ID |
Date |
Author |
Type |
Category |
Subject |
2668
|
Thu Mar 11 17:51:04 2010 |
Koji | Update | SUS | Recent status of SOSs |
Jenne, Koji
Recent status of SOSs:
We completed one of the suspension (ITMY).
ITMX: 6 Magnets, standoffs, and guide rod glued / balance to be confirmed / needs to be baked
ITMY: 6 Magnets, standoffs, and guide rod glued / balance confirmed / needs to be baked
SRM: 6 Magnets, one standoff, and guide rod glued, / waiting for the release from the gluing fixture.
PRM: one standoff, and guide rod glued / waiting for the magnet gluing.
We think we solved all the problems for hanging the suspensions.
--- Magnet gluing fixture ---
- There is the two kinds of fixtures. Neither does work propery in the original form!
- The height of the side magnets should be finely adjusted by changing the teflon sheets beneath the optics in the fixture.
- Be aware of the polarity of the fixture in terms of the side magnets
- Wrongly glued magnets (and others) can be removed by a razor blade with some amount of acetone.
- The pickle picker frequently knocks the magnets down during the release. Don't s be down in the dumps too much.
--- Suspending the mirror ---
- The wire winches must be carefully attached to the suspension tower such that the wires are not streached during fastening the clamps.
- There are a couple variations of the drawings for SOS. The one we have has #4-40 for the earthquake stops at the bottom.
Zach and Mott made the EQ stops with the right size.
|
2669
|
Fri Mar 12 13:52:18 2010 |
Zach | Update | elog | elog restarted |
The elog was down and I ran the restart script. |
2671
|
Sat Mar 13 21:30:22 2010 |
rana | Update | PEM | Styrofoam Cooler on the Seismos |

|
2672
|
Sat Mar 13 22:16:03 2010 |
rana | Update | WienerFiltering | Guralp Huddle Test software |
I used some recent better data to try for better Z subtraction.
Dmass helped me understand that sqrt(1-Coherence) is a good estimate of the theoretical best noise subtraction residual. This should be added to DTT. For reference the Jan statistic is the inverse of this.
This should get better once Steve centers the Guralps. |
Attachment 1: guralpznoise.png
|
|
2673
|
Mon Mar 15 09:43:47 2010 |
steve | Update | PEM | more sandblasting today |
Do not open IFO vacuum envelope today! They are sandblasting again at CES |
2674
|
Mon Mar 15 16:39:36 2010 |
steve | Update | PEM | Guralp2 centered |
Quote: |

Guralp 2 centered.The mass position offsets are: E-W 0.05V, N-S 0V, Z 0.4V
Guralp 1: E-W -0.1V, N-S -0.25V, Z 0V measured, not adjusted
The GUR2_X channel has an offset. See plot below when seismometers are disconnected. This offset has to be removed.
NOTE: this huddle is on bad-soft ground-lenoleum tile from prehistoric Flintstone age
|
|
Attachment 1: grlp2ffst.jpg
|
|
2675
|
Tue Mar 16 04:22:02 2010 |
Jenne | Update | Environment | Earthquake, Mag 4.4 |
Earthquake Details
Magnitude |
4.4 |
Date-Time |
- Tuesday, March 16, 2010 at 11:04:00 UTC
- Tuesday, March 16, 2010 at 04:04:00 AM at epicenter
|
Location |
33.998°N, 118.072°W |
Depth |
18 km (11.2 miles) |
Region |
GREATER LOS ANGELES AREA, CALIFORNIA |
Distances |
- 2 km (1 miles) ENE (58°) from Pico Rivera, CA
- 4 km (3 miles) ESE (115°) from Montebello, CA
- 4 km (3 miles) SSW (207°) from Whittier Narrows Rec. Area, CA
- 9 km (5 miles) NE (39°) from Downey, CA
- 9 km (6 miles) SSW (206°) from El Monte, CA
- 17 km (11 miles) ESE (112°) from Los Angeles Civic Center, CA
|
Location Uncertainty |
horizontal +/- 0.4 km (0.2 miles); depth +/- 0.9 km (0.6 miles) |
Parameters |
Nph=122, Dmin=5 km, Rmss=0.37 sec, Gp= 25°,
M-type=local magnitude (ML), Version=2 |
Source |
|
Event ID |
ci14601172
|
-----------------------------------------
MC1 and MC3 seem to have kept themselves together, but all the other optics' watchdogs tripped. |
Attachment 1: EQ_16Mar2010.png
|
|
2676
|
Tue Mar 16 05:10:39 2010 |
koji | Update | Environment | Earthquake, Mag 4.4 |
Some of the suspensions got watchdog tripped -> enabled -> damped.
The MC mirrors got slightly misaligned.
|
Attachment 1: 100316_MC_SUS.png
|
|
2677
|
Tue Mar 16 09:37:30 2010 |
steve | Update | SUS | eq 4.4 seen by oplevs and osems |
The oplev plots clearly show the alignment effect of this eq. |
Attachment 1: opleveq4.4.jpg
|
|
Attachment 2: eq4.4.jpg
|
|
Attachment 3: opleveq4.4d3.jpg
|
|
2678
|
Thu Mar 18 08:49:51 2010 |
steve | Update | PEM | Guralp2 centered again ? |
Someone adjusted the Guralp2 mass position last night??
NO |
Attachment 1: grlp2xadj.jpg
|
|
2679
|
Thu Mar 18 10:46:51 2010 |
Koji | Update | ABSL | PLL reconstructed |
Last night (Mar 17) I checked the PLL setup as Mott have had some difficulty to get a clean lock of the PLL setting.
- I firstly found that the NPRO beam is not going through the Faraday isolator well. This was fixed by aligning the steering mirrors before the Faraday.
- The signal from the RF PD was send to the RF spectrum analyzer through a power splitter. This is a waist of the signal. It was replaced to a directional coupler.
- Tee-ing the PZT feedback to the oscilloscope was producing the noise in the laser frequency. I put the oscilloscope to the 600Ohm output of the SR560, while connectiong the PZT output to the 50Ohm output.
- In addition, 6dB+6dB attenuators have been added to the PZT feedback signal.
Now the beating signal is much cleaner and behave straight forward. I will add some numbers such as the PD DC output, RF levels, SR560 settings...
Now I am feeling that we definitely need the development of really clean PLL system as we use PLL everywhere! (i.e. wideband PD, nice electronics, summing amplifiers, stop poking SR560, customize/specialize PDH box, ...etc) |
2680
|
Thu Mar 18 12:27:56 2010 |
Alberto | Update | ABSL | PLL reconstructed |
Quote: |
Last night (Mar 17) I checked the PLL setup as Mott had some difficulty to get a clean lock of the PLL setting.
- I firstly found that the NPRO beam is not going through the Faraday isolator well. This was fixed by aligning the steering mirrors before the Faraday.
- The signal from the RF PD was send to the RF spectrum analyzer through a power splitter. This is a waist of the signal. It was replaced to a directional coupler.
- Tee-ing the PZT feedback to the oscilloscope was producing the noise in the laser frequency. I put the oscilloscope to the 600Ohm output of the SR560, while connectiong the PZT output to the 50Ohm output.
- In addition, 6dB+6dB attenuators have been added to the PZT feedback signal.
Now the beating signal is much cleaner and behave straight forward. I will add some numbers such as the PD DC output, RF levels, SR560 settings...
Now I am feeling that we definitely need the development of really clean PLL system as we use PLL everywhere! (i.e. wideband PD, nice electronics, summing amplifiers, stop poking SR560, customize/specialize PDH box, ...etc)
|
I also had noticed the progressive change of the aux NPRO alignment to the Farady.
I strongly agree about the need of a good and robust PLL.
By modifying the old PDH box (version 2008) eventually I was able to get a PLL robust enough for my purposes. At some point that wasn't good enough for me either.
I then decided to redisign it from scratch. I'm going to work on it. Also because of my other commitments, I'd need a few days/1 week for that. But I'd still like to take care of it. Is it more urgent than that? |
2681
|
Thu Mar 18 13:40:35 2010 |
Koji | Update | ABSL | PLL reconstructed |
We use the current PLL just now, but the renewal of the components are not immediate as it will take some time. Even so we need steady steps towards the better PLL. I appreciate your taking care of it.
Quote: |
Quote: |
Last night (Mar 17) I checked the PLL setup as Mott had some difficulty to get a clean lock of the PLL setting.
- I firstly found that the NPRO beam is not going through the Faraday isolator well. This was fixed by aligning the steering mirrors before the Faraday.
- The signal from the RF PD was send to the RF spectrum analyzer through a power splitter. This is a waist of the signal. It was replaced to a directional coupler.
- Tee-ing the PZT feedback to the oscilloscope was producing the noise in the laser frequency. I put the oscilloscope to the 600Ohm output of the SR560, while connectiong the PZT output to the 50Ohm output.
- In addition, 6dB+6dB attenuators have been added to the PZT feedback signal.
Now the beating signal is much cleaner and behave straight forward. I will add some numbers such as the PD DC output, RF levels, SR560 settings...
Now I am feeling that we definitely need the development of really clean PLL system as we use PLL everywhere! (i.e. wideband PD, nice electronics, summing amplifiers, stop poking SR560, customize/specialize PDH box, ...etc)
|
I also had noticed the progressive change of the aux NPRO alignment to the Farady.
I strongly agree about the need of a good and robust PLL.
By modifying the old PDH box (version 2008) eventually I was able to get a PLL robust enough for my purposes. At some point that wasn't good enough for me either.
I then decided to redisign it from scratch. I'm going to work on it. Also because of my other commitments, I'd need a few days/1 week for that. But I'd still like to take care of it. Is it more urgent than that?
|
|
2684
|
Thu Mar 18 21:42:26 2010 |
Koji | Update | ABSL | PLL reconstructed |
I checked the setup further more.
- I replaced the PD from NewFocus 1GHz one to Thorlabs PDA255.
- I macthed the power level of the each beam.
Now I have significant fraction of beating (30%) and have huge amplitude (~9dBm).
The PLL can be much more stable now.
Koji |
2685
|
Fri Mar 19 18:00:14 2010 |
jenne | Update | PEM | Guralp2 centered again |
[Jenne, Sanjit]
It looks like Steve used a GND-12V supply to power the Guralp through the little breakout box (the box is for checking the centering of the mass). This is BAD. The Guralps want +/- 12V.
We centered all of the channels on Gur2, and checked the channels on Gur1, so we'll see how they're feeling after a while. |
2686
|
Fri Mar 19 21:15:33 2010 |
rana | Update | PEM | Guralp2 centered again |
This trend of the last 200 days shows that GUR2 has been bad forever...until now anyways. |
Attachment 1: Untitled.png
|
|
2687
|
Fri Mar 19 23:03:41 2010 |
rana | Update | PEM | Guralp2 centered again |
I went and double-checked and aligned the styrofoam cooler at ~5:00 UTC. It was fine, but we really need a better huddling box. Where's that granite anyway?
Here's the new Huddle Test output. This time I show the X-axis since there's some coherence now below 0.1 Hz.
You'll also notice that the Wiener filter is now beating the FD subtraction. This happened when I increased the # of taps to 8000. Looks like the noise keeps getting lower as I increase the number of taps, but this is really a kind of cheat if you think about it carefully. |
Attachment 1: huddlez.png
|
|
2689
|
Sun Mar 21 19:25:29 2010 |
rana | Update | PEM | Guralp2 centered again |
From this morning, now in calibrated units, and with the Güralp self noise spec from the Güralp manual. |
Attachment 1: huddlez.png
|
|
2690
|
Sun Mar 21 20:08:20 2010 |
kiwamu, rana | Update | PSL | EOM wasit size |
We are going to set the waist size to 0.1 mm for the beam going through the triple resonant EOM on a new PSL setup.
When we were drawing a new PSL diagram, we just needed to know the waist size at the EOM in order to think about mode matching.

This figure shows the relation between the waist size and the spot size at the aperture of the EOM.
The x-axis is the waist size, the y-axis is the spot size. It is clear that there is a big clearance at 0.1 mm waist size. This is good.
Also it is good because the waist size is much above the damage threshold of the EO crystal (assuming 1W input).
The attached file is the python code for making this plot. |
Attachment 2: waist.py.zip
|
2691
|
Sun Mar 21 21:02:39 2010 |
Koji | Update | PSL | EOM waist size |
You don't need a lengthy code for this. It is obvious that the spot size at the distance L is minimum when L =
zR, where zR is the Rayleigh range. That's all.
Then compare the spot size and the aperture size whether it is enough or not.
It is not your case, but if the damage is the matter, just escape to the large zR side. If that is not possible
because of the aperture size, your EOM is not adequate for your purpose. |
2694
|
Mon Mar 22 11:37:09 2010 |
steve | Update | PEM | jackhammering |
There was more jackhammering this morning just about 20 ft north-west of the beamsplitter chamber, outside. |
Attachment 1: jackhammering2.jpg
|
|
2696
|
Mon Mar 22 22:11:26 2010 |
Mott | Update | ABSL | PLL reconstructed |
It looks like the PLL drifted alot over the weekend, and we couldn't get it back to 9 dBm. We switched back to the new focus wideband PD to make it easier to find the beat signal. I replaced all the electronics with the newly fixed UPDH box (#17) and we aligned it to the biggest beat frequency we could get, which ended up being -27 dBm with a -6.3V DC signal from the PD.
Locking was still elusive, so we calculated the loop gain and found the UGF is about 45 kHz, which is too high. We added a 20 dB attenuator to the RF input to suppress the gain and we think we may have locked at 0 gain. I am going to add another attenuator (~6 dB) so that we can tune the gain using the gain knob on the UPDH box.
Finally, attached is a picture of the cable that served as the smb - BNC adaptor for the DC output of the PD. The signal was dependent on the angle of the cable into the scope or multimeter. It has been destroyed so that it can never harm another innocent experiment again! |
Attachment 1: IMG_0150.JPG
|
|
2697
|
Mon Mar 22 23:37:32 2010 |
Mott | Update | ABSL | PLL reconstructed |
We have managed to lock the PLL to reasonable stability. The RF input is attenuated by 26 dBm and the beat signal locks very close to the carrier of the marconi (the steps on the markers of the spectrum analyzer are coarse). We can use the marconi and the local boost of the pdh box to catch the lock at 0 gain. Once the lock is on, the gain can be increased to stabilize the lock. The locked signals are shown in the first photo (the yellow is the output of the mixer and the blue is the output to the fast input of the laser. If the gain is increased too high, the error signal enters an oscillatory regime, which probably indicates we are overloading the piezo. This is shown in the second photo, the gain is being increased in time and we enter the non-constant regime around mid-way through.
Tomorrow I will use this locked system to measure the PZT response (finally!). |
Attachment 1: 2010-03-22_23.14.00.jpg
|
|
Attachment 2: 2010-03-22_23.24.50.jpg
|
|
2698
|
Tue Mar 23 00:31:51 2010 |
Koji | Update | IOO | MC realigned |
This is the first touch to the MC mirrors after the earthquake on 16th.
- I made an aluminum access connector so that we can work on the MC even the door is open. We still can be able to open the aluminum tube. The photos are attached. Steve, could you please look it at a glance whether the seal is enough or not.
- MC resonances were flashing. Align MC2 and MC3 so that we have many TEM00s.
- Found c1vmesus2 gone mad. Restarted remotely according to the wiki entry.
- Reset the MC coil output matrix to 1. (Previously, balance was adjusted so that A2L was minimized.)
- Excite MC2 Pitch/Yaw at 8 and 9 Hz, looking at the peaks in the MC-MCL output. Move MC2 Pitch/Yaw so that the peak
is reduced. (*)
- MC1/MC3 were aligned so that we get the maximum transmission (or minimum reflection). (**)
- Repeat (*) and (**)
So far, I have aligned in Yaw such that the yaw peak is minimized. |
Attachment 1: IMG_2346.jpg
|
|
Attachment 2: IMG_2347.jpg
|
|
2699
|
Tue Mar 23 09:37:36 2010 |
steve | Update | IOO | vac envelope has to be sealed as antproof for overnight |
Quote: |
This is the first touch to the MC mirrors after the earthquake on 16th.
- I made an aluminum access connector so that we can work on the MC even the door is open. We still can be able to open the aluminum tube. The photos are attached. Steve, could you please look it at a glance whether the seal is enough or not.
- MC resonances were flashing. Align MC2 and MC3 so that we have many TEM00s.
- Found c1vmesus2 gone mad. Restarted remotely according to the wiki entry.
- Reset the MC coil output matrix to 1. (Previously, balance was adjusted so that A2L was minimized.)
- Excite MC2 Pitch/Yaw at 8 and 9 Hz, looking at the peaks in the MC-MCL output. Move MC2 Pitch/Yaw so that the peak
is reduced. (*)
- MC1/MC3 were aligned so that we get the maximum transmission (or minimum reflection). (**)
- Repeat (*) and (**)
So far, I have aligned in Yaw such that the yaw peak is minimized.
|
This seal is good for daily use- operation only. The IFO has to be sealed with light metal doors every night so ants and other bugs can not find their way in.
Our janitor Kevin is mopping the hole IFO room floor area with 5% ant killing solution in water in order to discourage bugs getting close to our openings of the vented chamber.
You may be sensitive to this chemical too. Do not open chamber till after lunch. |
Attachment 1: pc3.JPG
|
|
Attachment 2: pc4.JPG
|
|
2700
|
Tue Mar 23 09:55:20 2010 |
Koji | Update | IOO | vac envelope has to be sealed as antproof for overnight |
Roger.
Quote: |
This seal is good for daily use- operation only. The IFO has to be sealed with light metal doors every night so ants and other bugs can not find their way in.
|
|
2701
|
Tue Mar 23 10:11:13 2010 |
steve | Update | PEM | small air cond unit failed yesterday |
Old control room air condition failed yesterday around noon. It was blowing 80-85F hot air for about 2-3 hours at racks 1Y4-7 and the entry room 103 |
Attachment 1: 20datm.jpg
|
|
2702
|
Tue Mar 23 15:38:26 2010 |
Alberto | Update | elog | elog just restarted |
I found the elog down and I restarted it.
Then, after few seconds it was down again. Maybe someone else was messing with it. I restarted an other 5 times and eventually it came back up. |
2703
|
Tue Mar 23 18:44:46 2010 |
Mott | Update | ABSL | PLL reconstructed |
After realigning and getting the lock today, I tried to add in the SR785 to measure the transfer function. As soon as I turn on the piezo input on the PDH box, however, the lock breaks and I cannot reacquire it. We are using an SR650 to add in the signal from the network analyzer and that has worked. We also swapped the 20 dB attenuator for a box which mimics the boost functionality (-20 dB above 100 Hz, 0 dB below 6Hz). I took some spectra with the SR750, and will get some more with the network analyzer once Alberto has finished with it.
The SR750 spectra is posted below. The SR750 only goes up to 100 kHz, so I will have to use the network analyzer to get the full range. |
Attachment 1: NPRO_PLL_freqresp.png
|
|
2704
|
Tue Mar 23 22:46:43 2010 |
Alberto | Update | 40m Upgrading | REFL11 upgraded |
I modified REFL11 according to the changes lsited in this schematic (see wiki / Upgrade 09 / RF System / Upgraded RF Photodiodes ).
I tuned it to be resonant at 11.06MHz and to have a notch at 22.12MHz.
These are the transfer functions that I measured compared with what I expected from the LISO model.

The electronics transfer function is measured directily between the "Test Input" and the "RF Out" connector of the box. the optical transfer function is measured by means of a AM laser (the "Jenne laser") modulated by the network analyzer.
The AM laser's current was set at 20.0mA and the DC output of the photodiode box read about 40mV.
The LISO model has a different overall gain compared to the measured one, probably because it does not include the rest of the parts of the circuit other than the RF out path.
I spent some time trying to understand how touching the metal cage inside or bending the PCB board affected the photodiode response. It turned out that there was some weak soldering of one of the inductors. |
2705
|
Wed Mar 24 02:06:24 2010 |
Koji | Update | IOO | vac envelope has to be sealed as antproof for overnight |
Matt and Koji:
We closed the light doors of the chambers.
Quote: |
Roger.
Quote: |
This seal is good for daily use- operation only. The IFO has to be sealed with light metal doors every night so ants and other bugs can not find their way in.
|
|
|
2706
|
Wed Mar 24 03:58:18 2010 |
kiwamu, matt, koji | Update | Green Locking | leave PLL locked |
We are leaving the PLL as it is locked in order to see the long term stability. And we will check the results in early morning of tomorrow.
DO NOT disturb our PLL !!
(what we did)
After Mott left, Matt and I started to put feedback signals to the temperature control of NPRO.
During doing some trials Matt found that NPRO temperature control input has an input resistance of 10kOhm.
Then we put a flat filter ( just a voltage divider made by a resistor of ~300kOhm and the input impedance ) with a gain of 0.03 for the temperature control to inject a relatively small signal, and we could get the lock with the pzt feedback and it.
In addition, to obtain more stable lock we then also tried to put an integration filter which can have more gain below 0.5Hz.
After some iterations we finally made a right filter which is shown in the attached picture and succeeded in obtaining stable lock.
|
Attachment 1: DSC_1402.JPG
|
|
2707
|
Wed Mar 24 04:22:51 2010 |
kiwamu, matt | Update | Green Locking | two NPRO PLL |
Now some pedestals, mirrors and lenses are left on the PSL table, since we are on the middle way to construct a PLL setup which employs two NPROs instead of use of PSL laser.
So Please Don't steal any of them. |
2710
|
Wed Mar 24 14:52:02 2010 |
Alberto | Update | Green Locking | two NPRO PLL |
Quote: |
Now some pedestals, mirrors and lenses are left on the PSL table, since we are on the middle way to construct a PLL setup which employs two NPROs instead of use of PSL laser.
So Please Don't steal any of them.
|
Can I please get the network analyzer back? |
2711
|
Wed Mar 24 14:57:21 2010 |
Alberto | Update | 40m Upgrading | REFL11 upgraded |
Hartmut suggested a possible explanation for the way the electronics transfer function starts picking up at ~50MHz. He said that the 10KOhm resistance in series with the Test Input connector of the box might have some parasitic capacitance that at high frequency lowers the input impedance.
Although Hartmut also admitted that considering the high frequency at which the effect is observed, anything can be happening with the electronics inside of the box. |
2712
|
Wed Mar 24 15:59:59 2010 |
kiwamu, matt | Update | Green Locking | leave PLL locked |
Matt checked it in this morning and he found it's been locked during the night.
|
2713
|
Thu Mar 25 09:07:08 2010 |
steve | Update | PEM | Guralp2 x problem is back |
Quote: |
I went and double-checked and aligned the styrofoam cooler at ~5:00 UTC. It was fine, but we really need a better huddling box. Where's that granite anyway?
Here's the new Huddle Test output. This time I show the X-axis since there's some coherence now below 0.1 Hz.
You'll also notice that the Wiener filter is now beating the FD subtraction. This happened when I increased the # of taps to 8000. Looks like the noise keeps getting lower as I increase the number of taps, but this is really a kind of cheat if you think about it carefully.
|
The same thing happening again. The intermittent offset upstream of the seismometer that never got fixed.
The granite plate and ball bearings are in. I will place seismometers on it. |
Attachment 1: grlp2xproblm.jpg
|
|
2714
|
Thu Mar 25 17:29:48 2010 |
kiwamu, mott | Update | Green Locking | PLL two NPROs |
In this afternoon, Mott and I tried to find a beat note between two NPROs which are going to be set onto each end table for green locking.
At first time we could not find any beats. However Koji found that the current of innolight NPRO was set to half of the nominal.
Then we increased the current to the nominal of 2A, finally we succeeded in finding a beat note.
Now we are trying to lock the PLL.
P.S. we also succeeded in acquiring the lock
nominal setup
|
innolight |
lightwave |
T [deg] |
39.75 |
37.27 |
current [A] |
2 |
2 |
laser power [mW] |
950 |
700 |
|
2715
|
Thu Mar 25 17:32:42 2010 |
Alberto | Update | 40m Upgrading | REFL55 Upgraded |
I upgraded the old REFL199 to the new REFL55.
To do that I had to replace the old photodiode inside, switching to a 2mm one.
Electronics and optical transfer functions, non normalized are shown in the attached plot.

The details about the modifications are contained in this dedicated wiki page (Upgrade_09 / RF System / Upgraded RF Photodiodes) |
Attachment 1: 2010-03-25_REFL55_model_to_meas_comparison.png
|
|
2716
|
Fri Mar 26 10:48:35 2010 |
steve | Update | SAFETY | safety glasses measured |
Safety glasses 1064 nm transmission measured at ~200 mW level. They are all good. |
Attachment 1: P1060188.JPG
|
|
Attachment 2: P1060199.JPG
|
|
2717
|
Sat Mar 27 16:23:10 2010 |
Koji | Update | SUS | another SRM sidemagnet glued |
Kiwamu and Koji
Last night we have released PRM from the gluing fixture. All of the six magnets are successfully released from the fixture.
We put SRM on the fixuture and glued a side magnet which we had failed at the last gluing.
We let it cure in the Al house. This should be the last magnet gluing until ETMs are delivered.
[Current status]
ITMX (ITMU03): all of magnets/guiderod/standoffs glued, mirror baked; balance to be confirmed
ITMY (ITMU04): all of magnets/guiderod/standoffs glued, balance confirmed, mirror baked
SRM (SRMU03): magnets/guiderod/standoff glued; a side magnet gluing in process, balance to be confirmed, last stand off to be glued, mirror to be baked
PRM (SRMU04): magnets/guiderod/standoff glued; balance to be confirmed, last stand off to be glued, mirror to be baked
TT: magnets/guiderod/standoff glued; balance to be confirmed, last stand off to be glued, mirror to be baked |
2718
|
Sun Mar 28 17:28:26 2010 |
matt, kiwamu | Update | Green Locking | frequency discriminator for green PLL |
Last Friday, Matt made a frequency discriminator circuit on a bread board in order to test the idea and study the noise level. I think it will work for phase lock acquisition of Green locking.
As a result a response of 100kHz/V and a noise level of 2uV/rtHz @ 10Hz are yielded. This corresponds to 0.2Hz/rtHz @ 10Hz.
The motivation of using frequency discriminators is that it makes a frequency range wider and easier for lock acquisition of PLLs in green locking experiment.
For the other possibility to help phase lock acquisition, Rana suggested to use a commercial discriminator from Miteq.
(principle idea)
The diagram below shows a schematic of the circuit which Matt has built.

Basically an input signal is split into two signals right after the input, then one signal goes through directly to a NAND comparator.
On the other hand another split signal goes through a delay line which composed by some RC filters, then arrive at the NAND comparator with a certain amount of delay.
After going through the NAND comparator, the signal looks like a periodic pulses (see below).
If we put a signal of higher frequency we get more number of pulses after passing through the NAND.

Finally the pulse-signal will be integrated at the low pass filter and converted to a DC signal.
Thus the amplitude of DC signal depends on the number of the pulses per unit time, so that the output DC signal is proportional to the frequency of an input signal.
(result)
By putting a TTL high-low signal, an output of the circuit shows 100kHz/V linear response.
It means we can get DC voltage of 1 V if a signal of 100kHz is injected into the input.
And the noise measurement has been done while injecting a input signal. The noise level of 0.2Hz/rtHz @ 10 Hz was yielded.
Therefore we can lock the green PLL by using an ordinary VCO loop after we roughly guide a beat note by using this kind of discriminator.
 |
Attachment 1: DSC_1407.JPG
|
|
Attachment 2: FD.png
|
|
Attachment 3: FDnoise.png
|
|
2719
|
Sun Mar 28 20:00:17 2010 |
rana | Update | Cameras | GigE camera no work from screen |
Not that this is an urgent concern, just a data point which shows that it doesn't just not work at the sites. |
Attachment 1: Untitled.png
|
|
2727
|
Mon Mar 29 10:40:59 2010 |
josephb | Update | Cameras | GigE camera no work from screen |
Quote: |
Not that this is an urgent concern, just a data point which shows that it doesn't just not work at the sites.
|
I had to restart the dhcpd server on Ottavia that allows us to talk to the camera. I then also changed the configuration script on the camera so that it no longer thinks ottavia is 131.215.113.97, but correctly 192.168.113.97. Overall took 5 minutes.
I also looked up services for Centos 5, and set it using the program serviceconf to start the DHCP server when Ottavia is rebooted now. That should head off future problems of that nature. For reference, to start the dhcp server manually, become root and type "service dhcpd start".
|
2728
|
Mon Mar 29 15:19:33 2010 |
mevans | Update | Green Locking | frequency discriminator for green PLL |
Thanks for the great entry!
In order to make this work for higher frequencies, I would add Hartmut's suggestion of a frequency dividing input stage. If we divide the input down by 100, the overall range will be about 200MHz, and the noise will be about 20Hz/rtHz. That might be good enough... but we can hope that the commercial device is lower noise!
Quote: |
Last Friday, Matt made a frequency discriminator circuit on a bread board in order to test the idea and study the noise level. I think it will work for phase lock acquisition of Green locking.
As a result a response of 100kHz/V and a noise level of 2uV/rtHz @ 10Hz are yielded. This corresponds to 0.2Hz/rtHz @ 10Hz.
The motivation of using frequency discriminators is that it makes a frequency range wider and easier for lock acquisition of PLLs in green locking experiment.

|
|
2731
|
Mon Mar 29 18:50:14 2010 |
Koji | Update | SUS | PRM sidemagnet glued |
PRM was released from the fixuture without any trouble. This was the last magnet gluing until ETMs are delivered.
The below is the up-to-date Jenne stat table.
The clean room is getting too narrow. I am thinking that we should install ITMs to the chamber so that we can accommodate SRM/PRM suspensions. |
Attachment 1: StatusTable.png
|
|
2737
|
Wed Mar 31 02:57:48 2010 |
kiwamu | Update | Green Locking | frequency counter for green PLL |
Rana found that we had a frequency counter SR620 which might be helpful for lock acquisition of the green phase lock.
It has a response of 100MHz/V up to 350MHz which is wide range and good for our purpose. And it has a noise level of 200Hz/rtHz @ 10Hz which is 1000 times worse than that Matt made (see the entry).
The attached figure is the noise curve measured while I injected a signal of several 100kHz. In fact I made sure that the noise level doesn't depends on the frequency of an input signal.
The black curve represents the noise of the circuit Matt has made, the red curve represents that of SR620. |
Attachment 1: FCnoise.png
|
|
2739
|
Wed Mar 31 10:34:02 2010 |
josephb | Update | elog | Elog not responding this morning |
When I went to use the elog this morning, it wasn't responding. I killed the process on nodus, and then restarted, per the 40m wiki instructions. |
2741
|
Wed Mar 31 12:30:31 2010 |
rana | Update | Green Locking | frequency counter for green PLL |
Its a good measurement - you should adjust the input range of the 620 using the front panel 'scale' buttons to see how the noise compares to Matt's circuit when the range is reduced to 1 MHz. In any case, we would use it in the 350 MHz range mode. What about the noise of the frequency discriminator from MITEQ? |
2742
|
Wed Mar 31 15:31:53 2010 |
steve | Update | PSL | Reference Cavity RF PD base upgraded |
Quote: |
Some more words about the RFAM: I noticed that there was an excess RFAM by unlocking the RC and just looking at the RF out with the 50 Ohm input of the scope. It was ~100 mVp-p! In the end our method to minimize the AM was not so sensible - we aligned the waveplate before the EOM so as to minimize the p-pol light transmitted by the PBS cube just ahead of the AOM. At first, this did not minimize the RFAM. But after I got angry at the bad plastic mounting of the EOM and re-aligned it, the AM seemed to be small with the polarization aligned to the cube. It was too small to measure on the scope and on the spectrum analyzer, the peak was hopping around by ~10-20 dB on a few second timescale. Further reduction would require some kind of active temperature stabilization of the EOM housing (maybe a good SURF project!).
For the EOM mount we (meaning Steve) should replace the lame 2-post system that's in there with one of the mounts of the type that is used in the Mach-Zucker EOMs. I think we have spare in the cabinet next to one of the arms. 
After the RFAM monkeying, I aligned the beam to the RC using the standard, 2-mirror, beam-walking approach. You can see from the attached plot that the transmission went up by ~20% ! And the reflection went down by ~30%. I doubt that I have developed any new alignment technique beyond what Yoichi and I already did last time. Most likely there was some beam shape corruption in the EOM, or the RFAM was causing us to lock far off the fringe. Now the reflected beam from the reference cavity is a nice donut shape and we could even make it better by doing some mode matching! This finally solves the eternal mystery of the bad REFL beam (or at least sweeps it under the rug).
At the end, I also fixed the alignment of the RFPD. It should be set so the incident angle of the beam is ~20-40 deg, but it was instead set to be near normal incidence ?! Its also on flimsy plastic legs. Steve, can you please replace this with the new brass ones?
|
Teflon feet removed and heavy brass-delrin pd base installed. Ref-cavity reflected light remains to be beautiful doughnut shape on camera. |
Attachment 1: brspdbs.JPG
|
|