Displaying reports 54541-54560 of 86276.Go to page Start 2724 2725 2726 2727 2728 2729 2730 2731 2732 End
Reports until 11:42, Friday 16 December 2016
H1 CDS
david.barker@LIGO.ORG - posted 11:42, Friday 16 December 2016 (32632)
wind chill script

For fun I've written a script to calculate the site windchill now the wind has kicked up. It uses the NOAA formula. The script is called windchill

david.barker@zotws2: windchill
EX temp 20.1(degF) wind 09.0(mph) windchill 09.6(degF)
MX temp 19.4(degF) wind 09.0(mph) windchill 08.8(degF)
CS temp 21.2(degF) wind 08.0(mph) windchill 11.7(degF)
MY temp 19.3(degF) wind 08.0(mph) windchill 09.4(degF)
EY temp 17.8(degF) wind 08.0(mph) windchill 07.6(degF)
 
wind chill average over site 9.4 degF
 
 

H1 DetChar
jeffrey.bartlett@LIGO.ORG - posted 11:39, Friday 16 December 2016 (32631)
Run A2L Script
   At 19:06 (11:06) took advantage of LLO being down to dropped out of Observing to run the A2L script. Back in Observing at 19:18. 
Images attached to this report
H1 OpsInfo
jeffrey.bartlett@LIGO.ORG - posted 09:03, Friday 16 December 2016 (32629)
Accept SDF Diff
   After relocking this morning had an SDF diff for IMC-REFL_SERVO_IN1GAIN. 
Images attached to this report
H1 General
jeffrey.bartlett@LIGO.ORG - posted 08:13, Friday 16 December 2016 (32628)
Ops Day Shift Transition

Ops Shift Transition:12/16/2016, Day Shift 16:00 – 00:00 (08:00 - 16:00) -  UTC (PT)

State of H1: IFO unlocked  
Intent Bit: Commissioning
Weather: Wind is a Light to Gentle Breeze (4- 12 mph), cold and partly cloudy
Primary 0.03 – 0.1Hz: Currently at 0.06um/s and increasing 
Secondary 0.1 – 0.3Hz: Currently at 0.8um/s
Quick Summary: Recovering from Lockloss just before shift change     
Outgoing Operator: Travis
H1 General
travis.sadecki@LIGO.ORG - posted 08:00, Friday 16 December 2016 (32626)
Ops Owl Shift Summary

TITLE: 12/16 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 75.8911Mpc
INCOMING OPERATOR: Jeff
SHIFT SUMMARY:  Smooth sailing for the first 6 hours of shift.  Then a mysterious lockloss, followed by a quick IA, and back to Observing.
LOG:

See previous aLogs for the play-by-play.

15:59 Lockloss.  Cause unknown.  I'll let Jeff investigate and relock.
 

H1 General
travis.sadecki@LIGO.ORG - posted 07:33, Friday 16 December 2016 - last comment - 07:52, Friday 16 December 2016(32625)
Observing at 15:29 UTC

After a quick and painless IA, we are back to Observing.  I had to accept a few more SDF diffs for ECAT systems. Seems oddly similar to Corey's mysterious lockloss followed by ECAT diffs in aLog 32591.  Seen screenshots of accepted SDF diffs.

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 07:52, Friday 16 December 2016 (32627)

Yeah, I was gonna mention that your lockloss sounds similar to the last (2) locklosses for H1 in that everything else seemed to fine (quiet environment & StripTools also looking fine).  Just not sure about the ALS diffs and if they can be a reason for locklosses since the ALS is shut off, but I don't know.  Hmmmm.

H1 General
travis.sadecki@LIGO.ORG - posted 06:15, Friday 16 December 2016 (32624)
Lockloss 14:12 UTC

Cause is yet unknown.  Nothing seemed to ring up on any of the normal FOMs.  Just got a sudden Verbal Alarms notification that the HAM6 ISI WD had tripped.

H1 General
travis.sadecki@LIGO.ORG - posted 04:06, Friday 16 December 2016 (32623)
Ops Owl Mid-shift Summary

Locked for ~22.5 hours.  No issues.

H1 General
travis.sadecki@LIGO.ORG - posted 00:50, Friday 16 December 2016 (32622)
Ops Owl Shift Transition

TITLE: 12/16 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 69.5545Mpc
OUTGOING OPERATOR: Patrick
CURRENT ENVIRONMENT:
    Wind: 10mph Gusts, 8mph 5min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.27 μm/s
QUICK SUMMARY:  Locked in Observing for 19+ hours.  No issues as of yet.
 

LHO General
patrick.thomas@LIGO.ORG - posted 23:49, Thursday 15 December 2016 (32621)
Ops Evening Shift Summary
TITLE: 12/16 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 73.1215Mpc
INCOMING OPERATOR: Travis
SHIFT SUMMARY: No changes to note since mid shift summary. 
LOG:
01:10 UTC Brief notification that HWSX code stopped running.
01:40 UTC Out of observing to run a2l.
01:48 UTC a2l done. No errors reported. Back to observing.
02:04 UTC EY started constantly saturating.
02:44 UTC Out of observing. Changed gain for H1:SUS-ETMY_L2_DAMP_MODE10 from 100 to 0.02. Turned off FM1 and turned on FM9 and FM10 (Settings at Dec 15 2016 08:46:51 UTC from conlog test machine). 4.7kHz mode has come down and saturations have stopped.
02:59 UTC Accepted SDF differences. Back to observing.
03:17 - 03:27 UTC Stepped out of control room.
03:48 UTC Changed phase to damp PI mode 26.
LHO General
patrick.thomas@LIGO.ORG - posted 20:02, Thursday 15 December 2016 - last comment - 23:46, Thursday 15 December 2016(32619)
Ops Evening Mid Shift Summary
Out of observing twice. Once to run a2l and once to damp 4.7kHz violin mode. PI mode 26 started increasing again. This time changing the phase damped it.
Comments related to this report
patrick.thomas@LIGO.ORG - 23:46, Thursday 15 December 2016 (32620)
Attached are coherences before and after running a2l.
Images attached to this comment
H1 SUS
patrick.thomas@LIGO.ORG - posted 18:26, Thursday 15 December 2016 - last comment - 19:04, Thursday 15 December 2016(32616)
constant ETMY saturations
Verbal alarms started alerting that EY was saturating at 02:04 UTC. It has continued since. Attached is a plot of the L3 ESD drive signals for the last 2 hours. They have been growing. Is this the violin mode at 4.7 kHz that Keita and Cheryl were investigating?
Non-image files attached to this report
Comments related to this report
patrick.thomas@LIGO.ORG - 19:01, Thursday 15 December 2016 (32617)
02:44 UTC Out of observing.
Changed gain for H1:SUS-ETMY_L2_DAMP_MODE10 from 100 to 0.02. Turned off FM1 and turned on FM9 and FM10. 4.7kHz mode has come down and saturations have stopped.
02:59 UTC Back to observing.
patrick.thomas@LIGO.ORG - 19:04, Thursday 15 December 2016 (32618)
Accepted SDF differences attached.
Images attached to this comment
LHO General
patrick.thomas@LIGO.ORG - posted 17:06, Thursday 15 December 2016 (32614)
Ops Evening Shift Start
TITLE: 12/16 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 71.2515Mpc
OUTGOING OPERATOR: Cheryl
CURRENT ENVIRONMENT:
    Wind: 0mph Gusts, 0mph 5min avg
    Primary useism: 0.08 μm/s
    Secondary useism: 0.20 μm/s 
QUICK SUMMARY:

Locked for over 11 hours.
H1 General
cheryl.vorvick@LIGO.ORG - posted 15:51, Thursday 15 December 2016 - last comment - 17:35, Thursday 15 December 2016(32609)
Ops Day Summary:

TITLE: 12/15 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 70.0775Mpc
INCOMING OPERATOR: Patrick
SHIFT SUMMARY:

Activities:

Comments related to this report
cheryl.vorvick@LIGO.ORG - 16:27, Thursday 15 December 2016 (32613)

additional activity before I arrived:

  • 17:29UTC - alog 32600 - ETMY violin mode 10 damping switched from 4.7KHz to 1009Hz
  • this was successful in damping the 1009Hz, however the 4.7KHz harmonics are growing, see attached
Images attached to this comment
keita.kawabe@LIGO.ORG - 17:35, Thursday 15 December 2016 (32615)

Just FYI.

The problem of big violin (or any big high-Q resonances) is mostly the saturation of ADC (OMC DCPD) or DAC (mostly ESD).

To tell if whatever peak is too big or not, measure the OMC DCPD A  IN1 and one of the EY ESD output as shown in the attached.

First of all, you see the time series and OMC DCPD is still very far from its ADC ceiling of +-32k, and ESD output is also very far from its ceiling of +-131k, so you don't need to worry about saturations. Note that you need to set the resolution of dataviewer 16384 and observe for at least 10 seconds before making your judgement.

If these things approach the ceiling you need to damp the worst offender, which you identify by looking at the DARM spectrum, or better, by measuring the DCPD_A_IN1 and ESDOUTF_LL_OUT spectrum (second attachment). In this case, even though we already know that it's still safe, you can see that the 4.7kHz mode is the biggest offender. In DCPD it's about 100 cts RMS or 2*sqrt(2)*100 ~300 cts pp, which is totally negligible compared with DC. In ESDOUTF_LL_OUT, it's about 10k cts RMS or ~30k pp.

Images attached to this comment
H1 CAL (CAL)
evan.goetz@LIGO.ORG - posted 19:09, Tuesday 13 December 2016 - last comment - 11:24, Friday 16 December 2016(32542)
Some investigations needed
Looking at a few tasks on the calibration to-do list, I ended up down the rabbit hole. Sadly, it's getting late and will have to return to this tomorrow.

Investigations:

1) Working on fixing the PCAL --> CAL-CS_DELTAL_EXTERNAL calibration (see LHO alog 31994). Kiwamu's original script computed a transfer function accounting for time delays caused by the DAQ and the CAL-CS whitening filter. However, this is already taken into account in the clock cycles delay in the CAL-CS model when adding the sensing and actuation paths. Since CAL-CS corrects for the phase delay caused by AA/AI filtering--analog and digital--using the delayed actuation path, then what one really wants is to correct CAL-CS for the magnitude changes of the AA/AI filtering and any CAL-CS whitening on this channel while also correcting the PCAL_RX_PD channel for the effect of AA and that we also have not applied a filter with two poles at 1 Hz (for the free-mass response):

DELTAL_EXT   W * [Derr/C_foton + A*Dctrl*delay]
---------- = ----------------------------------
PCAL_RX_PD         m * f^2 * AA_a * AA_d

 m     DELTAL_EXT [C_real/C_foton] / [W * abs(AA_a * AA_d * uncompensatedOMCpoles)]
--- = ------------------------------------------------------------------------------
 m                PCAL_RX_PD / [f^2 * AA_a * AA_d]

Note that the correction factors applied in the numerator of the final equation are really only to be applied to the sensing side. However, the corrections are only at high frequency (low-frequency corrections are simply unity), so the numerator term is dominated by the sensing function.

Thus the calibration to be applied is thus:

   [C_real/C_foton] * [f^2 * AA_a * AA_d]
----------------------------------------------
[W * abs(AA_a * AA_d * uncompensatedOMCpoles)]

Unfortunately, this results in a large deviation in phase at higher frequencies (~60 degrees at 1 kHz, see attached figure) while recent measurements using an incorrect calibration filter do not suffer from this large phase deviation. The phase deviation is due to application of the analog and digital AA on the Pcal. Why?

2) I constructed an O2 version of the front-end calibration time delay diagrams based on the model (see attached), but when I look at the GDS correction factors to be applied to the CAL-CS channels, I do not find matching delays. In addition, the values obtained to not mesh with the recent work done at LLO (see LLO alog 29899). This will have to be investigated further tomorrow also.

Images attached to this report
Non-image files attached to this report
Comments related to this report
shivaraj.kandhasamy@LIGO.ORG - 09:59, Thursday 15 December 2016 (32601)CAL

The AA (analog and digital) had to be taken into for DELTAL_EXT also, including their phase. And also we need a cycle advacne for DELTAL_EXT. Attached plot show the same comparison with the mentioned modifications and we see that the old correction factor was good to use. I have also attached the script used to make the plot. Most of these correction factors are calculated in computeSensing.m of DARM model code, so I just get these factors from there.

Images attached to this comment
Non-image files attached to this comment
evan.goetz@LIGO.ORG - 15:03, Thursday 15 December 2016 (32606)
Thanks to Shivaraj for pointing out the 7 clock cycles adjusted the actuation path to have consistent phase with the sensing path, but that a signal measured by back CAL-CS_DELTAL_EXTERNAL would have an apparent delay of 117.6 usec (see PDF attachment to original alog entry above) + 61 usec for the delay between OMC user model and CAL-CS user model. The apparent 117.6 usec on the sensing side is a combination of optical response, AA filtering, and uncompensated, super-Nyquist OMC DCPD poles.

The correct math is as follows:

DELTAL_EXT   W * [Derr/C_foton + A*Dctrl*delay]
---------- = ----------------------------------
PCAL_RX_PD         m * f^2 * AA_a * AA_d

 m     DELTAL_EXT * [C_foton/C_real] / [W * AA_a * AA_d * OMCpoles * OMCtoCALCSdelay * lightTimeDelay * unknownSensingDelay]
--- = -----------------------------------------------------------------------------------------------------------------------
 m                                       sign * PCAL_RX_PD / [f^2 * AA_a * AA_d]


So the calibration transfer function is:

                           [C_foton/C_real] * f^2
-------------------------------------------------------------------------------------------
[W * sign * uncompensatedOMCpoles * OMCtoCALCSdelay * lightTimeDelay * unknownSensingDelay]


A comparison of the new transfer function is attached below. Note that the magnitude is basically unchanged, but there are changes in phase at the ~5 degree level or less from 10 Hz to 1 kHz. The new transfer function is stored at: /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PreER10/H1/Scripts/ControlRoomCalib/pcal2darm_calib.txt.

I also attach a comparison of DTT transfer functions using the old calibration versus the new calibration. The magnitude of the transfer function is basically unchanged. The phase is modestly affected. Unfortunately, since the transfer function wasn't perfect before and it remains imperfect (darn). I saved 2016-11-30_H1_PCAL2DARMTF_4to1200Hz_fasttemplate.xml with the new calibration transfer function.
Images attached to this comment
evan.goetz@LIGO.ORG - 11:24, Friday 16 December 2016 (32630)
The broad-band calibration has also been updated. The transfer function is also created by the same script,
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PreER10/H1/Scripts/ControlRoomCalib/H1_pcal2darm_correction.m

The broad band transfer function is stored at: /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PreER10/H1/Scripts/ControlRoomCalib/caldeltal_calib.txt

I have updated the most recent DTT session with this changed calibration (see attached): /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Measurements/PCAL/2016-11-30_H1_PCAL2DARMTF_BB_5to1000Hz.xml

Note that the DTT session calibrates the DELTAL_EXTERNAL and PCAL_RX_PD channels separately. The PCAL_RX_PD channel is calibrated by zpk([],[1;1],1,"n"); therefore, the DELTAL_EXTERNAL needs to have all the other calibration applied to it:

                           [C_foton/C_real]
-------------------------------------------------------------------------------------------
[W * sign * uncompensatedOMCpoles * OMCtoCALCSdelay * lightTimeDelay * unknownSensingDelay]
Images attached to this comment
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