Displaying reports 68021-68040 of 77131.Go to page Start 3398 3399 3400 3401 3402 3403 3404 3405 3406 End
Reports until 12:39, Monday 20 January 2014
H1 ISC
stefan.ballmer@LIGO.ORG - posted 12:39, Monday 20 January 2014 (9392)
Added an xarm initial alignment (IAL) relieve script
For now it relieves the IAL drive to top mass lock filter banks.

asc/h1/scripts/xarm_IALrelieve
SVN revision 6911
H1 ISC
stefan.ballmer@LIGO.ORG - posted 16:10, Sunday 19 January 2014 (9391)
12h with the x-arm alignment loops on
I had left the IAL dither loops running for the last 12h. There is still frequent mode-hopping to the 10 mode. But when It jumps on the 00 mode, the x-arm build-up in transmission seems to consistently be up to 650 cts.

Images attached to this report
H1 ISC
stefan.ballmer@LIGO.ORG - posted 02:46, Sunday 19 January 2014 (9390)
BS Y2Y and PRM P2P and Y2Y
The BS Y2Y coupling measurement finished and was saved in controls/sballmer/20140115/BSTFdata/BSTFyaw.xml

The PRM P2P coupling measurement finished and was saved in controls/kizumi/binary_stars/20140116_PRMdiag/PRM_P2P.xml

The PRM Y2Y coupling measurement was started. It is now at 0.7Hz and running. It was temporarily saved in controls/kizumi/binary_stars/20140116_PRMdiag/PRM_Y2Y.xml
H1 ISC
stefan.ballmer@LIGO.ORG - posted 02:37, Sunday 19 January 2014 (9389)
Inital Alignment (IAL) for X arm commissioned
I tuned the dither alignment for the x-arm tonight.

YAW:
 - Dithering PZT1 at 410Hz using oscillator 2. Driving ETM using control bank 2.
 - Dithering PZT2 at 470Hz using oscillator 3. Driving TMS using control bank 3.
 - Oscillator 1 and control bank 1 are currently not used.

PIT:
 - Dithering PZT1 at 380Hz using oscillator 2. Currently not driving anything.
 - Dithering PZT2 at 440Hz using oscillator 3. Driving TMS using control bank 3.
 - Dithering ETMX at 1.7Hz using oscillator 1. Driving ETM using control bank 1.


I didn't use the PZT1 pitch dither because there is a DC offset in the demodulated error signal. Note that PZT1 is input pointing position (PZT2 is angle).
I was able to zero the dither offset byputting offsets into the green QPDs:
H1:ALS-X_QPD_A_PIT_OFFSET = -0.464
H1:ALS-X_QPD_B_PIT_OFFSET = -0.084
Those offsets were chosen such that they only lead to a different PZT1 drive, leaving PZT2 untouched.

Attached is a snapshot of all relevant screens.

Still to do:
 - Relieve script or servo (or move integrators to the suspensions).
 - Automatic turn-off of the servo if the arm power drops below a threshold.
 - Actuation node dither for ITM centring. (I would prefer less mode-hopping for this.)
Images attached to this report
H1 ISC
stefan.ballmer@LIGO.ORG - posted 22:54, Saturday 18 January 2014 (9387)
Choice of x-arm modulation frequency
Sheila, Stefan

The low-finesse in the green cavity poses a problem for stabilizing the x-arm length:
 - The PDH error signals of 00-mode and 01-mode overlap.
 - Alignment fluctuations lead (to the first non-trivial order) to a fluctuation in 01-mode power. I.e. the relative contribution of the 10-mode-PDH-signal to the main PDH-signal varies.
 - If the 10-mode-PDH-signal at the main locking point is non-zero, this will couple into frequency fluctuations (relative between arm length and green light). These can be a significant fraction of the line width (about 1.5kHz ?).
 - To avoid this we need the 10-mode-PDH-signal to have a co-located zero-crossing, leading to only gain modulation, but no frequency fluctuations.

 - I can think of two strategies to achieve that:
   1) Set the modulation frequency to exactly 1 transverse mode spacing off the resonance. This lines up the zero-crossings of the PDH signals.
      Setting the demodulation phase exactly will guarantee that the large q-signal does not couple.
      Disadvantages: - The slope of the 10-mode-PDH-signal is large, leading to large gain fluctuations, and requiring an exact knowledge of the transverse mode spacing. (Problem with thermal heating later on?)
                     - The q-signal is maximal - setting the demod phase accurately is crucial.
   2) Pick the modulation frequency at some different value, but set the demod phase such that on the locking point the contribution of the 10-mode-PDH-signal is zero. This will need some more modeling.

For now we chose solution 1): We set the modulation frequency to 24.424281MHz (5099Hz below the co-resonant point of 24.429380MHz). 5099Hz is our current best guess of the transverse mode spaceing - we will need to measure that accurately. Using our phasing table from alog 9386, we set the delay phase shifter to 18.8125nsec (switches up: 1/16, 1/4, 1/2, 2, 16; down: 1/8, 1, 2, 4). As expected, when locked on the 00-mode, we now get a big q-phase offset.
H1 ISC
stefan.ballmer@LIGO.ORG - posted 22:31, Saturday 18 January 2014 - last comment - 23:32, Saturday 18 January 2014(9386)
Setting the demod phase for the x-arm
Sheila, Stefan

The low-finesse cavity made it non-trivial to set the demod phase correctly. Today we used the trick that any Q-signal disappears when the side-band is exactly anti-resonant. We then made an interpolation table to set the phase accurately within about 0.5nsec (~5deg) at any frequency.

1) First we identified the frequencies at which side-band and carrier are co-resonant (no demod signal):
   The 621st co-resonance we found experimentally at 23'303'644Hz, the 681st co-resonance at 25'555'116Hz. Fitting this to line up we get an FSR of about 37525.93Hz +-0.1Hz, or an arm length of 3994.47m +-1cm. Compare this to Daniel's alog: 3994.485m. (And I swear I did the error analysis before seeing Daniel's number.)

2) Next we hit the frequencies where the side-band is exactly anti-resonant, and phased the signal there. The delay numbers correspond to the phase shifter setting, assuming the delay is in with the switch up (i.e. 16.5nsec = 16sec and 1/2nsec switches up, rest down).
   23.922799MHz    31.5000nsec
   24.147946MHz    26.5000nsec
   24.260520MHz    23.3125nsec
   24.373093MHz    20.0000nsec
   24.448142MHz    18.1875nsec
   24.560716MHz    15.5000nsec
   24.785863MHz    10.5000nsec

Comments related to this report
daniel.sigg@LIGO.ORG - 23:32, Saturday 18 January 2014 (9388)

No, it isn't. The true front panel.

H1 ISC (SYS)
daniel.sigg@LIGO.ORG - posted 21:31, Saturday 18 January 2014 - last comment - 14:17, Tuesday 21 January 2014(9385)
X-arm Cavity Length

Doc D0901920 lists the cavity length as 3994.485 m (as built, anyone?). The attached Mathematica snipped calculates the axial location of the sidebands.

Non-image files attached to this report
Comments related to this report
daniel.sigg@LIGO.ORG - 12:51, Tuesday 21 January 2014 (9402)

The as-built distance for the X-arm cavity according to IA (Jason & Doug) is 3994.472 ± 0.004 m.

douglas.cook@LIGO.ORG - 14:17, Tuesday 21 January 2014 (9403)
I would like to get an accurate X arm cavity length measurement when we do a cavity characterization. I have ask JAX if she had some time for this after we pump down. She did this during the HIFOy test. This along with the survey as built numbers would help verify the BTVE-8 (gold standard) monument position at the X-end station with its relationship to the BTVE-5 in the corner station. We would incorporate data from the ITMx survey monuments based on their as built position to the BTVE-5. We would possibly gain a more accurate measurement of the distance between the BTVE monuments for the future.
H1 ISC
koji.arai@LIGO.ORG - posted 21:26, Saturday 18 January 2014 - last comment - 19:45, Thursday 30 January 2014(9384)
Simulation of Xgreen PDH signal

Written by Yuta, posted by Koji, while he is waiting for renewal of his ligo.org account:


In the entry alog #9381, Sheila explained how the PDH signal is distorted by the broadened resonance
of the higher-order modes
due to low finesse of the cavity.

Here in this entry I explain how the shape of the PDH signal can be modified by changing the sideband frequency.

[Motivation]
ETMX transission for green was larger than designed(designed:5% -> measured:36%) and cavity length lock does not stay long.
The PDH signal looks strange(see alog #9381). To explain the situation and see how we can improve the PDH signal,
we calculated PDH signal including HOMs.

[Method]
1. Calculate PDH signal including the effect of carrier HOMs and sideband HOMs.
2. Change sideband frequency to see how PDH signal changes.

The parameters I used are the same as the ones listed in alog #9381.

Calculated TMS is 5.076kHz and the sideband frequency before we have changed last night was 24.407079MHz.
HOM content and vertical scale are arbitary in the following plots.

[Result]
1. HOMPDH_sb24_4MHz.png and HOMPDHIQ_sb24_4MHz.png show the calculated transmission, PDH signals,
and XY plot of I-phase and Q-phase PDH signals, when the sideband frequency was set to the original value. This
IQ plot is very similar to what we have seen(see video in alog #9381) and agrees well with Sheila's calculation.

2. HOMPDH_sbonres+0_5TMS.png and HOMPDHIQ_sbonres+0_5TMS.png are the plots when one of the sideband
is at the middle of the TEM00 and TEM01/10 resonances. PDH signal gives zero crossing at TEM00 resonances,
but it also gives zero crossing at other HOMs. So, mode hopping rate is expected to be high.

3. HOMPDH_sbonres+TMS.png and HOMPDHIQ_sbonres+TMS.png are the plots when one of the sideband is
at the TEM10/01 resonance. PDH signal does not give zero crossing at TEM00 resonances, but if the correct offset
is given, mode hopping rate should be low. The IQ plot will be somewhat simple "8" shaped plot in this case.

See alog #9379 for what we have done using these results.

Images attached to this report
Comments related to this report
paul.fulda@LIGO.ORG - 19:45, Thursday 30 January 2014 (9690)

Written by Yuta



Calculation on demodulation phase dependence was done. See also alog #9429.
Requirement for the demodulation phase adjustment, TMS measurement and mirror alignment fluctuation to achieve frequency noise of few Hz are;

demod phase error < ~ 5deg
TMS measurement error < ~ 5% (~250 Hz)
mirror alignment fluctuation < ~0.3 urad


[Method]
1. Fix sideband frequency at the middle of the TEM00 and TEM01/10 resonances and calculate PDH slope and offset at 00 resonance for various demodulation phases.

2. Calculate PDH signal when the demodulation phase is set so that PDH offset will be zero at 00 resonance (see alog #9384).

3. Calculate zero crossing point of PDH signal dependence on differential cavity mirror misalignment (see alog #9429) when demodulation phase is off by 5 deg (see alog #9386) from the phase where the PDH offset is zero.

4. Repeat 3 by slightly changing the sideband frequency.

[Result]
1. misPDHdemod.png shows PDH slope and offset vs demod phase. Note that demodulation phase which maximizes the slope is different from the phase which minimizes the offset. The phase which minimizes the offset does not depend on TEM01/10 content, but the slope does.

2. misHOMPDH.png shows PDH signal when the demodulation phase is set so that PDH offset will be zero at 00 resonance.

3. zerocrossingPDH_5deg.png shows PDH zero crossing point shift by differential mirror misalignment when demodulation phase is off by 5 deg.

4. zerocrossingPDH_5deg_5percent.png shows PDH zero crossing point shift by differential mirror misalignment when demodulation phase is off by 5 deg and TMS measurement 5% wrong (worst combination).

[Discussion]
1. Assuming we can adjust the demodulation phase within ~5deg to minimize PDH offset by misalignment, measure TMS at <5% precision and alignment fluctuation is <~0.3 urad, misalingment induced frequency noise is smaller than few Hz.

2. The PDH signal looks nice when sideband is at the middle of the TEM00 and TEM01/10 resonances. It has about TMS of linear range and the range symmetric (compare with alog #9384).

Images attached to this comment
H1 SUS (ISC)
kiwamu.izumi@LIGO.ORG - posted 18:12, Saturday 18 January 2014 (9383)
BS L to P correction filter installed

Stefan, Koji, Kiwamu,

We newly installed a L2P correction filter on BS which reduces the coupling to the bottom stage pitching from the penultimate length actuator drive.

Stefan completed the L to P and P to P measurements on BS yesterday. Then Koji fitted the data using LISO and I punched in the fitted poles and zeros of the ratio L2P/P2P in foton and loaded the filter in M2_DRIVEALIGN_L2P. We did a quick test in which we had a big excitation in the M2 length drive and monitored the pitch motion by the oplev with and without the L2P correction. It looked successful although we did this test at only two frequencies, namely 1.1 and 0.8 Hz, because a Y to Y measurement was running in background which we didn't want to screw up at that moment. The coupling looked successfully reduced at least by a factor of 10 at both frequencies as far as we can observe it on a StripTool screen. Note that in order to get the cancelation right, the gain of the L2P  correction chain needs to be -1. If one wants to further test the performance, he or she should run a swept since measurement extensively.

* * *  the L2P correction filter * * *

- - - - freq [Hz]   Q - - - - - -
pole 0.3737768342347  3.4267960418
pole 0.4822474954282  7.0937407121
pole 1.1164786260     9.7341833818
pole 2.1443263848     3.2444753770

zero 0.4313822619174  2.1809027959
zero 0.7477704984560 224.3944177073
zero 1.7628959088     1.1355062310

gain factor -0.0108000650535
H1 ISC
sheila.dwyer@LIGO.ORG - posted 16:46, Saturday 18 January 2014 (9381)
PDH signals from low finesse arm cavity confused by higher order modes

With the difficulty we had been having locking the green arm stably, there was some speculation about what the difference in the ETM transmission from the design of 5% would mean for our locking.  Here are a few plots of pdh signals and resonance profiles for the cavity we have. 

First, the IQ scatter plot we see doesn't look anything like a PDH signal I am used to.  There was some speculation that this is caused by Doppler fringing.  Using the equation 20 from P000017 the critical velocity for doppler effects with our etm is 200um/second, (about 800 fringes per second!) so we were never in this regime.  (if the transmission of the ETM was 5%, this velocity would have been 3um second, which would have been reasonable with the motion that we had on thursday and before)  Since Hugh's changes to the ISIs yesterday we are seeing about 3 fringes/ second when it is fast, (more often 1 or 2 fringes) so our cavity length is changing at about 0.8um/second at most.

Here  is an IQ plot of the PDH signals (units not meaningful) for an ETM transmission of 1% (normal looking), 5% (lobes from sidebands are becoming large) and 38% (our situation).  

Even though that looks strange, it still seems like an OK signal for locking to if the demod phase is tuned correctly: Plot  (In this plot I have used a different demod phase for the low finesse cavity than the one showing the design)

We also have been wondering how we are going to measure the modulation depth, since we do not have an OSA that works for green light.  At some point we tried to lock on a sideband to have a look at the transmitted power relative to the 00 mode.  The power we saw would have suggested a ridiculously high modulation depth.  I believe that we might have been fooled by the camera image and were really locked onto a first order mode.

Keita suggested that I check if we really lock to the side band resonance when by flipping the sign of our servo.  We would if the demod phase is tuned correctly and we didn't have higher order modes. Plot  (This plot shows the shape of the resonance profiles for the carrier and each sideband against the PDH signal, the vertical scale is not meaningfull.  The lower panel shows what happens with the wrong demod phase).   I made the same plot for a higher finesse (Tetm=1%) where the sidebands are resonant when the cavity is locked with the sign flipped, even for the wrong demod phase.

We also wondered if our low finesse would mean that higher order modes would be resonant when the cavity is locked.  Here is a plot of resonance profiles for the first 7 higher order modes.  The top panel shows Tetm=5%, the bottom panel Tetm=38%.  The only of these modes that is resonant with the carrier is the lower sideband of the 5th order modes, which we should be able to keep small once we have a good alingment.  

The last few plots are what higher order modes do to our locking signals. Here is an IQ scatter plot and the locking signal with resonance profiles of the carrier and sidebands when 10% of the power is in a second order mode.   With a mode mismatch like this we still get reasonable locking signal.  

I had a look at some of our cavity transmission peaks , and made a rough approximation of the higher order mode content.  Here are plots of the PDH signals (with my approximation of the transmission profile in the bottom panel) and an IQ plot.   These are both with the demod phase tuned for the 00 mode with our finesse (by using the plot without higher order modes).  

Daneil and I took a video when we were at the X end last night of our actual IQ scatter plot, which looks about as crazy as the prediction above. 

The next two plots are what the IQ plot and PDH signals would look like with my approximation of our higher order mode content and the intended ETM reflectitvy of 5%.  The higher order mode content doesn't totally confuse the locking signal the way that it does with the lower finesse.  

I think that Yuta has some similar plots, and maybe has tried to actually match some of the PDH signals that we see.  

In all of these plots I used: 

Tetm=0.38;
Titm=0.01;
RoCetm=2241.54;
RoCitm=1939.52;
Length=3996;
Gamma=0.1 
 
In all of the plots that say "cavity length" along the horizontal axis, it is of course the microscopic change in cavity length that is plotted, not the total cavity length.  
T1=0.38;
cav.T2=0.01;
cav.RoC1=2241.54;
cav.RoC2=1939.52;
cav.L=3996;
Images attached to this report
Non-image files attached to this report
H1 General (ISC)
sheila.dwyer@LIGO.ORG - posted 14:24, Saturday 18 January 2014 (9382)
at X end

Since the fringe velocity is so much less than it has been ( 1-3 per second) after Hugh's changes yesterday, I decided to see if I could adjust the demod phase by looking at the open loop gain.  I went to the end station from about 1:45 to 2:11.  This wasn't verry sucsessfull since the cavity wasn't well alinged and I couldn't see any cameras to know what mode it was locked to.  I'm back at the corner now.

H1 ISC
stefan.ballmer@LIGO.ORG - posted 00:11, Saturday 18 January 2014 (9380)
First round of IAL alignment (PIT)
I tried the PZT dither today:
- The green arm transmitted signal is now available in the ASC system
  (ADC card 3, channel 24-27 [25-28], are connected to output 1-4 form the the ALS PD concentrator 3) 
- I used the demodulated green arm transmitted signal for all the loops I tried today.
- Dithering PZT2 provided a nice error signal for TMS pointing.
- Dithering PZT1 gave an error signal that I couldn't zero out - not sure why yet. (TMS position offset?)
- Dithering ITM at 1.7 Hz provided a good loop for aligning ITMY.
- The loop did a good job aligning the cavity, but mode-hopping was still hampering the effort.


Still to do:
- Try higher frequency ITM dither (lower stage drive?)
- Investigate PZT1 dither error signal offset - Try Green QPD pointing offset?
- Do yaw loops.
H1 ISC
stefan.ballmer@LIGO.ORG - posted 23:56, Friday 17 January 2014 (9379)
arm modulation frequerncy
Yuta, Kiwamu, Koji, Stefan

- Yuta's calculation (see other alog) showed that the error signal significantly depends on the modulation frequency.
- We therefore used and IFR to try several choices of frequencies.
- We measured the FSR at
  24.429380MHz +-20Hz, and
  24.391480MHz +-20Hz
- This gives us an arm length of 3992.973m +-6m....
- The estimated transverse mode spacing is 5.12kHz.    (R_ITM=1939.52m, R_ETM=2241.54m)
- We tried to set the frequency to exactly FSR +- 5.076kHz (an old estimate of the transverse mode spacing), as well as half of that.
  Subjectively the best performance (least mode hopping) was at 24.424304MHz. It was not perfect.

Still to do:
 - Find a spot with minimal locking point dependence on the 10-mode power.
 - Explore the I/Q demod phase.
H1 General (ISC)
sheila.dwyer@LIGO.ORG - posted 21:23, Friday 17 January 2014 (9378)
X end work

Daniel and I went out to the X end at 5, and were back at 6:30.  we measured the PDH TF now that the loop is staying locked for longer due to less motion, we saw a UGF around 2kHz with lots (around 70 degrees) of phase margin.  We also connected I mon of the FET demod to H1:LSC-X_EXTRA_AI_1_OUT_DQ and Q mon to H1:LSC-X_EXTRA_AI_2_OUT_DQ. 

H1 IOO
kiwamu.izumi@LIGO.ORG - posted 18:48, Friday 17 January 2014 (9377)
PRM parking beam found and parking position re-estiablished

Stefan, Yuta, Kiwamu

As a part of the 10 W preparation, we searched for the PRM parking beam and re-established the parking position.

After some time of steering PRM, we found it hitting on the in-vac aperture which was attached to the inner ceiling of the HAM2 chamber. We could see it from the left most lower viewport of the east side with an IR viewer. We centered the parking beam on the aperture to re-establish the parking position.

The new parking position for PRM is:

With this parking position, I was able to see the beam at the south ceiling viewport with a sensor card. The beam was round which indicated that the beam was not clipped. Indeed, I didn't see any scattered light in HAM2 as far as I looked from the lower side viewports. I took some pictures of the ceiling viewport and its canister. Note that the sensor card attached on the inner wall of the canister was removed after the pictures were taken.

I consulted with Gerardo about possibility of mounting a Kentek beam dump today without removing the lexan plate. However since the beam is so low in the canister with an agressive angle, we agreed that the dump will not fit it without a trick -- the beam is close to the lexan plate and it just hits the guard ring due to its output angle. We need to come up with a better idea to mount a dump.

Images attached to this report
H1 SEI
hugh.radkins@LIGO.ORG - posted 18:11, Friday 17 January 2014 (9376)
ETMX ISI Damping vs Isolation

I have a pretty coarse plot of spectra for the ETM interial sensors with damping only and then with 750mHz Blend level1 Isolation compared.  Not a lot happening in the area of interest below ~1Hz.  I did notice that the Rz was worse though.  This shows up mostly below 0.4Hz.  Stefan removed the Rz Isolation but it only recovers about half way back to the damping only spectra.  There is also the cost of noise between 1 & 2 Hz.  The Reference traces are the damping only except the Rz reference 14 & 20.  These two are the 750mHz spectra with the Rz in the loop.  The Current traces are with the Rzs out of the loop.  The next time the ISI is brought back to isolation, the Rz will be back in.  It doesn't sound like removing the Rz made anyone especially happy.  I wanted to take the ISI to greater levels of isolation but the commissioners said they'll work with this for now.

Before going back to damping only I took the isolation from 750mHz everywhere expect Stage1 X Y & Rz where there was 100mHz blends down to T100mHz (T240s included) on the horz dofs.  This did not improve the situation.  I've noticed too that sometimes the scripts stall part way through and with out the script window popping up to show the status, some states may not be what they seem.

Images attached to this report
LHO General
thomas.vo@LIGO.ORG - posted 17:35, Friday 17 January 2014 (9374)
01/17/2014 Ops Summary
PSL Checklist was OK

Before 8 AM:
- Balers were removing tumbleweeds up and down the X-arm.

9:23AM  - 9:45AM Richard M in the PSL to install Lighthouse dust monitor
9:24AM  - 9:56AM Kiwamu rotates the HWP in the PSL to dial down power to 100 mW
9:30AM  - 9:45AM Gerardo in the LVEA to survey viewports at HAM2
11:11AM - 3:35PM Fil and crew in LVEA pulling cables to ISC racks.
1:14PM  - 4:00PM SEI at HAM4
1:36PM  - 3:00PM Corey at EY in TMS lab.
H1 IOO (PSL)
kiwamu.izumi@LIGO.ORG - posted 09:54, Friday 17 January 2014 - last comment - 17:52, Friday 17 January 2014(9355)
IMC incident decreased to 100 mW

Stefan, Yuta, Kiwamu

We are currently in a low power state for performing the PRM parking beam search.

Power decreased:

We decreased the IMC incident to approximately 100 mW by rotating the motorized half wave plate. We unlocked the interlock to allow us to rotate it while blocking the main laser pipe just in case. Currently the incident power is at 116 mW at the monitor channel, H1:PSL-PERISCOPE_A_DC_POWERMON. Then we locked the interlock back so that nobody can change the power.

Autolocker modified:

We then changed the ISC_IMC guardian script to adapt it to this lower power configuration. The threshold and in1 gain are increased by a factor of 10. Also all the LSC and ASC triggers are lowered by a factor of 10. We found that increasing the ASC common gain by a factor of 10 made the loops unstable. Therefore we set the common gain to be back at 1 as usual. So far it seems locking fine and stable enough to proceed with the parking beam mission.

Comments related to this report
kiwamu.izumi@LIGO.ORG - 17:52, Friday 17 January 2014 (9375)

Now we are back to 1W since we are done with the PRM parking search. We restored all the settings that we changed.

H1 IOO (ISC, PSL)
kiwamu.izumi@LIGO.ORG - posted 16:00, Friday 06 December 2013 - last comment - 17:22, Monday 20 January 2014(8867)
EOM characterization: good

Alexa, Stefan, Sheila and Kiwamu

Yesterday, we set up an optical spectrum analyzer on the PSL table to measure the characteristic of the EOM. The results look good except for the 24 MHz resonance . The resonance for the 24 MHz sideband is apart from the modulation frequency by 250 kHz or so. However the IMC doesn't need a large modulation depth and the IMC locking has been OK, we are good. Also, I took some impedance data and will put those data together into a DCC document for a record purpose.

The plots below are the measured modulation depth when driven hard as a function of the modulation frequencies. The vertical dashed-lines represent our actual modulation frequencies i.e. f1 = 9099471 Hz , f_mc = 24078360 Hz and f5 = 5 x f1.

Images attached to this report
Comments related to this report
kiwamu.izumi@LIGO.ORG - 15:55, Monday 20 January 2014 (9393)

A document summarizing the measurements and their results is now available in DCC (https://dcc.ligo.org/LIGO-E1300966).

kiwamu.izumi@LIGO.ORG - 17:22, Monday 20 January 2014 (9395)ISC

I kept forgetting to report the important information regarding to the modulation depths. Here are the estimated modulation depths:

   Modulation depths [rad] Peak height measured with OSA RF power at the input
9 MHz 0.1 20 mV 12.3 dBm
24 MHz less than 0.04  less than 3 mV 13.8 dBm
45 MHz 0.07 10 mV 10.8 dBm

The peak height of the carrier light was about 7.3 V. I used 2 * sqrt(V_sideband / V_carrier) to derive the modulation depths.

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