Displaying reports 69941-69960 of 77084.Go to page Start 3494 3495 3496 3497 3498 3499 3500 3501 3502 End
Reports until 16:08, Wednesday 07 August 2013
LHO General
corey.gray@LIGO.ORG - posted 16:08, Wednesday 07 August 2013 (7375)
Ops Day Summary

EY Oplev pier disassembled (Thomas)

HEPI fluid work at EX (Hugh)

Craning Clean Room "skeleton" in preparation for move to EY (Apollo)

As-Built drawing check of racks at EX & EY (Dave, Jim)

TMS Assy work at EX (Andres, Cheryl, Jeff, Keita)

A couple of big tours of kids (with Dale)

H1 PSL
kiwamu.izumi@LIGO.ORG - posted 14:38, Wednesday 07 August 2013 (7374)
ISS is running but needs further investigation

[Kiwamu with a help from Christina@AEI remotely]

 Today I made some efforts to bring the ISS back on by following an instruction by Christina and made it sort of running --- the loop can be closed by the autolocker but the diffraction power seems bit too high and also the gain seems too low. Certainly the ISS needs further investigations.

 

H1 SUS
betsy.weaver@LIGO.ORG - posted 11:55, Wednesday 07 August 2013 (7373)
H1-ITMx QUAD metal assembly status

Yesterday, after suffering severe brain damage via knocking the massive mechanical test stand numerous times with my head, I managed to connect the balance of the suspension wires between all stages of the ITMx QUAD while mounted to the ISI.  The QUAD is ready for coarse alignment which will take many days before assembling the OSEM control brackets and lacing cables.  Deepak has been helping us with this work, including getting the cable brackets mounted for upcoming testing.

H1 AOS
thomas.vo@LIGO.ORG - posted 11:26, Wednesday 07 August 2013 (7372)
HIFO-Y ETMY Optical Lever
The optical lever for ETMY that was used in the OAT and HIFO-Y has been de-installed and dis-assembled in preparation for the cartridge transfer from BSC6 to BSC10.  The leaner pylon will be placed in storage and an opposite-handed leaner will be used for the H1 optical lever configuration, but the transmitter pylon is transferable so it will stay at the EY until we re-install the H1 optical lever.
H1 CDS
david.barker@LIGO.ORG - posted 09:21, Wednesday 07 August 2013 (7371)
Mechanical Room Vacuum Controls VME booted using new boot server

Late entry for Tues 6th Maintenance.

The Vacuum Controls VME system in the corner station mechanical room (h0vemr) was booted against the new Linux based vxworks boot server as a first test. The plan is to migrate all Vacuum VME sysems from the legacy Sun Solaris boot servers to the new server, at which point the Sun servers can be decommissioned. This will reduce the power and heat loading of the MSR, and remove reliance on an old RAID unit which is showing errors.

H1 IOO
kiwamu.izumi@LIGO.ORG - posted 20:09, Tuesday 06 August 2013 (7369)
IMC started locking fine again

[Stefan, Jamie, Kiwamu]

 After a couple of small tweaks, the IMC came back to the point where it routinely locks.

Since there will be a couple of scheduled measurements tonight for HAM2/HAM3 HEPIs/ISIs/SUSs, we disabled the autolocker so as not to disturb the measurements and also not to drive the FSS crazily.

 

H1 AOS
keita.kawabe@LIGO.ORG - posted 18:21, Tuesday 06 August 2013 - last comment - 00:23, Wednesday 07 August 2013(7368)
TMS tele/table weighed (Corey/Keita)

TMS tele/table was released from the support bridge, stabilizer bars were detached, all on-table cables were installed, and then the entire structure was put on a scale using Genie lift with a TMS lift tooling.

It was measured 79.5kg. Nominally it should be 82 so we'll have to add some masses.

Then we wanted to balance the entire structure on a balance bridge tooling, we had the bridge itself but it turns out that we don't have a special bolt and a pin that provide pivot point for balancing, it seems like all units are still at LLO. We're stuck, so no mating to the SUS today.

Wrote an email to Matt Heinze, if he finds them we'll be back to business.

Comments related to this report
corey.gray@LIGO.ORG - 00:23, Wednesday 07 August 2013 (7370)

As always, all EX TMS photographic progress is documented in Resource Space here:

https://ligoimages.mit.edu/?c=1327

Images attached to this comment
LHO General
patrick.thomas@LIGO.ORG - posted 17:46, Tuesday 06 August 2013 (7367)
plots of dust counts
Attached are plots of dust counts requested from 4 PM August 5 to 4 PM August 6.
Non-image files attached to this report
LHO General
patrick.thomas@LIGO.ORG - posted 17:25, Tuesday 06 August 2013 (7363)
Ops Summary
CP5 filled
Constantly high dust counts in all three OSB optics labs
Jim B. updated the control room CDS workstation GDS tools
09:06 Ace Portable Toilets on site
10:16 spike in dust counts at end Y, possibly coincident with Hugh R. flushing HEPI air lines
Hugh R. reported he could not control medm screens from end Y, had me update HEPI pump control settings from control room
10:21 - 10:30 Cyrus R. reconfiguring and rebooting the mechanical room vacuum VME crate, MR INST AIR went invalid for a short period
10:34 Paradise water delivery
11:13 Hugo P. updating HAM ISI master model
11:49 Hugo P. restarting HAM ISI models, DAQ restarted
H1 IOO
stefan.ballmer@LIGO.ORG - posted 17:22, Tuesday 06 August 2013 (7364)
HIFO-Y IMC noise measurement limited by laser intensity noise (ISS was off)
(Josh Smith, Stefan Ballmer)

We estimated the IMC transmitted frequency noise due to the PSL intensity noise. The intensity noise explains the IMC frequency noise below 80Hz (the light discrepancy is likely due to me using ISS data from today). Interestingly, this noise also explains the HIFO-Y green readout noise between ~6Hz and ~50Hz (alog entry 7216).

At the time of data taking (7/25/2013, 06:23:53 UTC) the ISS was off, i.e. the MC RIN was high (plot 2).

Conversion:

IMC_trans_freq_noise = f0/L*PWR*(2+1+1)/c/mMC2/(2*pi*f)^2 * RIN

where
f0=2.818e14 Hz (red frequency)
L=16.4736 m    (IMC length, one way)
PWR=164 Watt   (Power in the IMC, = 1 Watt * Finesse/pi, Finesse=516)
mMC2=2.9kg     (Mass of MC2 mirror, same as for MC1 and MC2)
(2+1+1)        (effect of MC2 at 0deg, MC1 at 45deg, MC3 at 45deg)
f              (Audio frequency)



Images attached to this report
H1 SEI
hugo.paris@LIGO.ORG - posted 16:16, Tuesday 06 August 2013 (7361)
HAM-ISI - Cart Biases Update Installed

I installed the latest {master model/Medm/scripts} update from Stanford, on the HAM-ISIs (Details, ECR E1300548

This new version features the replacement of local biases with Cartesian Biases for the ISIs.  Doing so allows removing the DC value of the CPS readouts of the error signal (biases use) while still keeping information regarding the platform position, and alignment, in the cartesian basis (which we could not do with the local biases).

Master models, MEDM screens and scripts were updated for the HAM-ISI. Every H1 HAM-ISI model was recomplied and restarted. 

Safe.snap files were updated for HAM2 and HAM3 so the local biases are left off when the model is restarted. Snap files are commited under the SVN (r5268)

the DAQ was restarted.

Everything work as expected. Isolation loops are turned back ON on both HAM2 and HAM3 ISIs. yes

 

Details about svn updates can be found in the attached log.

Work was performed under WP4082, which is now closed.

Updates are ready for installation on BSC-ISI as well. 

Images attached to this report
Non-image files attached to this report
H1 SEI
hugh.radkins@LIGO.ORG - posted 16:15, Tuesday 06 August 2013 (7362)
EndY SEI/HEPI Progress Update
We added fluid to the main line piping today and the fluid is flowing under servo control at 40psi.
LHO VE
kyle.ryan@LIGO.ORG - posted 15:58, Tuesday 06 August 2013 (7360)
Shut down YBM QDP80 pump @ ~1330 hrs. local


			
			
H1 FMP
jodi.fauver@LIGO.ORG - posted 14:11, Tuesday 06 August 2013 (7359)
Y-End Prep
I talked with Richard at Craftsman Flooring today. It appears from the file at Craftsman that we ordered enough material to cover the balance of the VEA floor around the chambers. Bubba knows where at least a partial roll of flooring is (Y-End by emergency exit). So I asked Craftsman to schedule flooring install ASAP, which will be next week. They will call me if they can get here sooner.
H1 PSL
kiwamu.izumi@LIGO.ORG - posted 11:29, Tuesday 06 August 2013 (7357)
bad ISS - autolocker is off for now

It seems that the ISS has been preventing the FSS from locking since yesterday (see alog 7340).sad

I turned off the ISS autolocker for the moment so that we can go ahead with the IMC locking which is one of the main activities recently.

X1 DTS
james.batch@LIGO.ORG - posted 10:58, Tuesday 06 August 2013 (7356)
Updated GDS Version to branch 2.16.5
For the linux-x86_64 workstation, the gds tools have been changed to branch gds-2.16.5 to be consistent with the LHO control room.
H1 CDS
james.batch@LIGO.ORG - posted 10:03, Tuesday 06 August 2013 - last comment - 13:36, Tuesday 06 August 2013(7355)
Updated GDS tools for control room
The gds tools have been updated to branch 2.16.5.  The gds tools include diag, diaggui, chndump, foton, awggui, ezcaread, ezcawrite, ezcaswitch, ezcademod, ezcaservo, ezcastep, and some other utilites.  Here's a list of more significant changes:

GUI programs (diaggui, foton, awggui):

Expand channel field width in fields and menus that display channel names.

Ability to generate .png files for plots (bugzilla 420)

Update to allow more than 128 tp and awg responses from front ends

Release notes viewable from Help menu (if installed)

For foton:

Modify to report in much better detail errors that are encountered when reading a filter file.  Errors reading a file are indicated by changing the File... button to a red color.  When mouse clicking the red File... button, errors are displayed in a popup dialog box.  (see image 1)
Use caution if the File... button is red.  This indicates that saving the filter file will most likely result in some (defective) filters not being saved.

Change matlab merge batch mode to not display any ROOT graphics.  Batch mode foton returns 0 for successful operation or -1 (255) for failure.  Errors will be written to stdout if any are encountered.

Filters with output ramp set with 0 ramp time will be converted to immediate switching with a warning issued to the user.

Foton preserves filters that consist of only gain(1).

For ezcademod, expanded the number of channels it can read to 200,000.  This is inadequate, and is a stop-gap measure which will have a more permanent fix implemented.


Images attached to this report
Comments related to this report
james.batch@LIGO.ORG - 13:36, Tuesday 06 August 2013 (7358)
The Mac OS X gds tools have also been updated.
H1 ISC
jeffrey.kissel@LIGO.ORG - posted 20:29, Thursday 25 July 2013 - last comment - 12:00, Thursday 08 August 2013(7235)
Red Arm Locked with High-Performing SEI/SUS
J. Kissel, H. Paris, A. Pele, B. Shapiro

After spending all afternoon getting all the chambers up into their best (local) performance, I've used Stefan's instructions to lock the Y ARM on Red. So easy -- even I could do it! Thanks to all of those who've written scripts to automate the ALS and IMC :-). Interestingly, and I forgot to ask about it, but there's no need to run any down script when the lock is lost. One just runs the two scripts again (assuming your Beam Splitter alignment remains good).

OK, I wrote the aLOG too soon. There have been several lock stretches, and the ISI-BS has tripped. I detailed time line is written below, for as long as I stayed here.

Here's the configuration of the SEI/SUS during these stretched:

Cavity Lock: 
Chamber    HEPI                                   ISI                               SUS
HAM1       Locked                                 n/a                               n/a
HAM2       Floating, Alignment Offsets Only       Level 2 Isolated                  MC1, MC3, PRM damped Level 1.5; PR3 damped Level 1.0
HAM3       Floating, Alignment Offsets Only       Level 2 Isolated (eLIGO Blends)   MC2, PR2 damped Level 1.5 
BS         Level 2 Isolated (Position Locked)     Level 3 Isolated*                 BS damped Level 2.0
ITMY       Locked                                 Level 3 Isolated                  ITMY damped Level 2.1
ETMY       Level 2 Isolated (Position Locked)     Level 3 Isolated                  ETMY damped Level 2.1, TMSY damped Level 2.0

* I noticed ISI-BS had tripped around 2:53 UTC, but it may have been down for some time. I didn't bother bringing it back up, 'cause I didn't want to blow the cavity lock. Or another three hours.

All Optical Levers are well centered.

All BSC-ISIs have been brought up to the configuration outlined in LHO aLOG 7226, but just for posterity, this means:
Level 3 Isolation Filters
Blends at ST1 "T250mHz" and ST2 "250mHz"
GND to ST1 STS2 Sensor Correction is ON (The corner station ISIs are both using the beer-garden STS2)
ST1 to ST2 T240 Sensor Correction is ON
ST0 to ST1 HEPI L4C Feed-Forward is ON (with "FF01_2" filters)
The Input Gains for the L4Cs and GS13s are OFF (I *think* this means they're in low -gain mode). They're ON for the T240s.

----------
Time Line (all times UTC, Jul 25 2013)
2:27 Locked on Red
2:46 Lost Red Lock
2:47 Regained Red Lock
    2:50 Glitch in CARM_IN1!
    2:53 Noticed ISI-BS had tripped. All other ISIs are still fully operational
    2:57 Glitch in CARM_IN1!
3:00 Lost Red Lock
3:06 Regained Red Lock
    3:11:23 Glitch in CARM_IN1! 
    3:24:47 Glitch in CARM_IN1!
3:27 We begin to ignore the IFO and go home, be cause there's enough data in the can to get a 0.01 [Hz] measurement in the past (assuming those glitches don't spoil the spectra)... but may the lock last through the night!
Comments related to this report
joshua.smith@LIGO.ORG - 11:30, Friday 26 July 2013 (7245)
Josh Smith, Chris Pankow

Hi HIFO-Y folks,

Stefan asked us to look into coherence around the time of the HIFO-Y tests of the past two days. Here we're comparing the data from the 25th in alog 7220 with the one from the 26th in this alog. The most noticeable difference between the two times is that the CARM noise is significantly lower, and nearly the whole effect comes from engaging the PSL ISS. Attached plots are: 

1) CARM noise from 25th compared to CARM noise from 26th.
2) PSL ISS PDA and PDB for 25th -  ISS OFF (sorry for not having this in RIN, will try to update with that info.)
3) PSL ISS PDA and PDB for the 26th - ISS ON
4) Coherence between ISS and CARM for 25th (very high)
5) Coherence between ISS and CARM for 26th (almost none)

Note: o find the clean times we looked at ALS-Y_REFL_B_LF_OUT_DQ and LSC-CARM_IN1_DQ to make sure it was locked and had not glitches. 

Stefan mentioned that this could be from Intensity noise coupling to length/frequency noise in the IMC via radiation pressure. This should not be hard to calculate with the RIN of the PSL, the length and geometry of the MC, and the mirror masses. Is it already in the noise budget? 

We will continue for looking for other systems that have coherence during the quieter time on the 26th. 
Non-image files attached to this comment
joshua.smith@LIGO.ORG - 17:46, Friday 26 July 2013 (7250)
For the lower-noise HIFO-Y time from the 26th in the comment above, the PSL table/periscope accelerometer channels are somewhat coherent with the ratty noise from 100-400Hz (see attached PDF). This is not quite a strong as the coherence with the green laser HIFO-Y signal reported by Robert and co on 7150. In addition to that, the HAM3 GS13s show coherence at 0.4, 1, 3, and 4.2Hz (see second attachment). I also checked MICs, MAGs, TILTs, and L4Cs and didn't find anything to write home about. 
Non-image files attached to this comment
stefan.ballmer@LIGO.ORG - 17:24, Tuesday 06 August 2013 (7365)
vincent.lhuillier@LIGO.ORG - 12:00, Thursday 08 August 2013 (7378)
Lock happens on Jul 26 2013 (UTC)
2:27 Locked on Red
2:46 Lost Red Lock
H1 ISC
stefan.ballmer@LIGO.ORG - posted 01:04, Thursday 25 July 2013 - last comment - 13:35, Sunday 22 September 2013(7215)
Input Mode Cleaner transmitted frequency noise
(Jeff, Kiwamu, Stefan)

With the H1:LSC-REFLAIR_A_RF9_I calibrated in Hz, and the open loop transfer function measured, here is the noise it sees: Input Mode Cleaner transmitted frequency noise.
Also plotted is dark noise (shutter closed).

We do not know yet what the ugly noise ~1/f^3 noise is.
Images attached to this report
Comments related to this report
stefan.ballmer@LIGO.ORG - 01:10, Thursday 25 July 2013 (7217)
The loop transfer functions are attached:

Open loop gains:
CARM_OLG_RED.txt
CARM_OLG_GREEN.txt

Closed loop gains:
CARM_CLG_RED.txt
CARM_CLG_GREEN.txt

Inverse closed loop gains
CARM_iCLG_RED.txt
CARM_iCLG_GREEN.txt


Inverse closed loop gain with a factor of 1/2 gor Green Hz to Red Hz conversion: 
CARM_iCLG_RED_g2r_special.txt
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 10:50, Friday 26 July 2013 (7243)
S. Ballmer, J. Kissel

We had made an estimate for the coil driver noise in low-noise mode (State 3, ACQ off, LP ON), and ruled it out. However, I've checked the state of the Binary IO switches, and MC2 is running in State 2, ACQ ON, LP OFF, and and MC1 and MC3 are running in State 1, ACQ OFF, LP OFF. We'll try for this measurement again, with the coil drivers in their lowest-noise mode.
stefan.ballmer@LIGO.ORG - 17:25, Tuesday 06 August 2013 (7366)
jeffrey.kissel@LIGO.ORG - 13:35, Sunday 22 September 2013 (7825)
I've plotted the above-attached, red and green, open loop gain transfer functions (see *_full.pdf attachment). Through trial and error, I figured out that the text file columns are (freq [Hz], magnitude [dB], phase [deg]). And remember these are IN1/IN2 measurements, so it's a measurement of - G, not G (which is why the phase margin is between the data and 0 [deg], not -180 [deg]). 

Also, because the data points around the UGF were so sparse, I interpolated a 50 point fit around the UGF to get a more precise estimate of the unity crossing and phase margin. See _zoom.pdf for a comparison of the two estimates. I get the following numbers (rounded to the nearest integer) for the raw estimate and the fit estimate:

The raw CARM UGF is: 136 [Hz], with a phase margin of: 33 [deg]
The Fit CARM UGF is: 146 [Hz], with a phase margin of: 30 [deg]
The raw CARM UGF is: 169 [Hz], with a phase margin of: 35 [deg]
The Fit CARM UGF is: 170 [Hz], with a phase margin of: 34 [deg]

Non-image files attached to this comment
Displaying reports 69941-69960 of 77084.Go to page Start 3494 3495 3496 3497 3498 3499 3500 3501 3502 End