TITLE: 04/24 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    Wind: 10mph Gusts, 6mph 5min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.27 μm/s
QUICK SUMMARY:

• Mark & Tyler are craning items into the Beer Garden.
• Had to restart video4 & video3. 
• Nuc5's low freq seismic DMT Viewer stuck in 2015 :(
• Verbal Alarm is down.

Thanks to Sheila for the alert.  I suspect something has changed and is pushing on the platform or preventing motion.  I'll inspect and then do some range of motion tests to help find the interference and confirm freedom.

FRS 10483

WP 7491: "Update PLC1 and the system manager on h1ecatc1 to provide remote control of the motorized polarization controller in the MSR through its RS232 interface."

Quick conclusion: The 80MHz EOM calibration is 0.98 rad/V. We are currently modulating the pump light at 0.094 rad.

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The 20dB attenuator at RF power output to the 80MHz EOM (EO-80M3-NIR) was temporary taken off to let the SB show higher on the OPO cavity scan. 12.3 dBm (0.92 Vrms) was measured going into the patch panel. Using Sqrt(Sideband peak/Carrier peak) = J₁(ß)/J₀(ß) gives the modulation depth of 0.9 for 12.3 dBm input power, or 0.98rad/V. 

The RF power going through 20dB attenuator measured -7.84 dBm (0.0906 Vrms). This gives the modulation depth of 0.094 rad and that's how much we're modulating the pump light currently. 

The spec I found in the quote claimed ~16dBm (1.41Vrms) is required for 1 rad modulation for 532nm, off by 3dBm.

Corey, TJ, Thomas Vo, Terry, Dan Brown, Alexei, Sheila

Today we swapped the lenses in the squeezer path for a ROC +250mm lens (1st lens) and a +350 lens (translation stage), both were lenses from the enhanced LIGO squeezer (E1000077) which Corey cleaned this morning.  

When Terry and I swapped the lenses the beam became very misaligned through the squeezer Faraday, so we spent some time re-aligning and then aligning through the apperatures we had placed on HAM6.  To do this we made mechanical adjustments to ZM1 pitch. 

After the PSL crew was done for the day Thomas Dan and I co-alinged the squeezer beam to the interferometer beam very roughly.  (NB, HAM5 HPI has been tripping all evening, so we will need to redo this with HAM5 isolated.)  We were able to close the centering and OMC QPD loops and get a mode scan, results are still being interpreted.

We have removed the apertures we placed in HAM6 this afternoon. 

The turbo pumping CP4 tripped off this afternoon.  As found, the turbo controller was de-energized and the scroll baking pump had isolated itself and remained running.  The power switch for the turbo controller doubles as a circuit breaker and was found in the OFF position.  This switch only has two states ON and OFF as opposed to the more common ON, OFF and "TRIPPED" states ->

None of the power cords appeared to be disturbed and my conclusion is that the turbo had likely tripped due to over temperature.  This pump is surrounded by hot, baking surfaces, has no fan but is, instead, cooled by a local chiller circulating 30C water through its electric motor.  For weeks leading up to today, the relevant temperatures have been non-changing and the turbo has been 80C at its inlet flange and 45C - 48C internally (as per the thermocouple read by the controller).  I think that the internal "trip" threshold is 50C.  Ambient conditions are getting warmer ->

I was able to restart the turbo and reach full RPM while the backing pump remained isolated.  Once at full RPM, I valved-in the baking pump.  Everything seems normal.  As a precaution, I added a small fan and folded back some of the aluminum foil to expose the turbo+RGA hardware and allow some, minimal, convection cooling. 

This morning I valved in the "pressure build circuit" on CP4 Dewar (1/2 turn CCW). The Dewar head pressure is now at 17 psig (just a hair below 16 psig on other gauge) and GN2 flow is back up to ~50 scfhx100 (fluctuates between 40-55), up from 12 scfhx100 this morning. More flow means decreased regen temperature and therefore I also increased the variac today in increments:  58%, then 60%. Attached is 8 hr plot of the GN2 regen temperature - both inlet and exhaust.

Leaving pressure build circuit valved in overnight. Will valve out tomorrow morning before LN2 truck delivery.

14:46 UTC Mark to end Y to retrieve engine hoist for taking doors off BSC chambers
14:51 UTC Chris S. to beer garden to wrap BSC chambers in prep for vent
14:52 UTC Hugh to end Y to top off HEPI fluid
15:24 UTC Hugh leaving end Y
15:29 UTC APS through gate
Chandra to mid Y and end Y
15:46 UTC Reset tripped Beckhoff laser safety interlock
15:47 UTC Nutsinee to HAM6
16:00 UTC Meeting in CR
16:26 UTC Karen to end Y
16:28 UTC Mark taking HEPI fluid barrel to end X
16:49 UTC Hugh to HAM6
16:49 UTC Filiberto to end X to unlock door
h1boot server was down, restarted
17:11 UTC APS through gate
17:11 UTC Vacuum group restarting mid X cold cathode gauges
17:16 UTC TJ to LVEA to get equipment then to optics lab
17:25 UTC Corey to LVEA to get flashlights
17:51 UTC Chandra WP 7501
17:51 UTC Peter to H2 and then H1 PSL enclosure
17:54 UTC Mark moving cleanroom from mid Y to high bay
17:58 UTC Jason to PSL enclosure
18:01 UTC Thomas and Georgia to squeezer bay to take measurements
18:04 UTC Hugh back
18:13 UTC Karen back
18:13 UTC Nutsinee back
18:17 UTC Hugh to HAM6
18:18 UTC Thomas and Georgia back
18:48 UTC TJ back
19:03 UTC Dave to end X to reboot SUS
19:09 UTC Hugh back
19:28 UTC Dave back
19:44 UTC Dave to end X to reboot SUS IO chassis
19:51 UTC Filiberto to LVEA to look for RF cable
20:00 UTC Corey moving nitrogen tank from cleaning area to optics lab
20:07 UTC Jeff B. to LVEA and optics lab
20:10 UTC APS through gate
20:13 UTC Dave back
20:17 UTC TJ to optics lab
20:19 UTC Karen to mid Y
20:36 UTC Hugh to end Y to reset HV and mechanically adjust the trip level of the HEPI fluid reservoir
20:38 UTC Nutsinee to HAM6 to take measurements
20:48 UTC Filiberto to mid X to check on tripped vacuum gauges
20:49 UTC Karen leaving mid Y
21:06 UTC Peter and Jason out for lunch
21:38 UTC TJ back
21:45 UTC TJ to optics lab and then LVEA
21:51 UTC Tyler and Mark moving engine hoist and cleanroom into LVEA through high bay
21:56 UTC TJ back
22:11 UTC Peter and Jason to H1 PSL enclosure
22:11 UTC Corey done in optics lab for the day
22:18 UTC Sheila to HAM6
22:24 UTC Terry to HAM6
22:26 UTC Jeff B. done

Moved the barrel of HEPI Fluid (Thanks Mark & Tyler) to EndX in prep for filter change.  So, topped up the EndY fluid before the barrel was gone.

HEPI & ISI Fully isolated now without issue.

TVo, Patrick

A medm screen for RS232 readout of the TCS chillers has been added to the sitemap for TCS.

Top right TCS on sitemap -> 'CO2X CHILLERS' or 'CO2Y CHILLERS' in light blue.

The supply toggles were still 'On' so this is in response to a VE glitch.

Believe the 16 & 1/2" (C1) and new 2.75" fiber feedthru conflats (D4 2 & 3, see D1002877) are metal to metal now.  Ready for leak check,  later.

I thought to get a head-start on tomorrow's reboots by rebooting h1susey early. After having to power cycle the IO Chassis to regain connection with the computer, the code is now waiting for h1seib3 to restart. So I'm leaving it down for tonight. BTW I restarted the models on h1seiey and h1iscey after they were dolphin glitched.

https://services.ligo-la.caltech.edu/FRS/show_bug.cgi?id=6031

https://dcc.ligo.org/cgi-bin/private/DocDB/ShowDocument?docid=E1600252&version=

We forgot about this modification that was done at LLO, therefore our OMC DCPD dark noise (only 1 stage of whitening, whitening gain = 0dB, HighZ) is still dominated by ADC noise for f<60Hz or so. See attached and compare with LLO plot in https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=27556.

This modification will use the second stage of the OMC DCPD whitening as an anti-whitening such that the stage 1+2 will act as a low-frequency whitening zp([1,500];[10,50]) without amplifying the violin in analog. This way we can enable all stages to get more whitening in low frequency without worrying about violin saturating ADC.

(After the modification, CAL group should make a careful analog measurement.)

Chandra, Dave:

while Chandra is working on CP4, and while MX-X1 cold cathode is trying to reacquire, I have bypassed these channels from sending cell phone texts (emails continue to be sent)

Bypass will expire:
Mon Apr 23 16:40:52 PDT 2018
For channel(s):
    H0:VAC-MX_X1_PT343B_PRESS_TORR
    H0:VAC-MY_CP4_TE253A_REGEN_TEMP_DEGC

Georgia, Robert

This entry gives results from the test discussed by Georgia here: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=41559

Sometimes during PEM injections, we sanity check that external electric fields (like from a lightning strike) do not significantly affect DARM by sneaking into the chamber through a viewport. A repeat of these injections allowed for a comparison of the field measured by the EFM to the test mass motion that has been induced in the past by similar injections. In the past, we only did a single frequency in the bucket - because the integration time to see the signal in DARM was long.

We repeated the injection by placing an insulated plate over the illuminator port of the EX chamber, and driving at 211 Hz with a voltage of about +/- 11 V relative to the chamber. Similar injections have produced an rms DARM signal as high as 1.5e-21 m in the past, though this is variable, and sometimes we can’t integrate long enough to see the injection in DARM.

The figure shows an EFM spectrum for this injection and DARM for a similar injection in the past. The calibration from the log referenced above gives an rms field at 211 Hz of about 1e-5 V/m at the EFM. Assuming similar conditions to those in the past, we get a coupling of about 1.6e-16 meters of DARM motion per V/m measured by the EFM, for this injection configuration. The SNR of the EFM signal for the injection appeared to be nearly ten times greater than the DARM SNR had been during similar injections in the past. Shielding may differ for different injection points, but at least for this port injection, the EFM appears to be more sensitive than DARM.

Armed with the knowledge about the OM3 sign flip, I was able to close the angular loops on the AS WFS DC centering as well as the OMC ASC loops at the same time with the IFO beam.  I had to go pretty far with the alignment sliders on OM1 and OM2 to get the IFO beam back on the QPDs but this seems to let the control loops converge and the alignment offsets are closer to their zero position on OM1 and OM2.  However, I was not able to turn on the integrators but this configuration might be good enough to do an OMC scan. 

The squeezer crew could try to walk the OPO squeezer beam from last night towards this new alignment with the ZMs and try scanning from here, maybe it'll be less noisy with the angular loops closed.

One thing that is a little odd is that there seems to be an oscillation in the power of AS_C_SUM and AS_A/B_SUM, however, none the optics' suspensions seem to be moving excessively and all but one ISI was in isolated state.  HAM5 was the only one in "ISI Damped HEPI Offline" but when I tried to go to "Isolated" the HEPI ACT limit watchdog tripped so I left it alone.  This oscillation occurs both when the AS WFS DC centering loops are open and closed so it might be coming from further upstream of HAM6.  Particularly, it seems like AS_A_DC_PIT is the noisiest of the WFS signals but I don't know where there source is coming from.