Displaying reports 36401-36420 of 89208.Go to page Start 1817 1818 1819 1820 1821 1822 1823 1824 1825 End
Reports until 11:15, Friday 10 January 2020
H1 General
thomas.shaffer@LIGO.ORG - posted 11:15, Friday 10 January 2020 - last comment - 15:56, Friday 10 January 2020(54407)
Lock Loss 1912 UTC

Seemed very fast, no obvious reasons.

Comments related to this report
thomas.shaffer@LIGO.ORG - 15:56, Friday 10 January 2020 (54414)

I didn't get a chance to look into this much, but it was anther fast lockloss. This time it showed up a bit more in LSC_POP_A_LF_OUT, and as usual the OMC DCPDs saw it just before.

Images attached to this comment
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 11:05, Friday 10 January 2020 (54406)
h1nds1 restarted its daqd process

At 10:49 PST the daqd process on h1nds1 restarted itself. This is the default NDS for the workstations.

dmesg reports daqd segfaulted, and then monit restarted the process.

[6728271.848460] dqprod used greatest stack depth: 2928 bytes left
[6728344.956938] dqepics[32031]: segfault at 0 ip (null) sp 00007f7840439fb8 error 14 in daqd-3.2-r4285[400000+8d000]
[6729234.107738] dql8088[32209]: segfault at 8 ip 000000000043acdf sp 00007f5ec3fd0180 error 4 in daqd-3.2-r4285[400000+8d000]

the log file does not show any unusual data requests around this time.

H1 CAL
vladimir.bossilkov@LIGO.ORG - posted 10:13, Friday 10 January 2020 - last comment - 13:00, Friday 10 January 2020(54403)
Issue in Pcal Boards
Since my last aLog on this topic, I have disconnected the temperature sensors and manually run currents across where it was to look for cross coupling, and found that there was none. This leaves me to understand that there is a lot of unknown weirdness on the Pcal board. I did tests where I input current to the Pcal board where the photodiode would be, and found temperature dependances that I would expect to be from just the Resitance of resitor R5 on the boad (board document link is further down this post). This lead me to look into what might be going wrong between the Transimpednace amplifier and the Photodiode - Hence motivating this post.
 
Reading carefully through the spec sheet I noticed that for the Transimpedance amplifer (THS4631) [https://www.ti.com/lit/ds/symlink/ths4631.pdf [Table 1, on page 10]] , the capacitance values of our photo-diode don't really line up with this table, and what our feedback capacitor value is.
 
The stability equation is as follows:
https://alog.ligo-wa.caltech.edu/aLOG/uploads/54403_20200110100238_Stability_Equation.gif
I refer to the board diagram in D1300210-v5.
Where C_F = Required feedback capacitance (C5 on our board, currently 2.7 pf)
R_F = Feedback resistance (R2 on our board, currently 20000 Ohm)
f_GBWP = Unity Gain bandwidth of our Transimpedance Amplifier (first thing listed in spec sheet: 325 MHz)
C_i = the Capacitance of the input (in this case our photo-diode)
 
If our photo-diode has a capacitance of 300 pf (when it has a 5 V voltage across it) - this would evaluate to C_F = 2.7 pf. (You'll have to chase up the spec sheet of the photodiode upon the internet, there is no convenient direct link. The model is C30665GH, and I'm referring to the 2018 version of the spec sheet)
 
*However*, we run our photo-diode in photovoltaic mode where it has better noise characteristics. In this case it actually has a capacitance of 1000 pf - meaning we need C_F = 4.96 pf
 
This should be the last piece in the puzzle with regard to things not understood in our board, and why its doing weird things with rising temperatures. *This currently affects all Pcal instruments (all IFOs)*
Images attached to this report
Comments related to this report
vladimir.bossilkov@LIGO.ORG - 13:00, Friday 10 January 2020 (54408)

If you are reading this in Calibration, and not sure what it means for the IFO and not some hand wavy "temperature dependence study" sence:

Pcal is only ever calibrated at DC frequency (0 Hz).

Having the wrong feedback capacitance introduces frequency dependant response change. Simply: With increasing frequency, the response change will have some non unity magnitude, and is unstable after some frequency.

To understand that change, the system needs to be modelled in a SPICE package.

H1 General
thomas.shaffer@LIGO.ORG - posted 10:05, Friday 10 January 2020 - last comment - 10:08, Friday 10 January 2020(54404)
Out of Observing 1801 UTC Brief Vac VEA Incursion

We will be out for a short bit while the vac team goes into the EY VEA.

WP8510

Comments related to this report
thomas.shaffer@LIGO.ORG - 10:08, Friday 10 January 2020 (54405)

Back to Observing at 1808 UTC

LHO General
corey.gray@LIGO.ORG - posted 08:08, Friday 10 January 2020 (54398)
Owl Shift Summary

TITLE: 01/10 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 56Mpc
INCOMING OPERATOR: TJ
SHIFT SUMMARY:

H1 has been locked 29+hrs & we just rode through an "unannounced" EQ from Mexico.

Tumbleweed status: 

LOG:

LHO General
thomas.shaffer@LIGO.ORG - posted 08:06, Friday 10 January 2020 - last comment - 08:09, Friday 10 January 2020(54400)
Ops Day Shift Transition

TITLE: 01/10 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 118Mpc
OUTGOING OPERATOR: Corey
CURRENT ENVIRONMENT:
    SEI_CONF state: EARTH_QUAKE
    Wind: 13mph Gusts, 10mph 5min avg
    Primary useism: 0.10 μm/s
    Secondary useism: 0.45 μm/s
QUICK SUMMARY: Sudden earthquake from mexico, but is seems to have past. 29 hour lock.

Comments related to this report
thomas.shaffer@LIGO.ORG - 08:09, Friday 10 January 2020 (54401)

Just switched SEI_CONF back to WINDY. The ENV_STAT transitioned back to CALM as well.

LHO General (SQZ)
corey.gray@LIGO.ORG - posted 04:02, Friday 10 January 2020 (54399)
Mid Shift (OWL) Status
H1 AOS
corey.gray@LIGO.ORG - posted 00:14, Friday 10 January 2020 (54397)
Transition to OWL Log

TITLE: 01/10 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 117Mpc
OUTGOING OPERATOR: Jim
CURRENT ENVIRONMENT:
    SEI_CONF state: WINDY
    Wind: 6mph Gusts, 4mph 5min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.35 μm/s

Slight step up in microseism in the last 12hrs (by a factor of ~2, but still under 90th percentile).
QUICK SUMMARY:

H1 General
jim.warner@LIGO.ORG - posted 23:58, Thursday 09 January 2020 (54396)
Shift Summary

TITLE: 01/10 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 120Mpc
INCOMING OPERATOR: Corey
SHIFT SUMMARY: Quiet Shift
LOG:

Nothing to report. Environment is quiet, mostly no one here.
 

LHO General
thomas.shaffer@LIGO.ORG - posted 16:01, Thursday 09 January 2020 (54389)
Ops Day Shift Transition

TITLE: 01/09 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 117Mpc
INCOMING OPERATOR: Jim
SHIFT SUMMARY: Locked for 13 hours, we stepped out of Observing for ~30min for calibration.
LOG:

H1 CAL
jeffrey.kissel@LIGO.ORG - posted 14:22, Thursday 09 January 2020 (54395)
Calibration Measurements: Quick Sensing Function Check Today
J. Kissel

No explorative measurements today -- just a quick, standard, 30 minute check-in with the sensing function. Data and analysis to come.
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O3/H1/Measurements/FullIFOSensingTFs/
    2020-01-09_H1_DARM_OLGTF_LF_SS_5to1100Hz_15min.xml
    2020-01-09_H1_PCALY2DARMTF_LF_SS_5t1100Hz_10min.xml

    2020-01-09_H1_PCALY2DARMTF_BB_3min.xml

Plan to install a new front-end calibration model on Monday, 01/13, so this data set will be processed and included in the presentation materials of that data.
Among the improvements will be to 
 - rid the DELTAL_EXTERNAL / PCAL transfer function (which is representative of the systematic error in the calibration) of the sharp feature at 150 Hz due to previously poor models of the UIM dynamics -- see G2000037. (~3% improvment at 150 Hz, 0.5 % improvement between 10 - 100 Hz.)
 - update the sensing function to better match the current 38W IFO (instead of the 2019-09-09 model, which used data from the O3A 36W IFO). (~0.5 % improvement above ~30 Hz)
 - update to correctly model the O3 ETMX test mass' mass (we've been using the O2 test mass' mass since ... well O2, even though we've replaced the mass) (~0.1% improvement between 20 Hz and 100 Hz.)
Images attached to this report
H1 GRD (ISC, OpsInfo, SUS)
jeffrey.kissel@LIGO.ORG - posted 13:28, Thursday 09 January 2020 (54393)
Unmonitored TMS SDF TEST OFFSETS
S. Dwyer, J. Driggers, J. Kissel, T. Shaffer

We resolved why we've been "having" to recently offload the TMS TEST P and Y offset value (which is currently used for MISALIGNMENT offsets in the SUS gaurdian, INCREASES_FLASHES of the ALS gaurdians, and MOVE_SPOTS in the ISC_LOCK guardian) to the OPTICALIGN offsets upon the arrival in to NOMINAL_LOW_NOISE: (a) you don't *want* to do this offloading [I, Jeff, suggested we needed to do this in error], (b) these TEST offsets get used by enough guardians that we should just un-monitor them in the SDF system.

We've confirmed that the *important* values of these offsets (i.e. the ones that must remain static and don't change between lock stretches) -- the MISALIGNMENT offsets -- are stored in the lsc_params file and forced in place in the DOWN state (and the INCREASES_FLASHES state restores the values it started with).


Thus, there should now longer be anything showing up as an SDF DIFF upon arrival in to nominal low noise.
H1 General
thomas.shaffer@LIGO.ORG - posted 13:24, Thursday 09 January 2020 - last comment - 14:02, Thursday 09 January 2020(54392)
Out of Observing for Calibration 2101 UTC

We will return in around 30min.

Comments related to this report
thomas.shaffer@LIGO.ORG - 14:02, Thursday 09 January 2020 (54394)

Back to Observing at 2136 UTC

H1 CDS (SUS)
david.barker@LIGO.ORG - posted 13:14, Thursday 09 January 2020 (54391)
SUS violin mode gains detailed MEDM

Camilla, TJ, Dave:

The violin mode EPICS IOC was updated to also serve the MAXGAIN values (and VIOLIN_DAMPER.py was modified accordingly to write the max_gains).

The details of the gains are displayed in a new MEDM window H1SUS_VOILIN_MODE_GAINS.adl. This can be opened from the VIOLIN_ALL_MONITORS window via a 'Gains' related display button in the lower right.

The detailed gain window highlights those modes whose gains fall outside of the range defined by NOMINAL and MAX. In this case, a MAX=0 is assumed to have not been set and is ignored.

Images attached to this report
H1 General
camilla.compton@LIGO.ORG - posted 01:09, Thursday 09 January 2020 - last comment - 10:36, Thursday 09 January 2020(54380)
H1 Lockloss 08:48 UTC

Lockloss from a 6.3M EQ in Russia (not far from Alaska) knocked us out of lock fast from EQ mode. 0.03-0.1Hz band nearly touching 20μm/s. Waiting for the ground to calm a little before attempting relocking.

Comments related to this report
camilla.compton@LIGO.ORG - 03:29, Thursday 09 January 2020 (54381)GRD
  • 10:55 NLN
    • I had to offload the TMS offsets from H1:SUS-TMS{X/Y}_M1_TEST_{P/Y}_OFFSET to H1:SUS-TMS{X/Y}_M1_OPTICALIGN_{P/Y}_OFFSET as I did with TJ this morning (alog 54364), and it sounds like Jeff and Cheryl did this afternoon (alog 54376). So I think somewhere in the guardian they arn't being offloaded correctly (tagging GRD).
    • I then turned off the TMS test offsets before reverting them (and the ramp times I changed) in SDF as attached image shows.
  • 11:16 Observing
Images attached to this comment
thomas.shaffer@LIGO.ORG - 10:36, Thursday 09 January 2020 (54388)GRD, ISC, OpsInfo

So it looks like Increase_Flashes has been restoring the TMS TEST bank offsets properly, but ISC_LOCK changes them in ENGAGE_SOFT_LOOPS and MOVE_SPOTS and does not restore the test bank offsets.

Attachment 1 - Showing Incr. Flashes restoring and turning off the TMS offsets in the last lock acquisition.

Attachment 2 - ISC_LOCK moving the TMS and not restoring the offsets.

I'll look next to see why this has changed.

Images attached to this comment
H1 General
jim.warner@LIGO.ORG - posted 00:07, Thursday 09 January 2020 - last comment - 10:43, Thursday 09 January 2020(54376)
Shift Summary

TITLE: 01/09 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Camilla
SHIFT SUMMARY: Violins were a problem early on, quiet after locking
LOG:
When I came, TJ had the IFO sitting while he and Cheryl worked on violins.

5:00 We got to NLN and Jeff and Cheryl had to do the TMS offload again

From 5:00 on we were locked and the IFO was in an Observation ready state, but I thought I had heard Jeff set the Observation bit, somehow I never caught that never actually happened until Camilla came in. Don't know how that happened. So there are about 3 hours here where the IFO was in a good state, just nobody had pushed the button.

Comments related to this report
keita.kawabe@LIGO.ORG - 10:43, Thursday 09 January 2020 (54390)DetChar

Flagging this for DetChar.

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