Displaying reports 50521-50540 of 85102.Go to page Start 2523 2524 2525 2526 2527 2528 2529 2530 2531 End
Reports until 13:56, Monday 17 April 2017
H1 ISC
sheila.dwyer@LIGO.ORG - posted 13:56, Monday 17 April 2017 - last comment - 17:05, Tuesday 18 April 2017(35589)
a few minutes of commisioning time

I started to repeat the measurement described in llo alog 28797 while we were waiting for LLO to come back up around 20:05 UTC. Since LLO is back, I have stopped and put things back to normal, and Cheryl is running A2L before we go back to observing. (This was about 45 minutes of commisioning). 

I got as far as tuning an excitation and finding that an offset of around 0.3 in POSY may be about right, but that we need to wait a long time for the OMC ASC loops and the slow kappa C calculation to settle when making these measurements.  The template with the excitation is saved at sheila.dwyer/OMC/OMC_alignment_jitter_check.xml  We will continue this Wednesday.

Images attached to this report
Comments related to this report
terra.hardwick@LIGO.ORG - 16:34, Monday 17 April 2017 (35595)

Set the gain of PI modes 27 to zero next time you do this measurement.

As Cheryl noted, mode 27 rang up during your work today (mode 19 was just bleed over from 27). Since we're using OMC DCPD as the error signal for this mode, driving OMC ASC loops changes the phase as seen by this mode such that we must've been driving up the PI; mechanical drive up was real, as it was seen by the TransMon QPD. 

This mode is nominally stable after the thermal transient, so as long as you're an hour or so into a lock, you can just set the gain of mode 27 to zero during OMC commissioning.   

Images attached to this comment
sheila.dwyer@LIGO.ORG - 17:05, Tuesday 18 April 2017 (35645)

I also took about 10 minutes with the interferometer locked on RF just now to put some offsets into the OMC alignment loops.  These dither loops are very slow, it takes about 3 minutes for them to react to an offset change.  For POS X introducing an offset of 0.3 decreases the transmitted power to 88%, for POS Y an offset of 0.3 decreases it to 95% of the power for the normal alingment.  I didn't get to check the ANG loops, but it seems like they will need larger offsets (2 or 3). 

LHO VE
logbook/robot/script0.cds.ligo-wa.caltech.edu@LIGO.ORG - posted 12:10, Monday 17 April 2017 - last comment - 08:22, Tuesday 18 April 2017(35587)
CP3, CP4 Autofill 2017_04_17
Starting CP3 fill. LLCV enabled. LLCV set to manual control. LLCV set to 50% open. Fill completed in 1200 seconds. LLCV set back to 20.0% open.
Starting CP4 fill. LLCV enabled. LLCV set to manual control. LLCV set to 70% open. Fill completed in 1484 seconds. LLCV set back to 38.0% open.
Images attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 08:22, Tuesday 18 April 2017 (35609)

Raised both by 1%.

CP3 to 21%

CP4 to 39%

 

Contemplating the next layer of automation by adding to code incremental increases/decreases to LLCV control value.

H1 CAL (CAL)
sudarshan.karki@LIGO.ORG - posted 11:53, Monday 17 April 2017 (35586)
Pcal beam spot Position at LHOX

RickS, VaishaliA, HeatherF, SudarshanK

We analyzed the pictures of the ETM and Pcal beam spots taken on 2017/04/11 (Tuesday maintenance) to determine the position of the Pcal beams. The numbers below are the position of the Pcal beams from their nominal position of [ 0, 111.6] mm for upper beam and  [0, -111.6] mm for lower beam. 

Upper Beam [1.1+/-0.3, 1.1+/-0.2]

Lower Beam [-1.1+/-0.2, 1.3+/-0.3]

These numbers are comparable to numbers obtained from the pictures taken few weeks ago - LHO alog # 35347.

P.S. The number reported here are mean values of multiple analysis on multiple pictures  and the number in the attached picture is only one such number and thus may be different.

Images attached to this report
H1 SEI
travis.sadecki@LIGO.ORG - posted 10:28, Monday 17 April 2017 (35585)
HEPI Pump Pressure 45 Day Trends

I don't see any egregious excursions.  The brief dip in the EX pressure was previously noted in TJ's trend from March 20 (aLog 34936).  Also, the glitching in the EY pressure noted in the same aLog seems to have been fixed.  This closes FAMIS task 4531.

Images attached to this report
H1 General
cheryl.vorvick@LIGO.ORG - posted 08:17, Monday 17 April 2017 (35583)
Ops Day Summary:

TITLE: 04/17 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 64Mpc
OUTGOING OPERATOR: Ed
CURRENT ENVIRONMENT:
    Wind: 9mph Gusts, 7mph 5min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.13 μm/s
QUICK SUMMARY:

H1 General
edmond.merilh@LIGO.ORG - posted 07:53, Monday 17 April 2017 (35582)
Shift Summary - Owl

TITLE: 04/17 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 55Mpc
INCOMING OPERATOR: Cheryl
SHIFT SUMMARY:

Nothing to report. IFO locked for 34hrs20min
LOG:

H1 General
edmond.merilh@LIGO.ORG - posted 00:41, Monday 17 April 2017 (35581)
Running a2l - Livingstgon still down from EQ

7:28UTC YAW out by .65

7:33UTC Intention Bit Undisturbed

H1 General
edmond.merilh@LIGO.ORG - posted 00:10, Monday 17 April 2017 (35580)
Shift Transition - Owl

TITLE: 04/17 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 63Mpc
OUTGOING OPERATOR: Corey
CURRENT ENVIRONMENT:
    Wind: 14mph Gusts, 12mph 5min avg
    Primary useism: 0.06 μm/s
    Secondary useism: 0.12 μm/s
QUICK SUMMARY:

 

LHO General
corey.gray@LIGO.ORG - posted 00:03, Monday 17 April 2017 (35575)
EVE Shift Summary

TITLE: 04/16 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 64Mpc
INCOMING OPERATOR: Ed
SHIFT SUMMARY:

H1 locked for over 26hrs.  Fairly quiet other than an earthquake (which we rode through).
LOG:

H1 SEI (OpsInfo, SEI)
corey.gray@LIGO.ORG - posted 23:22, Sunday 16 April 2017 (35578)
Earthquake Report: 5.6 Barbuda Island

Didn't really notice this until I happened to look up at the Pit ASC Control Signal strip tool and saw noticeable oscillations, & then I saw all other markers for an EQ.

H1 SUS
corey.gray@LIGO.ORG - posted 17:48, Sunday 16 April 2017 (35577)
L1 Down, Ran A2L & Damped 4.7kHz

A2L measurement showed elevated in Yaw, so ran A2L.

4.7kHz was damped at the beginning of the lock last night with 0deg (MODE10 outmon went down to +/-2000counts on strip tool).  But saw that the resonance was rung up again.  So, I tried +30deg & this quickly rung up the resonance.  I then added -60deg (for net -30deg) & this took damped out the resonance within minutes (& took the MODE10 outmon to +/-10 counts).

Summary of 10min out of Observing:

LHO General
corey.gray@LIGO.ORG - posted 16:33, Sunday 16 April 2017 (35574)
Transition To Eve

TITLE: 04/16 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 64Mpc
OUTGOING OPERATOR: Cheryl
CURRENT ENVIRONMENT:
    Wind: 7mph Gusts, 5mph 5min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.12 μm/s 
QUICK SUMMARY:

H1 General
cheryl.vorvick@LIGO.ORG - posted 16:02, Sunday 16 April 2017 (35570)
Ops Day Summary

TITLE: 04/16 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 62Mpc
INCOMING OPERATOR: Corey
SHIFT SUMMARY: locked all shift, no issues other than some wind causing some noise, web page stat was yellow is now green

H1 CAL (CAL)
aaron.viets@LIGO.ORG - posted 09:39, Sunday 16 April 2017 - last comment - 16:20, Sunday 16 April 2017(35569)
LHO pipeline restarted to correct bad kappas and h(t)
I have just restarted the primary and redundant pipelines at LHO at GPS time 1176395700. Due to an issue with the computed kappas being out of the expected range, h(t) was marked bad by the calib_state_vector. This is due to a bug in the most recent release of the calibration code, gstlal-calibration-1.1.5-v1. For more information on this bug and the proposed fix, see https://bugs.ligo.org/redmine/issues/5494
Comments related to this report
corey.gray@LIGO.ORG - 16:20, Sunday 16 April 2017 (35571)OpsInfo

Is this something Operators should worry about, or is it handled by others offsite?  Jim & Cheryl both alogged status and that Aaron was working on/fixed it.  Just wondering if this rises to the state of needing an alarm because it affects H1 data, or does it just mean one of our tools is having an issue (i.e. GWI.stat being yellow and the Daily Summary Pages reporting an on BNS range).  

Should we be checking the GWI.stat through the shift (I can put it in our Shift Check Sheet), or is this something we leave to off-site staff?  For GWI.stat's Help Page it says we should report bugs to Peter Shawhan.  I'm not sure of who we report Summary Page bugs to.

Images attached to this comment
H1 General
jim.warner@LIGO.ORG - posted 08:07, Sunday 16 April 2017 (35568)
Shift Summary

TITLE: 04/16 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 64Mpc
INCOMING OPERATOR: Cheryl
SHIFT SUMMARY:
LOG:
Quiet night again. Apparently, something happened with h(t) last night at 3:11 local (?), got a call from UWM about it. Sounds like they are looking into it.

LHO General
corey.gray@LIGO.ORG - posted 00:11, Sunday 16 April 2017 - last comment - 16:31, Sunday 16 April 2017(35566)
EVE Operator Summary

TITLE: 04/15 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 65Mpc
INCOMING OPERATOR: Jim
SHIFT SUMMARY:

One lockloss through the night (~30min down).  

Had a couple of SDF diffs:  

Comments related to this report
corey.gray@LIGO.ORG - 16:31, Sunday 16 April 2017 (35576)OpsInfo

Oh, and forgot to mention Jim & I encountered a porcupine at the OSB entrance last night at around 12:30am!  It was right near the 3-wheel bike.  It slowly walked away when it heard us, but just be careful!

H1 CAL (CAL, DetChar)
sudarshan.karki@LIGO.ORG - posted 08:32, Tuesday 11 April 2017 - last comment - 00:05, Monday 17 April 2017(35441)
High Frequency Pcal Injections

There were number of high frequency calibration lines injected using the automated Guardian scripts. These lines are injected using the Pcal at ENDX (ENDY is used for calibration purpose). The GPS time at which these lines were running are listed below:

Frequency Starttime Endtime
2001.3 1174765755 1174843009
2501.3 1174843010 1175048873
3001.3 1175048874 1175185602
3501.3 1175185604 1175280996
4001.3 1175280998 1175367396
4501.3 1175367398 1175532906
5001.3 1175532908  

 

Comments related to this report
sudarshan.karki@LIGO.ORG - 14:21, Tuesday 11 April 2017 (35479)

Rick, Sudarshan

Th high frequency line was moved to 5501.3 Hz. The guardian script was designed to go upto 5001.3 Hz so Rick moved the frequency to 5501.3 Hz manually during the maintenance period.  We will move this line to 6001.3 Hz when we have enough data and the ifo goes out of lock next time.

sudarshan.karki@LIGO.ORG - 00:05, Monday 17 April 2017 (35579)

Updated list of lines with their start and endtime.

Frequency Starttime Endtime
5001.3 1175532908 1175971199
5501.3 1175971561 1176156175
5751.3 1176156177 1176255835
5251.3 1176255837 1176350524
4751.3 1176350525  
H1 CAL (CAL)
aaron.viets@LIGO.ORG - posted 09:54, Friday 24 March 2017 - last comment - 05:20, Wednesday 07 June 2017(35041)
Data collected to analyze SRC detuning
I have added an (unreleased) algorithm into the GDS/DCS pipeline to compute the SRC spring frequency and Q. This algorithm was used to collect 18 hours of data on February 4 (first plot) and 18 hours of data on March 4 (second plot). The plots include kappa_c, the cavity pole, the SRC spring frequency, the SRC Q, and 4 of the coherence uncertainties (uncertainty of the 7.93 Hz line is not yet available).

The derivation this algorithm was based on is similar to what Jeff has posted ( https://dcc.ligo.org/DocDB/0140/T1700106/001/T1700106-v1.pdf ), with differences noted below:
1) The approximation made at the bottom of p4 and top of p5 was only used in the calculation of kappa_c and the cavity pole. So SRC detuning effects were not accounted for in computing S_c. However, kappa_c and the computed cavity pole were used in the calculation of S_s.
2) In eq. 18, I have a minus (-) sign instead of a plus (+) sign before EP6. S_c = S(f_1, t) has been computed this way in GDS/DCS since the start of O2 (I assume during O1 as well).
3) Similarly, in eq. 20, I have a minus sign (-) before EP12.
4) In the lower two equations of 13, I have the terms under the square root subtracted in the opposite order, as suggested by Shivaraj. (Also, I noted that the expression for Q should only depend on S(f_2, t), with no dependence on S(f_1, t). )

The smoothing (128s running median + 10s average) was done on f_s and 1/Q, since that is the way they would be applied to h(t). Therefore, the zero-crossings of 1/Q show up as asymptotes in the plot of Q. I think it would be better to output 1/Q in a channel rather than Q for this reason.

There is a noticeable ramping up of f_s at the beginning of lock stretches, and the range of values agrees with what has been measured previously.

I've noted that it is quite difficult to resolve the value of Q with good accuracy. These are some reasons I suspect:
1) Higher uncertainty of calibration measurements at low frequency can add a systematic error to the EPICS values computed at 7.93 Hz. This may be why the Q is more often negative than positive ??
2) In the calculation of S_s, the actuation strength is subtracted from the ratio of pcal and DARM_ERR. Since this is such a low frequency, the subtracted values are close to the same value in magnitude and phase. Thus, subtracting magnifies both systematic error and uncertainty.
3) The imaginary part of S_s (see eq. 13, bottom equation) in the denominator, is very close to zero, so small fluctuations (about zero, as it turns out) in 1/Q cause large fluctuations in Q.

These reasons make it difficult to measure Q with this method. The effect of these measured-Q fluctuations on S_s, the factor we would actually apply to h(t) (see eq. 22), is not enormous, so long as we apply the smoothing to 1/Q, as I have done here.
Images attached to this report
Comments related to this report
shivaraj.kandhasamy@LIGO.ORG - 09:16, Monday 27 March 2017 (35105)CAL

First attachment is a hand written note containing derivation of the equations 13 in DCC document T1700106. As Aaron mentioned above, in the derivation the order of the quantities in the sqrt function comes out to be in the opposite order  (Re[S] - abs[S]^2 instead of abs[S]^2 - Re[S]).  The second plot show  the estimation of the four sensing function quantities for 2017-01-24 calibration sweep measurement done at LHO (a-log 33604). Instead of tracking across time here we track across sweep frequencies. The top two plots in the second figure show the estimation of optical gain and cavity pole frequency assuming no detuning. We see that above ~100 Hz we get almost constant values for optical gain and cavity pole frequency suggesting detuning doesn't affect the estimation of those quantities (currently we use 331.9 Hz line at LHO for estimating optical gain and cavity pole). Substituting back the optical gain and cavity pole calculated this way, we then calculated detuning frequency and Q. The bottom two plots of the second figure show those. We see that upto ~60 Hz we can use the lines to estimate detuning frequency (currently at LHO we are running the line at 7.83 Hz). However the Q is hard to estimate, the variation is pretty large (Evan's recent a-log also indicate this 34967; Aaron also finds this to be the case). Also in the 7-10 Hz region its value seems to be negative (need to look at more data to make sure that it not just a fluctuation). With the current set of calibration lines, it seems tracking of detuning frequency would easy but estimating Q might be a little difficult.

Images attached to this comment
Non-image files attached to this comment
shivaraj.kandhasamy@LIGO.ORG - 10:21, Monday 17 April 2017 (35584)

In the second page of the derivation,  at the half way point I have unintentionally switched the notation from S_s to S_c (it should be S_s till the end of the page 2).

aaron.viets@LIGO.ORG - 05:20, Wednesday 07 June 2017 (36692)
[Daniel Finstad, Aaron Viets]

The time series and histograms attached show additional data collected using the DCS calibration pipeline from Jan 19, 2017 at 21:44:14 UTC (GPS 1168897472) until Jan 20, 2017 at 09:02:38 UTC (GPS 1168938176).
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