Displaying reports 42481-42500 of 88684.Go to page Start 2121 2122 2123 2124 2125 2126 2127 2128 2129 End
Reports until 18:25, Monday 18 March 2019
H1 ISC
jenne.driggers@LIGO.ORG - posted 18:25, Monday 18 March 2019 (47616)
Measured MICH and SRCL FF at 35W

Earlier today I took data for redoing the MICH and SRCL feedforward filters, following my instructions from alog 47185.

* Measured MICH FF with both mich and srcl ff off

* Turned on mich ff (feb 28 filter), then measured Srcl ff.

I apparently don't actually understand the nuances of the fitting scripts as well as I thought, so I haven't actually created new filters.  I checked the current coherences of MICH and SRCL with DARM, and they are both quite low (1e-2 level), so they're already fine for now anyway. 

Note that the PRCL coherence is still around 5e-2, so we will want to address this. Hopefully it'll be fixed by the TCS tuning to minimize frequency noise coupling, but if that doesn't work, we may need to consider using the PRCL FF filters.

H1 SYS
jenne.driggers@LIGO.ORG - posted 18:08, Monday 18 March 2019 - last comment - 18:32, Monday 18 March 2019(47622)
SDF diffs / accepts

I am accepting things in SDF, so that we can go to Observe.

Why does IMC-MCL_FM_TRIG_THRESH_[ON/OFF] change?  This filter bank isn't in use after we acquire lock, so it shouldn't matter.  I've reverted to the value that was in both the safe and observe snap files.

We are also leaving on several lines, for monitoring overnight.  Dan's script will kill these if we lose lock.  This does, however, mean that we are *ignoring* excitations in the LSC and ISS models.  We will revert these to being monitored when we are done with this test, end of next week at the absolute latest (i.e. before O3).

To make this work, Dan has made some changes to the TCS guardian, that we likely want to keep anyway. Also, in order to prevent dropping out of Observe, we've not-monitored the CO2 rotation stage go-to-power buttons.

Images attached to this report
Comments related to this report
jenne.driggers@LIGO.ORG - 18:20, Monday 18 March 2019 (47630)

To help us remember what things must be undone before the actual observing run, we have made a large note on the whiteboard in the control room.  As is noted on it, please don't erase this note until these things have been done.

Images attached to this comment
daniel.brown@LIGO.ORG - 18:20, Monday 18 March 2019 (47631)

To adjust the CO2 powers tonight while also remaining in observation mode I have told the TCS guardian not to change the CO2 levels when we are in nominal low noise. The new state looks like this:

class PRE_HEATING(GuardState):
    """Idle state that can go to ADJUSTING_POWER
    if the IFO power is changed. Uses a range  window
    so that the CO2 power isnt adjusting power constantly.
    """
    index = 5

    @fault_checker
    def run(self):
        # Check if the current CO2 power is within
        # some range of where it should be.
        isc_lock_state = ezca[':GRD-ISC_LOCK_STATE_N']
        # Don't adjust CO2 powers whilst in nominal low noise
        if is_co2_out_of_range() and isc_lock_state != 600:
            return 'ADJUSTING_POWER'
        else:
            return True

daniel.brown@LIGO.ORG - 18:32, Monday 18 March 2019 (47636)

Lines that are running [Hz]:

  • 72.3
  • 74.7
  • 76.4
  • 3250
  • 4500

These are run using the script /opt/rtcds/userapps/release/isc/h1/scripts/run_lines.py

This script will start and watch the ISC_LOCK guardian state, if we leave state 600, nominal low noise, then it will switch off the lines and close the excitation points:

LSC-OUTPUT_MTRX_11_9
LSC-MOD_RF9_AM_EXCITATIONEN
LSC-REFL_SERVO_COMEXCEN

If the script is left running it will wait until we are back in state 600 and ramp the lines on and switch on the excitation points above.

It is currently running on a terminal on ZOTWS21, workspace 1.

 

 

H1 General
travis.sadecki@LIGO.ORG - posted 18:00, Monday 18 March 2019 - last comment - 01:03, Tuesday 19 March 2019(47625)
OPS Overview FOM not displaying Observing state

The OPS Overview FOM that displays the Observatory Mode is displaying only a white box when Observing is selected as the mode.  See screenshot.

Images attached to this report
Comments related to this report
thomas.shaffer@LIGO.ORG - 01:03, Tuesday 19 March 2019 (47648)

Fixed.

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H1 General
travis.sadecki@LIGO.ORG - posted 17:53, Monday 18 March 2019 - last comment - 18:41, Monday 18 March 2019(47624)
H1 in Observing at 0:53 UTC
Comments related to this report
travis.sadecki@LIGO.ORG - 18:03, Monday 18 March 2019 (47626)

Commissioning at 1:03 UTC.  Dropped out due to TCS fiddling.

travis.sadecki@LIGO.ORG - 18:06, Monday 18 March 2019 (47627)

Back to Observing 1:06 UTC.

travis.sadecki@LIGO.ORG - 18:09, Monday 18 March 2019 (47628)

Commissioning at 1:09 UTC due to SQZ unlocking.

travis.sadecki@LIGO.ORG - 18:13, Monday 18 March 2019 (47629)

Back to Observing at 1:13 UTC.

travis.sadecki@LIGO.ORG - 18:22, Monday 18 March 2019 (47632)

Commissioning at 1:18 UTC then back to Observing at 1:20 UTC.

travis.sadecki@LIGO.ORG - 18:25, Monday 18 March 2019 (47633)

Commissioning at 1:25 UTC.

travis.sadecki@LIGO.ORG - 18:27, Monday 18 March 2019 (47634)

Observing at 1:27 UTC.

travis.sadecki@LIGO.ORG - 18:29, Monday 18 March 2019 (47635)

Commissioning at 1:29 UTC.

travis.sadecki@LIGO.ORG - 18:34, Monday 18 March 2019 (47637)

Observing at 1:34 UTC.

travis.sadecki@LIGO.ORG - 18:35, Monday 18 March 2019 (47638)

Commissioning at 1:35 UTC.

travis.sadecki@LIGO.ORG - 18:36, Monday 18 March 2019 (47639)

Observing at 1:36 UTC.

travis.sadecki@LIGO.ORG - 18:39, Monday 18 March 2019 (47640)

Commissioning at 1:39 UTC.

travis.sadecki@LIGO.ORG - 18:41, Monday 18 March 2019 (47641)

Observing at 1:41 UTC.

H1 General
travis.sadecki@LIGO.ORG - posted 17:46, Monday 18 March 2019 (47623)
H1 in Observing at 0:42 UTC

Then back to Commissioning at 0:44 due to SQZ Guardian.

H1 CAL
jenne.driggers@LIGO.ORG - posted 16:58, Monday 18 March 2019 (47621)
New inverse sensing function exported, put into CalSVN

Sheila exported our currently-in-use inverse sensing filter, and checked it into the svn.  It is at: /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O3/H1/Measurements/Foton/2019-03-16_H1CALCS_InverseSensingFunction_Foton_SRCD-2N_Gain_tf.txt

We exported the D2N filter, but not the actual gain filter, which has a gain of the order 1e-7.

In the attached figure, I plot the February filter versus the new one.  I have imported the .txt files to make these plots, so we're pretty sure that we've exported the correct filters. 

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 16:36, Monday 18 March 2019 (47620)
external edcu (h1edc) CRC bit now active

FRS12545.

If any of the component HnEPICS_*.ini files used by h1edc to create its full channel list are modified, the CRC bit in h1edc's STATE_WORD will turn red, and its MSGDAQ will report "Modified file detected". In the same way as for real-time front end models, this indicates that a h1edc and DAQ restart is necessary to add/remove the new slow channels to the DAQ.

I wrote a bash script (h1edc_generate_daq_ini_file.bsh) which generates the H1EDC.ini file in exactly the same way h1edc does when it is started. The script runs every minute, as a controls cronjob on h1fescript0. If a modified H1EDC.ini file is generated, the original is archived and the file is updated. The h1edc model then detects the CRC change of this file and raises the CRC condition.

Attached snippet of the CDS overview shows the CRC bit (green square). Note the DAQ bit and DAQ-CRC are still blank until h1edc is added to the DAQ tomorrow.

Images attached to this report
H1 General
edmond.merilh@LIGO.ORG - posted 15:59, Monday 18 March 2019 (47612)
Shift Summary - Day

TITLE: 03/18 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: None
SHIFT SUMMARY:
LOG:

15:54 FIl into CER

16:00  Meeting

16:33 LVEA Sweep - Richard, Betsy, Jenne, and DS

17:15 Robert, Kara, and Sharan out to LVEA - coil

17:30 LVEA Sweep done

17:56 Robert, Kara, and Sharan back

18:22 Dave Barker restarted h1edcu (CDS Overview)

18:35 Patrick and Sheila out to LVEA - ISCT1

19:03 Sheila and Patrick back

19:16 Kara, Sharan, and Robert out to LVEA

20:28 Lockloss - maybe due to PEM group activity in the LVEA

21:56 NLN 96.3Mpc

H1 ISC
sheila.dwyer@LIGO.ORG - posted 15:15, Monday 18 March 2019 (47618)
locking this morning

Ed, Sheila, Jenne, Patrick

We locked at 35W this morning following work done last night reported in 47606 and comments.  

We didn't go to observing, instead PEM injections went ahead, but we tried to do some checks that will make it easier to go into observing soon. 

Images attached to this report
H1 General (DetChar)
betsy.weaver@LIGO.ORG - posted 12:22, Monday 18 March 2019 (47617)
ER14 Sweep #1 performed

This morning, Daniel, Richard, Jenne, and I performed a sweep of the LVEA in prep for logging some ER14 Observation Mode overnight this week.  We did not prep everything for O3 since this and next week are still heavy in PEM injection and Calibration work which need equipment plugged into lots of places.  We also DID NOT do the end stations since we have quite a few Tuesday Maint items at the end stations tomorrow and will perform the list then.  The checklist item status after the morning sweep is as follows:

LVEA Sweep

 


 

VEA Sweep (for End Stations) - NOT DONE TODAY, STILL OK TO GO TO OBS MODE FOR TESTING

Items which required attention this morning, or are noted here as being the configuration for future sweeps:

IN COMPUTER ROOM

NEAR H1 PSL and RACKS

NEAR HAM2/3 RACKS

NEAR Y-arm Manifold

NEAR H2 PSL enclosure

NEAR HAM6 SQZ area

H1 PSL
edmond.merilh@LIGO.ORG - posted 10:02, Monday 18 March 2019 - last comment - 13:12, Monday 18 March 2019(47615)
PSL Weekly Report - 10 Day Trends FAMIS #10601
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edmond.merilh@LIGO.ORG - 13:12, Monday 18 March 2019 (47619)

Here are the same trends created with NDSCOPE. Zooming out automatically shifts to Minute trends and adds the min and max. There isn't a way to turn these traces off currently. The background can be reversed to white. I personally find the black background easier on the eyes.

Images attached to this comment
H1 SEI
edmond.merilh@LIGO.ORG - posted 10:01, Monday 18 March 2019 (47614)
Hepi Pump Trends - Monthly FAMIS# 8321
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