Displaying reports 51601-51620 of 85536.Go to page Start 2577 2578 2579 2580 2581 2582 2583 2584 2585 End
Reports until 17:35, Saturday 18 March 2017
H1 SEI (OpsInfo)
jim.warner@LIGO.ORG - posted 17:35, Saturday 18 March 2017 - last comment - 17:45, Saturday 18 March 2017(34919)
Seismic configuration and high (50-ish mph) winds

The short version: Wind (finally, at 50 mph) gave us trouble locking today. I tried some stuff that may have helped, but I need commissioning time (and wind!) to see if it will do any good, but ALS REFL CTRL seems a good IFO witness. Everything is switched back after winds died down.

Travis started have troubles locking when we were having sustained winds around 40 mph and gusts over 50, so I came out to see if some of the stuff we've tried in the past would help. I can't really say for sure if what I've done has helped because winds have now died down, but I wanted to log some ideas. As I found in alog 30547, it would probably be beneficial to push the St1 RX/RY blends down to reduce the amount that the BSCs tilt above .1 hz, so I switched the ST1 RX/RY blends from the normal Quite_250 to the Quite_90 blends. I have also worked on commissioning St2 RX/RY loops (which we don't normally use) that improve the St2 motion at 1-10hz so I tried turning those on. We also use some sensor correction from St1 to St2 around .5hz, which doesn't hurt us when winds are below 30mph, but could couple St1 tilt to St2 motion with high winds, so I tried turning this off. The first 2 attached plots show the EY ISI St2 seismometers and the ground seismometer (which is a better indicator ground tilt than Y motion at these wind speeds).

The first plot shows the St2 RX/RY GS13s and you can see the the table is moving less between .1-20hz (blue is the "high wind" state, red is nominal), while the wind had dropped off  a little (cyan to pink). 

The second plot shows that this improvement in RX didn't make a drastic difference in Y (green is the "high wind" state, brown is nominal), but we gave up a bit of isolation around .5 hz by turning off the St1-St2 sensor correction.

The third plot shows the difference in the ST2 CPS. Below the blend (250mhz) the CPS are a good witness of how much tilt is being injected into the table motion, so at 40  mph it would probably be a good idea to turn this off, if we can lock with more .5hz motion. 

On Monday or Tuesday, I'll try to get a configuration (lower ST1 RX/RY blends, ST1-2 sc off, maybe a hack to get ST2 RX/RY iso loops on) in the SEI_CONF guardian.

I have added a state (and tested the transition while at DC READOUT) to the SEI_CONF called MORE_WINDY that turns off the ST1-2 sensor correction. Operators should try this state (MORE_WINDY) with high winds (40+) and low microseism.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 17:45, Saturday 18 March 2017 (34920)

These are winds and the range for the last 10 hours, note that the range started suffering when winds hit 30 mph at the CS and EY. We didn't lose lock until we had an almost 60mph gust at EX.

Images attached to this comment
LHO General
patrick.thomas@LIGO.ORG - posted 16:07, Saturday 18 March 2017 (34918)
Ops Eve Shift Transition
TITLE: 03/18 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Wind
OUTGOING OPERATOR: Travis
CURRENT ENVIRONMENT:
    Wind: 35mph Gusts, 26mph 5min avg
    Primary useism: 0.26 μm/s
    Secondary useism: 0.24 μm/s 
QUICK SUMMARY:

Jim W. is here and configuring SEI in response to the high winds.
H1 General
travis.sadecki@LIGO.ORG - posted 16:00, Saturday 18 March 2017 (34917)
Ops Day Shift Summary

TITLE: 03/18 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Wind
INCOMING OPERATOR: Patrick
SHIFT SUMMARY:  First half of the shift was good, but the second half was plagued by high winds.  We had one short lock stretch during a lull in the winds, but the wind picked back up with even more ferocity.  Gusts to ~60 mph for the last couple of hours.  JimW is on site poking at ISI blends in hopes of helping combat the effects of the wind. 
LOG:  See previous aLogs.

 

H1 General
travis.sadecki@LIGO.ORG - posted 14:14, Saturday 18 March 2017 - last comment - 15:06, Saturday 18 March 2017(34914)
Lockloss 21:12 UTC

Apparently wind is still an issue.  After a brief lull, sustained winds are back above 40 mph.

Comments related to this report
krishna.venkateswara@LIGO.ORG - 15:02, Saturday 18 March 2017 (34915)SEI

Under such high sustained wind speeds (>40 mph), I would recommend switching the beam-direction rotation loops on Stage 1 ISIs to 90 mHz blends instead of the 250 mHz blends. This is not automated, I think, so you may have to do it by hand for each chamber: rX on ETMY, ITMY and rY on ETMX and ITMX. Jim and Rich had showed that this was helpful under high winds.

travis.sadecki@LIGO.ORG - 15:06, Saturday 18 March 2017 (34916)

I texted Jim for some more advice related to Krishna's suggestion.  He informed me that he is on his way to the site.  I will wait for him to arrive before making any changes to the SEI configuration.  Stay tuned.

H1 General
travis.sadecki@LIGO.ORG - posted 14:04, Saturday 18 March 2017 (34913)
Observing at 21:00 UTC

No issues coming back up.  Winds are still 30+ mph with a few 50 mph gusts, but we managed to get back to NLN.  PI mode 23 has been giving a bunch of alarms since the winds started, but they quickly ring back down (on the order of seconds).  Also have received a few Tidal X and Y error messages, but they don't seem to be affecting locking.

H1 General
travis.sadecki@LIGO.ORG - posted 12:55, Saturday 18 March 2017 (34912)
Lockloss 19:53 UTC

Lockloss likely due to high winds, which were gusting to 50 mph at the time of the lockloss.

H1 General
travis.sadecki@LIGO.ORG - posted 12:23, Saturday 18 March 2017 (34911)
Ops Day Mid Shift Summary

Locked in Observing for 11.5 hours.  Wind has picked up significantly since the beginning of the shift (now approaching 40mph) and the range has started to suffer as a result (~50 MPc).  No issues otherwise.

H1 General
travis.sadecki@LIGO.ORG - posted 08:29, Saturday 18 March 2017 - last comment - 08:30, Saturday 18 March 2017(34909)
GRB alert 15:28 UTC
Comments related to this report
travis.sadecki@LIGO.ORG - 08:30, Saturday 18 March 2017 (34910)

Another GRB alert at 15:30 UTC.

H1 General
travis.sadecki@LIGO.ORG - posted 08:02, Saturday 18 March 2017 (34908)
Ops Day Shift Transition

TITLE: 03/18 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 67Mpc
OUTGOING OPERATOR: Ed
CURRENT ENVIRONMENT:
    Wind: 10mph Gusts, 9mph 5min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.25 μm/s
QUICK SUMMARY:  No issues handed off.  Observing for the past 7 hours. 

 

H1 General
edmond.merilh@LIGO.ORG - posted 07:56, Saturday 18 March 2017 (34907)
Shift Summary - Owl

TITLE: 03/18 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 68Mpc
INCOMING OPERATOR: Travis
SHIFT SUMMARY:
LOG:
 

H1 General
edmond.merilh@LIGO.ORG - posted 05:23, Saturday 18 March 2017 (34906)
GRB Alert

12:12UTC GRB alert. Livingston contacted for confirmation of alert. Both IFOs observing.

H1 General
edmond.merilh@LIGO.ORG - posted 01:04, Saturday 18 March 2017 (34905)
Lockloss and Recovery

7:20 Lockloss - ?

7:57 NLN 

7:59 Checked a2l measurement - looked fine

8:00 accepted damping diffs for ITMY and ETMX as per the whiteboard notes

8:01 Intention Bit: Undisturbed 71Mpc

No alignments necessary. Had to spend time at Locking ALS to avoid repeated locklosses at FIND_IR. No further issues.

 

H1 General
edmond.merilh@LIGO.ORG - posted 00:12, Saturday 18 March 2017 - last comment - 00:23, Saturday 18 March 2017(34903)
Shift Transition - Owl

TITLE: 03/18 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 69Mpc
OUTGOING OPERATOR: Patrick
CURRENT ENVIRONMENT:
    Wind: 4mph Gusts, 3mph 5min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.26 μm/s 
QUICK SUMMARY:

No news is good news
 

Comments related to this report
edmond.merilh@LIGO.ORG - 00:23, Saturday 18 March 2017 (34904)

Spoke too soon.....

LHO General
patrick.thomas@LIGO.ORG - posted 23:59, Friday 17 March 2017 (34902)
Ops Eve Shift Summary
TITLE: 03/17 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 69Mpc
INCOMING OPERATOR: Ed
SHIFT SUMMARY: In observing the entire shift. No issues or changes in status to report. Note Cheryl's alog about SDF changes for bounce mode damping if we lose lock.
LOG:

~03:39 UTC Unidentified noise in control room. Sounded vibrational. Lasted for about a minute. HVAC?
LHO General
patrick.thomas@LIGO.ORG - posted 20:07, Friday 17 March 2017 (34901)
Ops Eve Mid Shift Summary
No change in status or issues to report.
H1 TCS (TCS)
aidan.brooks@LIGO.ORG - posted 17:25, Friday 17 March 2017 - last comment - 12:55, Friday 24 March 2017(34900)
Second measurement of ITMX

I analyzed the HWS data for the lock-acquisition that occurs around 1173641000. The "point source" lens appears very quickly (within the first 60s) and then we see a larger thermal blooming over the next few hundred seconds. I've plotted the data below (both gradient field and wavefront OPD). There are a few obviously errant spots in the HWS gradient field data. Since I'm still getting used to Python, I've not managed to successfully strip these off yet. However, it is safe to ignore them.

Check out the video too. Next step is to match a COMSOL model of thermal lensing with a point absorber to the data to get a best estimate of the size of absorber and the power absorbed (preliminary estimates are of the order of 10mW).

FYI: this measurement compares the system before, during and after a lock-acquisition (ignore the title that says "lock-loss"). The previous measurement, 34853, looked at lens decay before, during and after a lock-loss.

 

Images attached to this report
Non-image files attached to this report
Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 18:11, Monday 20 March 2017 (34958)

For your amusement I've attached a GIF file of the same data. My start time is 79 seconds prior to Aidan's "current time".

Images attached to this comment
aidan.brooks@LIGO.ORG - 12:09, Thursday 23 March 2017 (35043)

The integrated gradient field data for H1ITMX is contained in the attached MAT file. It shows the accumulated optical path distortion (OPD) after 2.75 hours following the lock acquisition around 1173640800. This is the total accumulated OPD for a round trip through the CP+ITMX substrates, reflection off ITMX_HR and back through ITMX+CP substrates.

  • H1HWSX_wf_data.x = hswf.grid_x;      % x coordinates of every point in WFcropped
  • H1HWSX_wf_data.xUnits = 'm';           
  • H1HWSX_wf_data.y = hswf.grid_y;      % y coordinates of every point in WFcropped
  • H1HWSX_wf_data.yUnits = 'm';
  • H1HWSX_wf_data.WFcropped = hswf.wf_numerical;        % optical path distortion of every point in WFcropped
  • H1HWSX_wf_data.WFcroppedUnits = 'm';
  • H1HWSX_wf_data.t0 = 1173640800;
  • H1HWSX_wf_data.t1 = 1173649900;
  • H1HWSX_wf_data.deltat = 1173649900-1173640800;
  • H1HWSX_wf_data.comments = 'Integrated HWS data. H1ITMX. Start (reference) and finish times are t0 and t1. x and y arrays contain coordinates. Cropped wavefront is central region where genuine data is believed to be. Outside the 85 mm radius is not real data'

Note: this image is inverted. In this coordinate system, the top of the ITM is at the bottom of the image.

Here is the wavefront data with the superimposed gradient field. The little feature around [+30mm, +20mm] does not appear in the animation of the wavefront or gradient field over much of the preceeding 2.75 hours. My suspicion is that this is a data point with a larger variance that the other HWS data points, rather than a true represtation of wavefront distortion.

 

 

Images attached to this comment
Non-image files attached to this comment
aidan.brooks@LIGO.ORG - 11:58, Friday 24 March 2017 (35069)TCS

I fitted, by eye, a COMSOL model of an absorber (14mm diameter Gaussian, ~25mW absorbed) to the measured HWS data. I then removed this modeled optical path distortion to get the following residual (lower left plot). I then fitted a COMOSL model of 30mW uniform absorption to this model and subtracted it to get the residual in the lower right plot.

 

Images attached to this comment
aidan.brooks@LIGO.ORG - 12:55, Friday 24 March 2017 (35071)

Here's the total fitted distortion from the sum of two COMSOL models (point absorber + uniform absorption):

 

Images attached to this comment
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