169)
LHO ER10 Gaussian Process Actuation Uncertainty Budget
C. Cahillane

The ER10 LHO Actuation Uncertainty Budget

What has been done:
(1) Gathering all the Newtons/count actuation function measurements for the three stages (UIM, PUM, TST) from November 8th, 9th, 11th, 12th, and 18th.  
(2) Running an MCMC over the physical parameters gain and delay for all three stages.  (Only used freq < 10 Hz for UIM, freq < 100 Hz for PUM)
(3) Plot MCMC cornerplots and resulting residuals uncertainty budget from the MCMC PDFs.  
(4) Take the residuals from the MCMC physical parameters' fit, and plug them into a Gaussian Process with kernel k(x,y) = a + b * exp(-0.5*(x-y)**2/l**2), where a, b, and l are the hyperparameters of the GP.
(5) Train the GP on the residuals, and produce a mean posterior fit and an uncertainty budget from the trained kernel.

TL:DR : Take measurements -> Physical MCMC -> Unmodeled GP -> Frequency-Dependent Systematic Error +- Uncertainty Budget

The mean posterior fit is the frequency-dependent systematic error.  The uncertainty budget is also frequency-dependent.  
The Gaussian Process results are shown in Plots 1, 2, and 3 for the UIM, PUM, and TST stages.  The 1-sigma, 68% confidence intervals are plotted.

I want to call attention to how small the uncertainty is in the bucket.
The frequency-dependent uncertainty in the bucket is on the order of 0.1%

This is exciting, but is it real?  
Points in favor:
(1) We have five sets of measurements, and uncertainty roughly goes as 1/sqrt(N) where N = measurement number.  This allows us to win a lot where the measurements are nearly the same and the errorbars are small.
(2) The GP fit hits most of the measurement errorbars.
(3) Uncertainty expands where we have less information.
Points against:
(1) Overfitting might be a problem.  There seem to be unphysical wiggles that nail our data in the bucket. 
(2) This uncertainty budget is lower than ever before by a factor of 10.  This requires extraordinary proof.   
Rebuttals:
(1) We might be able to combat overfitting by lengthening the kernel length-scale and adding more noise to our measurements.  Also, the whole point of this method is to capture unmodeled wiggles.  
(2) The data analysis methods used are more advanced and designed to handle frequency-dependence.  

Plots 4, 5, and 6 are the UIM, PUM, and TST physical model MCMC fits with the measurements.  
Plots 7, 8, and 9 are the UIM, PUM, and TST physical model MCMC parameter cornerplots.

A couple of points: 
(1) The GP uncertainty doesn't take into account the uncertainty from the MCMC physical parameters.  The GP uncertainty dominates nearly everywhere, since the MCMC uncertainty is so tiny (See plots 4, 5, 6).  I may try to incorporate the MCMC uncertainty directly into the measurement errorbars that I input into the GP.
(2) A lot remains to be done.  LLO actuation, sensing at both sites, and final response uncertainty.  
(3) If these results hold, we may have uncertainty dominated by time-dependence.  Stay tuned.
Images attached to this report
Comments related to this report
craig.cahillane@LIGO.ORG - 10:25, Thursday 08 December 2016 (32361)
C. Cahillane

I have changed the kernel the Gaussian Process runs on in order to get more realistic errorbars.

The plots for the UIM stage have a dot product kernel: k(x,y) = 1.0 + x.y + noise
The plots for the PUM and TST stage have a squared dot product kernel: k(x,y) = 1.0 + x.y + (x.y)**2 + noise

The results show a much more simplistic and physically realistic correlation between measurement points. (No more overfitting wiggles, slightly expanded uncertainty bars, no instabilities in the GP results)

Our minimum uncertainty in the TST stage in the bucket is on the order of ~0.6% and 0.3 degrees.  So still very good uncertainty.

Still to do:
(1) Remove time-dependence from the measurements by modifying the .conf files with the relevant kappas.
(2) MCMC to find physical parameters on only the reference measurement.
(3) LLO Actuation, LHO and LLO Sensing.
Images attached to this comment
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