Displaying reports 68121-68140 of 77131.Go to page Start 3403 3404 3405 3406 3407 3408 3409 3410 3411 End
Reports until 12:57, Wednesday 15 January 2014
H1 DAQ (CDS)
david.barker@LIGO.ORG - posted 12:57, Wednesday 15 January 2014 (9293)
LHO DAQ Stats

Prior to the pending DAQ upgrade, here are the DAQ stats at the start of ER5.

Frame Look Backs

system

science_frames

commissioning_frames

second_trends

fw0 3 days 22.5 hrs 19 days 8 hrs 8 days 8.5 hrs
fw1 1 day 21 hrs 9 days 4 hrs 3 days 23 hrs

Size of frames and data rates:

Science frames are 32 seconds in length, 308MB size, 9.6MB/s data rate

Commissioning frames are 32 seconds in length, 508MB size, 15.9MB/s data rate

H1 General
jeffrey.bartlett@LIGO.ORG - posted 10:32, Wednesday 15 January 2014 (9291)
Richard in H1-PSL
10:20 Richard working in H1-PSL enclosure.
11:00 Richard finished in H1-PSL enclosure.
 
H1 General
jeffrey.bartlett@LIGO.ORG - posted 09:05, Wednesday 15 January 2014 (9290)
Betsy in LVEA
09:00 Betsy in LVEA, gathering parts.
H1 General
jeffrey.bartlett@LIGO.ORG - posted 09:04, Wednesday 15 January 2014 (9289)
Sheila D
06:30 - 08:15 Sheila working in LVEA.
H1 General
jeffrey.bartlett@LIGO.ORG - posted 08:52, Wednesday 15 January 2014 (9288)
Electrical Work LVEA Roof
08:00 Towsen Electrical on LVEA roof working on lightning protection system.
09:30 John, Richard, and Towsen Ele on LVEA Roof
H1 ISC
sheila.dwyer@LIGO.ORG - posted 08:26, Wednesday 15 January 2014 (9287)
SHG on ISCT1

We have 0.77mW on the IR PD before the SHG, with 30dB of gain we get 0.21 Volts.  With 2k transimpedance this means the responsivity is 0.0041A/W (this seems too low).  We are getting 21mW onto ISCT1 from the PSL, meaning that the BS is 4% reflective, the same value we measured durring HIFO Y. 

21 mW is not enough for us to get a decent amount of conversion to green.  Right now we are getting about 2.5uW of green out of the SHG, not really enough to optimize the alignment.  

H1 ISC
stefan.ballmer@LIGO.ORG - posted 22:10, Tuesday 14 January 2014 (9286)
green arm locking
Koji, Kiwamu, Stefan

- We had some luck locking the xarm today. The best configuration was ITMX ISI State 1, ETMX ISI State 2. However we still had too much arm length motion - slightly more that the 15um that we can tolerate with the 1MHz VCO.
- We tried feeding back to the SUS ETMX top stage, but the speed was too high (every now and then it reached ~30um/sec, which is too fast for relieving through the 0.44Hz pendulum resonance).
- We haven't tried the HPI feed-back, which is currently not wired.

- We tried switching off both ISIs - the fringe velocity was definitely improved, but the alignment was no longer stable enough.

- We also did some alignment tweaking with the IAL system in dither-only mode, but we need better arm stability from the seismic isolation for further commissioning.
H1 PSL
kiwamu.izumi@LIGO.ORG - posted 21:17, Tuesday 14 January 2014 - last comment - 12:07, Wednesday 15 January 2014(9285)
replacement of a BS in PSL completed, ALS and main beam paths realigned.

Koji, Kiwamu with help from Cheryl and JoeD

As a part of the high power preparation, we swapped the beam splitter, IO_MB_M2, from the high transmissive one (T10%) to the low transmissive one (T2%). As expected, this replacement had caused misalignment in both the main and ALS pick off paths. We realigned them. Now the IMC is back to operation and is locking. The ALS beam also successfully comes out to ISCT1.

 

Preparation of the mount and BS:

We started today from peeling the first contacts off from the BSs. We had two identical BSs, one of which was supposed to be a spare. We removed the first contacts from both BSs and found that one showed many residues on the HR surface. Therefore we decided to use the other one which had much less residues and asked Joe to clean a couple of tiny residue off of it. Also, we asked Joe to apply new first contacts on the one which had many residues so that someone can use it for useful purpose in some future.

Cheryl already had Tyler to modify a PSL-custom-made base mount to nicely accommodate a Ultima mirror holder. So we took it from her desk and mount a left-handed 1 inch Ultima equipped with three actuation knobs so that we can control a translation in addition to the usual two angular degrees of freedom. Note that the old BS which had been in place is a 2 inch BS and that's why we needed to swap not only optic itself but also its mount and base.

Alignment of the main path:

The alignment of the main path went very smooth.

Before doing anything, we placed an iris on IOT2L as a reference. It was put before the length diode. After installing the new BS, we realigned the main path using Cheryl's irises on the PSL table. The important and excellent point is that we touched only this particular BS and didn't touch anything else for this alignment. After centering the beam on the irises on the PSL table, we then took a look at the beam on the table. The beam was already landing on the table and in fact it hit the length diode. So we coarsely centered the beam on the diode by steering the BS. At this point, the alignment was good enough for us to lock IMC. A fine alignment was then done by maximizing the IMC power build up. We could get as high power as it used to be in the transmitted light of IMC and hence we were satisfied with this alignment. After turning the ASC loops on, we found that WFSs' DC centering were excellent. I would say this alignment recovery was very successful.

Alignment of the ALS path:

The alignment of the ALS path was not as easy as the main path.

Because the thickness of the BS changed, the beam spot on the first mirror in the ALS path was translated. The translation was so big that the beam was not making through the faraday any more. We tried to recover the alignment without shifting the position of the Faraday and by touching the first steering mirror, but it turned out that it was quite difficult to do it. So eventually, we decided to shift the Faraday. The first steering mirror was steered so that the beam hits the center of the next steering mirror. Then we moved the Faraday, which is between the first and second mirrors, so that the beam goes through it. The transmissivity of the Faraday was measured to be approximately 94% (= 24.50 mW / 26.03 mW) which is acceptable. The we tweaked the second and third mirrors to steer the beam on an iris on ISCT1. After the tweak was done, we assessed the risk of clipping by introducing a large angle misalignment in the third steering mirror and confirmed that the beam is in the middle of the clipping aperture.

Comments related to this report
kiwamu.izumi@LIGO.ORG - 12:07, Wednesday 15 January 2014 (9292)

Before:

After:

Some more pictures are available on ResourceSpace: https://ligoimages.mit.edu/?c=1433

Images attached to this comment
H1 ISC
sheila.dwyer@LIGO.ORG - posted 18:24, Tuesday 14 January 2014 - last comment - 19:06, Tuesday 14 January 2014(9281)
X arm work today

Alexa, Keita, Sheila, Daniel,

Starting with yesterday's alingment alog 9230, I found some flashing this morning using the transmitted PD.  This lead to a clearly visible 00 mode on the ETM camera.  The final alingments we ended up with are in the attached screenshots. 

The trans PD (ALS COMM) has flashes up to 400 counts, which means that we have about 35 uW (a factor of 10 more than the single shot beam). The refl PD drops from about 19000 counts to about 16000 when the cavity is locked to the 00 mode.  There is also a 02 mode that has about 200 counts in transmission, so about half the power of the 00 mode. 

It seems as though all the previous alingments where we thought we had fringing were red herrings.  I moved the camera on ISCT1 (now using a lens and letting the beam hit a baffle) so that the single shot beam is no longer visible but you can clearly see the cavity modes. 

Since the locking was so unstable we thought of trying to feedback to HEPI as was done in HIFO-Y.  However, the IPC from the SUS to HEPI has been deleted. We either need to add it back or add an IPC directly from the LSC model to HEPI.  Hugo is working on it.   However, the situation that we have seems worse than in HIFO Y, there we would run out of range after tens of minutes, today we are running out of VCO range every few seconds.  Also, we get about 5 fringes per second, which if it is due to motion of the optic would mean 1um per second motion.  We need to investigate if the optics are really moving this much. 

Alexa and I went to the end station to look at what was saturating (we are exceeding the VCO input range it seems).  While we were there we also had a look at the IQ scatter plot on the scope.  One thing is that there is approximately the same amount of signal in I as Q, so this is not a usefull way to try to tune the demod phase.  Keita came out and we tried to measure the transfer function from the laser frequency to the demodeulated signals, however we could not because the lock was not stable enough.  We also tried to adjust the demod phase while watching the open loop TF, this also wasn't sucessfull because the loop did not stay locked long enough for us to get repeatable measurements.  

Alexa and I also looked at the residual AM by misaligning the ITM and looking at the output of the PD.  With the ITM misalinged, we have -33dBm of residal AM at the input to the demod, with it aligned we get some thing around -17dBm. 

Stefan is currently investigating the ISI performance. 

Images attached to this report
Comments related to this report
keita.kawabe@LIGO.ORG - 19:06, Tuesday 14 January 2014 (9284)

We started turning off ISI isolation to see how good or bad the length isolation is, and attached is the comparison of ISI isolation for both ITMX and ETMX ON (dashed lines) VS OFF (solid lines).

On: 2014/01/15 01:03:37 UTC

Off: 2014/01/15 02:31:55 UTC

We haven't looked at the seismometer, but just by looking at the fringe moving around it was obvious that ISI isolation makes the low frequency length motion much, much larger, and both SUS BOSEMS (left bottom) as well as the ISI CPS (left top) confirm this.

This looks too bad to be true, I guess ISI might have been in some bogus state when they were supposed to be in level 1 isolation.

OTOH, when ISI isolation was on the angular motion was smaller, and the oplevs (right, top=ETM, bottom=ITM) show that the problem was mostly in EX at about 0.4-0.5Hz. Again the same caveat (we're not looking at seismometer) applies.

Stefan is still playing with all available ISI isolation levels to in a hope to find a good compromise.

Images attached to this comment
H1 SEI
hugh.radkins@LIGO.ORG - posted 17:51, Tuesday 14 January 2014 (9283)
SEI work at WHAM4--Problems with Sensor signals getting to model

We left the LVEA around 3:30 after chasing GS13 signals.  EE/CDS drove our sensor cables at the AA & Interface chasses and confirmed we have signals coming out.  We find now that the HI ISI HAM4 model is incorrect according to the wiring (D1000298.)  Except for the expected difference regarding CPS on HAM2 & 3, the models match.  However, the GS13 & L4C wiring is different.  So we have to change the model or change the wiring.   At the moment we have just H2, V2 & H3 sensor on the ISI plugged in.  We'll continue when the wiring/model gets sorted.

H1 CDS
david.barker@LIGO.ORG - posted 17:41, Tuesday 14 January 2014 (9282)
electronics work on ISI HAM4 IO Chassis

Richard, Filiburto, Hugh, Hugo, Dave

In order to track ISI HAM4 signal issues we injected signals into the AA chassis for h1seih45 for GS13 V1,H1,V3,H3 (first two ADC cards of this IOChassis). Signals were tracked through the IOP and h1isiham4 models. Hugo is checking the model against the wiring diagram.

H1 AOS
sheila.dwyer@LIGO.ORG - posted 17:30, Tuesday 14 January 2014 (9280)
End X activity done for the day

Keita, Alexa and I have returned from end X

H1 ISC
alexan.staley@LIGO.ORG - posted 16:24, Tuesday 14 January 2014 (9278)
offset zeroing script for QPSs

Added an offset zeroing script for QPDs to the svn: asc/common/scripts/setQPDoffsets (SVN revision 6861).

It uses tdsavg to set the four segments to zero, and sets an offset of 4 counts into the sum filter module to avoid a division by zero.

Preconditions: no light on diodes, segment gains have to be -1

LHO General
patrick.thomas@LIGO.ORG - posted 16:01, Tuesday 14 January 2014 (9265)
Ops Summary
Tumbleweed bailing on X arm
10:07 - 10:28 Apollo moving contents of garbing room from West bay to HAM4 (by hand) (WP 4393)
10:54 Site water sample collecting
11:30 Lightning rod work
13:29 Sheila working at end X
H1 General
patrick.thomas@LIGO.ORG - posted 13:24, Tuesday 14 January 2014 (9276)
Mitchel, Hugh starting work on HAM4


			
			
H1 DAQ (CDS)
david.barker@LIGO.ORG - posted 13:02, Tuesday 14 January 2014 (9275)
DAQ Restart, new Beckhoff X1 PLC3 channel list

12:51 DAQ restart, new channel list for H1EDCU_ECATX1PLC3.ini for Thomas' ring heater changes.

I modified the mod_ini scripts to arrange channels in alphabetical order so we actually got new H1EDCU_ECATXXPLCX.ini files for all systems (new channel order) but only H1EDCU_ECATX1PLC3.ini had new/removed channels.

New ini files committed to svn, version 6859.

H1 PSL
patrick.thomas@LIGO.ORG - posted 09:49, Tuesday 14 January 2014 - last comment - 13:32, Tuesday 14 January 2014(9260)
Kiwamu, Koji replacing beam splitter on H1 PSL table


			
			
Comments related to this report
patrick.thomas@LIGO.ORG - 13:32, Tuesday 14 January 2014 (9277)
Breaking for lunch
H1 ISC
alexan.staley@LIGO.ORG - posted 19:27, Monday 13 January 2014 - last comment - 17:29, Tuesday 14 January 2014(9251)
EX PLL measurements

(Alexa, Daniel, Sheila)

PLL Beatnote:

PLL Open Loop Transfer Function:

PLL Noise Spectrum -- via IMON of PFD (S1000758)

PLL Servo Board Transfer Function:

 

Shot Noise of PLL BBPD:

Non-image files attached to this report
Comments related to this report
alexan.staley@LIGO.ORG - 17:29, Tuesday 14 January 2014 (9279)

The missing SR785 measurement:

PLL Open Loop Transfer Function:

Input 1 pol: NEG, Common Compensation: ON, Generic Filter: ON, Fast Option: ON, Fast Gain: -8dB, Input 1 Gain: 0db, Boost 1:ON rest OFF

  • EX_PLL_OpenLoopTFmag_BoostON
Non-image files attached to this comment
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