Displaying reports 66321-66340 of 77200.Go to page Start 3313 3314 3315 3316 3317 3318 3319 3320 3321 End
Reports until 08:22, Tuesday 08 April 2014
H1 SYS
daniel.sigg@LIGO.ORG - posted 08:22, Tuesday 08 April 2014 (11191)
Commissioning calendar for next 2 weeks

Here is the list of commissioning task for the next 7-14 days:

Green team:

Red team:

Blue team (ALS WFS):

Blue team (ISCTEY):

SEI/SUS team:

H1 PSL (DetChar, IOO)
laura.nuttall@LIGO.ORG - posted 07:22, Tuesday 08 April 2014 - last comment - 08:33, Friday 11 April 2014(11212)
PSL and IMC ODC look odd
Since Saturday the ODC for the PSL and (obviously) IMC have looked a little odd. They both keeping reporting very short, quick times when both the systems are not 'good'. These happen throughout the day as you can see by the two attached plots which show yesterday's activities (you can see more of these plots on the summary pages - https://ldas-jobs.ligo-wa.caltech.edu/~detchar/summary/). Just wanted to check you knew about this and if so is this nothing to worry about? Thanks! 
Images attached to this report
Comments related to this report
stefan.ballmer@LIGO.ORG - 08:33, Friday 11 April 2014 (11284)
This was another iteration of the ISS actuation running into its range limit.
H1 ISC
sheila.dwyer@LIGO.ORG - posted 19:50, Monday 07 April 2014 - last comment - 10:25, Wednesday 09 April 2014(11211)
ALS work today

Sheila, Chris, Alexa, Stefan

This morning we looked for coherences with many signals with our COMM noise.  There weren't any surprises, we see the same coherence with the end station PDH control signal around 1kHz that we are used to, ISCT1 accelerometers around 70-100Hz, and a little coherence (-0.7-0.9) with the oplevs at low frequencies (pitch at 0.5Hz, yaw around 0.1).  We don't see much coherence at all with the TMS QPDs, just a small bit at low frequencies.  We lose coherence with the in loop sensor below around 100Hz.  

Chris and I went out to End X to look into the beam quality problems.  We didn't find much that was promising.  We checked rather carefully for clipping on the way into the chamber again.  We also set up the nanoscan again, and we see that there really isn't anything coming back to the WFS when the ITM and the ETM are both misaligned (so it isn't a second beam that is directly reflecting a lens or some optic on transmon.)  

We also tried Daniel's suggestion of closing down an iris in the path.  For WFS B this only made things worse.  WFS A scans will be attached to this alog soon, but we didn't get any improvement there either.  

We came back and tried out some of Rich's blends.  We were able to get relatively low noise once without using WFS, 30z down to 0.02 Hz. The attached plot shows the COMM noise (measured by the IR) with different blends on.  We are curently seeing a lot of noise on ETMX T240s at around 3Hz, (100 times more) Rich is looking into this.

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 10:25, Wednesday 09 April 2014 (11242)
Non-image files attached to this comment
H1 AOS
keita.kawabe@LIGO.ORG - posted 18:43, Monday 07 April 2014 (11209)
ISCTEY BS for Hartman sensor installed

Optic is Newport 20B20NC.1 which has a 30min wedge. Since this is in a double path configuration it was not clear which orientation is the best, but I put it in such a way that the beam and the ghost beam going to the chamber separate immediately. OTOH this means that, for the return beam in HWS, PDH and WFS path, the main beam and the ghost crosses at a point 7" after the BS, and then separate. This is because it's easier to block the ghost beam(s) in HWS, PDH and WFS paths than at the back of the periscope.

After the installation of the BS, I used two irises downstream of the 2" PZT mirror to move the 2" PZT mirror position as well as the angle to recover the in-vac QPDs. I further adjusted the 2" PZT mirror and the corner steering mirror between the 1" lens and the 1" PZT mirror to center the beam horizontally on the 2" lens without losing the beam on QPDs.

The optic and the mirror holder were supplied by AOS, had to use lab stock for the post and the base plate.

H1 SEI
stefan.ballmer@LIGO.ORG - posted 17:31, Monday 07 April 2014 (11208)
etmx isi triped while switching blends
This is Sheila, logged in as stefan
Switching blends to test some of Rich's new filter's etmx tripped.  Apparently according to rich this is a know problem, that the filters are incorrectly switched on a zero crossing instead of ramped.  

Guardian has recovered without a hitch.  
Images attached to this report
LHO VE
kyle.ryan@LIGO.ORG - posted 17:07, Monday 07 April 2014 (11207)
Starting Y2 pressure accumulation data collection (early!) -> Expect "RED" alarms on PT424,23 and PT246,45 at some point during excercise
Hard closed GV11 (Bad, abnormal, "clank" from cam mechanism a few seconds before motor stopped) -> portable RGA assembly is valved into Y2 beam tube -> avoid this apparatus (at Y-mid on elevated slab near GV12) 
LHO General
corey.gray@LIGO.ORG - posted 16:03, Monday 07 April 2014 (11206)
Afternoon DAY Ops Summary

Took over for Justin/Pablo at about 2pm to cover the remainder of the shift.  The only new activities I can add are the following:

LHO VE
kyle.ryan@LIGO.ORG - posted 16:00, Monday 07 April 2014 (11205)
~1505 hrs. local -> Used LD to start pumping BSC6 annulus (it was vented)
PT410B seems to have responded, i.e. there looks to be some pressure "communication" via an inner O-ring (perhaps)
H2 SEI (SEI)
mitchell.robinson@LIGO.ORG - posted 15:44, Monday 07 April 2014 (11204)
Staging building, 3IFO (unit 3) progress
Scotty, Mitchell,
The Stage 2 midplate was torqued, inner hex walls added and torqued. The stage 1 Close out plate was added and torqued, the stage 1 close out plate cover was added. No hardware has been added, as there are 405 shcs's and the temp in the cleanroom was 85 which became a good stopping point.
H1 SEI (SEI)
richard.mittleman@LIGO.ORG - posted 15:23, Monday 07 April 2014 (11203)
ETMX Ground Monitor

Aaron put a dongle into the T240 ground monitor electronics to put it into high gain mode, I've  updated the caibration  filters so we should now be getting calibrated ground spectrum

***_STSINF_B_(X,Y,Z)_OUT

LHO General
justin.bergman@LIGO.ORG - posted 13:51, Monday 07 April 2014 (11199)
morning ops

TCS work ongoing in the corner station, mostly along X-arm today

0845 - LVEA transitioned to laser SAFE

1000 - Jodi staging equipment to be removed from LVEA, accessing exterior airlock located in South Bay area. Then Jodi to MY.

1005 - Corey to EX TMS lab for part hunt

1030-115 Beamtube cleaning along X1 by JoeD, ChrisS, ChristinaC (doors left open)

1100 - Jeff/Richard inspecting dust monitor vacuum lines in LVEA

1150 - Dave restarting H1IOPSEIH45

1245 - Karen to EY---advised to tread lightly near BSC10 (Jim working on iso loops)

1250 - LVEA transitioned laser HAZARD

1313 - TCS energizing CO2 laser on TCSX

1315 - Travis on parts hunt LVEA test stand

1400 - OPS handoff to Pablo

H1 ISC
keita.kawabe@LIGO.ORG - posted 13:42, Monday 07 April 2014 (11196)
EY green beam quality is much better than EX

Briefly measured the green return beam on ISCTEY. The first attachment shows the beam profile about 5" or so downstream of the BS that splits WFS and PDH. This is very good, though you might be able to tell that some broad thing is on top of mostly Gaussian main beam.

There are several ghost beams that potentially interfere with the main beam, the closest one being AR reflection from the 1" lens between two MadCityLabs PZT mirrors. The ghost beam is about 3uW in the WFS path while the main beam is 730uW, so this is not that bad, but I'll misalign the lens slightly so that the beam will not come on top of the main beam. The second attachment shows the beam profile of this ghost beam measured at the same position as the first one.

There was also a strong ghost beam coming from the BS to split WFS and PDH path. Total power coming to this BS is about 5.7mW, 5mW goes to PDH and 730 goes to main WFS beam while the ghost beam is about 17uW. This one is shifted in YAW and is easy to block. The third attachment shows this beam measured at the same position as previous two, but the scan head shifted in YAW by about 3mm.

Also there are many many internal reflections coming out of Faraday that  remain there even when the beam path to the chamber is blocked. The total power of these is 115uW. The brightest one is off in PIT but it was easy to block this by using an iris.

Images attached to this report
H1 ISC
stefan.ballmer@LIGO.ORG - posted 13:19, Monday 07 April 2014 (11200)
Control matrix for dither arm alignment
Calculated new output matrices for the IAL arm dither alignment:

Loops to be used:
OSC 1: ITM dither
OCS 3: PZT2 (angular dither at end station)
Loop better not used:
OSC 2: dither PZT1 (~position at the end station, but I don't know how accurately this is true.)

The output matrices are designed to only move the degree of freedom seen by the dither, i.e.
OSC 1:  only drives ITM
OSC 3: drives 1.065*ITM + 1*ETM (PIT) and -1.065*ITM + 1*ETM (YAW)
and for completeness
OSC 2: drives 2.065*ITM + 1.779*ETM (PIT) and 2.065*ITM - 1.779*ETM (YAW)

Calculation:
OSC 3:
- To rotate the beam axis around the end station, the ETM-to-ITM ratio has to be 1-to-gITM.
- The relative signs have to be the same as in the "soft" mode for the WFS output matrix.
OSC 2:
- To parallel-shift beam axis the ETM-to-ITM ratio has to be (1-gETM)-to-(1-gITM).
- Again, the relative signs have to be the same as in the "soft" mode for the WFS output matrix.

H1 PSL (PSL)
justin.bergman@LIGO.ORG - posted 13:08, Monday 07 April 2014 (11198)
PSL Status

I noticed the frontend watchdog was still in FAIL state from last restart---I went into the H1Diode room and reset watchdog.

 

 

Laser Status: 
SysStat is good
Output power is 27.9 W (should be around 30 W)
FRONTEND WATCH is Active
HPO WATCH is red

PMC:
It has been locked 3 days
Reflected power is 1.4 Watts and PowerSum = 11.7 Watts.
(Reflected Power should be <= 10% of PowerSum)

FSS:
It has been locked for 12 min (should be days/weeks)
Threshold on transmitted photo-detector PD = 0.82 V (should be 0.9V)

ISS:
The diffracted power is around 2.54 % (should be 5-15%)
Last saturation event was 13 minutes ago (should be days/weeks)
H1 CDS (VE)
david.barker@LIGO.ORG - posted 12:39, Monday 07 April 2014 (11197)
MEDM sitemap opening from icon bug fixed, added FMCS Fan sensors to SITEMAP

I forgot to define USERAPPS in the sitemap laucher script from icon, this should now be fixed.  You may have to log out and log back in to get the fix (in the mean time start the sitemap from terminal).

I added a link from the VE/FMC pink button to the H0VE_FAN_SENSORS.adl screen.

LHO VE
kyle.ryan@LIGO.ORG - posted 10:40, Monday 07 April 2014 (11195)
Increased voltage of IP9 pump #1 from 3000V to 5000V
Pump #1 was found to be 3000V and pump #2 5000V
H1 SEI
filiberto.clara@LIGO.ORG - posted 09:25, Monday 07 April 2014 (11193)
EY ISI GS-13 Corner 2
Last Friday, Jim W. reported an offset on corner 2 of GS-13. Found BSC ISI Anti-Alias Interface Chassis (S1103401) had one of its outputs railing. AA Board S1101875 had U3 AD8622 on channel 6 replaced. 
H1 SUS
arnaud.pele@LIGO.ORG - posted 18:05, Wednesday 02 April 2014 - last comment - 17:05, Monday 07 April 2014(11141)
ETMY TF running ovenight on opsws3 started @ 17:26:10

will run for ~ 16 hours (undamped / damped for main and reaction chain)

Comments related to this report
mark.barton@LIGO.ORG - 17:05, Monday 07 April 2014 (11202)

FInished when checked 4/7 (Arnaud is away).

M0 undamped: 2014-04-02-1080519986_H1SUSETMY_M0_0p01to50Hz_tf.mat

M0 damped: 2014-04-02-1080537980_H1SUSETMY_M0_0p01to50Hz_tf.mat

R0 undamped: 2014-04-03-1080555846_H1SUSETMY_R0_0p01to50Hz_tf.mat

R0 damped: 2014-04-03-1080573824_H1SUSETMY_R0_0p01to50Hz_tf.mat

Everything looks good except that as usual the R0 cabling has pushed the pitch modes up in frequency.

Comparison plots pending.

Non-image files attached to this comment
H1 SEI
sheila.dwyer@LIGO.ORG - posted 11:10, Friday 28 March 2014 - last comment - 14:28, Monday 07 April 2014(11059)
HAM2 HEPI L4C Trip

Images attached to this report
Comments related to this report
sebastien.biscans@LIGO.ORG - 14:28, Monday 07 April 2014 (11201)

For further record, it's actually HEPI-HAM3

X1 SUS
mark.barton@LIGO.ORG - posted 18:42, Wednesday 26 September 2012 - last comment - 14:47, Monday 07 April 2014(4312)
Taking more BSFM02 TFs
Mark B.

Resuming work on BSFM02. Will take damped and undamped TFs and damped and undamped spectra.
Comments related to this report
mark.barton@LIGO.ORG - 22:19, Wednesday 26 September 2012 (4314)
Mark B.

Done for the day. Undamped TF data is 

2012-09-26_1900_X1SUSBSFM02_M1_*_WhiteNoise.xml, 

and damped TF data is 

2012-09-26_2000_X1SUSBSFM02_M1_*_WhiteNoise.xml . 

Plots for these data set are appended. I've added the appropriate lines to plotallbsfm_tfs.m and committed it but I haven't run it - I want to check that it does the right thing with data taken on H2 but filed as X1.

Spectra time segment starts are

startTimeRef.gps = 1032753893; % GPS Start Time Damping OFF
startTimeRes.gps = 1032752625; % GPS Start Time Damping ON

I still need to generate plots for these and the ones earlier today, but as mentioned previously, first I have to modify plotbsfm_spectraBSFM02.m to accept X1 data (the script it's based on was hard-wired to L1/H1/H2).
Non-image files attached to this comment
mark.barton@LIGO.ORG - 09:47, Thursday 27 September 2012 (4319)
Mark B.

Here the comparison plot with all the BSFM02 data plus some for the real H2 FMY and X2 BSFM06. The noise in the BSFM02 data sets is rather worse than X2 BSFM06 (but comparable to H2 FMY), so it looks like we don't have the best drive parameters. However it does look like noise and there don't seem to be any significant features common to the noisy bits of 2012-09-25_1100 and 2012-09-26_0900.
Non-image files attached to this comment
mark.barton@LIGO.ORG - 16:16, Monday 08 October 2012 (4396)
Mark B.

After some discussion with Stuart, I processed the spectrum data from 7/26/12 morning and evening two ways. First I used a custom plotbsfm_spectraBSFM02.m to process it as X1/BSFM02/BUILD01 with tags of 2012-09-26_0900 (morning) and 2012-09-26_1900 (evening) with names like

^/trunk/BSFM/X1/BSFM02/BUILD01/SAGM*/Results/2012-09-26_*900_X1SUSBSFM02BUILD01H2:SUS-FMY_*.pdf

So if anyone is looking for the data by following the directory structure in the usual fashion for a Phase 1b test, appropriate plots will be there. The captions in these plots also specify X1 BSFM02 primarily and H2 FMY secondarily.

We also used the stock plotbsfm_spectra.m to process the data purely as H2:FMy with names like

^trunk/BSFM/H2/FMY/SAGM*/Results/2012-09-26_1900_H2SUSFMY_*.pdf

This is so that it can be found by the stock version of plotallbsfm_spectra.m, which Stuart felt was too much hassle to customize. We added two new lines to the measList section with comments to the effect that the suspension in each case was really BSFM02.

Attached is a set of comparison plots with the morning and afternoon's data. Unfortunately we couldn't include the 'L1','BS','2012-09-24_1200' dataset because it doesn't seem to have been committed from LLO.

Non-image files attached to this comment
mark.barton@LIGO.ORG - 14:47, Monday 07 April 2014 (11126)

In preparation for the Acceptance review, I redid the TF plots with up-to-date comparisons.

Red: 3IFO Phase 1b undamped (2012-09-26_1900)

Pink: 3IFO Phase 1b damped (2012-09-26_2000)

Black: H1 BS Phase 3b undamped (2013-07-30_1059269030)

Orange: L1 BS Phase 3b undamped (2013-08-29_0900)

Because the data was taken on a mechanical test stand in the LVEA with other work going on around, it is somewhat noisy (especially up to about 0.6 Hz in most DOFs and throughout in P) and the damping is a bit strong, but the peaks in the undamped TFs are very clean and in exactly the right positions.

I also redid the spectra with comparisons.

Green: 3IFO BS 2012-09-26_0900

Red: 3IFO BS 2012-09-26_1900 (later the same day)

Cyan: H1 BS 2013-02-25_1000 (on BSTST test stand)

Purple: H1 BS 2013-07-24_1400

Blue: L1 BS 2013-11-27_0930

Non-image files attached to this comment
Displaying reports 66321-66340 of 77200.Go to page Start 3313 3314 3315 3316 3317 3318 3319 3320 3321 End