ID |
Date |
Author |
Type |
Category |
Subject |
4782
|
Thu Jun 2 23:10:10 2011 |
Koji | Update | Electronics | REFL11 test results (Re: REFL11 fixed) |
The full characterization of REFL11 is found in the PDF.
Resonance at 11.062MHz
Q of 15.5, transimpedance 4.1kOhm
shotnoise intercept current = 0.12mA (i.e. current noise of 6pA/rtHz)
Notch at 22.181MHz
Q of 28.0, transimpedance 23 Ohm
Notch at 55.589MHz
Q of 38.3, transimpedance 56 Ohm
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Attachment 1: REFL11_test.pdf
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4783
|
Fri Jun 3 14:27:32 2011 |
Koji | Update | Electronics | POP55 test results |
The full characterization of POP55 is found in the PDF.
Resonance at 54.49MHz
Q of 2.5, transimpedance 241Ohm
shotnoise intercept current = 4.2mA (i.e. current noise of 37pA/rtHz)
Notch at 11.23MHz
Q of 2.4, transimpedance 6.2 Ohm
Notch at 110.80MHz
Q of 53.8, transimpedance 13.03 Ohm
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Attachment 1: POP55_test.pdf
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4787
|
Mon Jun 6 16:44:34 2011 |
Koji | Update | Electronics | POY11 tested |
The full characterization of POY11 is found in the PDF.
Resonance at 11.03MHz
Q of 7.6, transimpedance 1.98kOhm
shotnoise intercept current = 0.17mA (i.e. current noise of 7pA/rtHz)
Notch at 21.99MHz
Q of 56.2, transimpedance 35.51 Ohm
Notch at 55.20MHz
Q of 48.5, transimpedance 37.5 Ohm
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Attachment 1: POY11_test.pdf
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4805
|
Fri Jun 10 14:50:37 2011 |
Koji | Update | LSC | New LSC code installed |
[Koji Jamie]
The new c1lsc code has been installed. The LSC screens have also been updated (except for ASS screen).
The major changes are:
1. Naming of the RFPD channels. Now the PD signals were named like:
REFL11_I_IN1, REFL11_I_IN2, REFL11_I_OUT ....
instead of REFL11I_blah
2. NREFL11, etc has been removed. We now have the official error signals
named like
REFL11_I_ERR
We can't use the name "REFL11_I" for the error signal as this name is
occupied by the name of the filter module. |
4813
|
Tue Jun 14 03:15:29 2011 |
Koji | HowTo | Computer Scripts / Programs | Kissel Button Generator |
I have made a python script to generate the button designed by Jeff Kissel for his ISI screen.
It is currently located at the following location:
/cvs/cds/rtcds/caltech/c1/medm/c1lsc_tst/master/KisselButtonGenerator/generate_KisselButton.py
but should be relocated to somewhere appropriate.
It also uses fragmented medm files named "MATRIX*.adl_parts ".
# Jamie, could you suggest the right place?
The parameters are assigned at the beggining of the script.
This script print the result to stdout. So you need to redirect the output into a file.
e.g.
> ./generate_KisselButton.py >tmp.adl
The script should be modified such that it accepts the command line options.
It needs more python learning for me.
# Number of the column
mat_h = 20;
# Number of the row
mat_v = 10;
# horizontal pixel size of the rectangular display for each matrix element
button_width = 8;
# vertical pixel size of the rectangular display for each matrix element
button_height = 8;
replace_dict = {
# Title
'${DISPLAY_LABEL}':'ITMX_INMATRIX',
# Path of the MEDM file to be open by clicking the button
'${DISPLAY_NAME}':'/cvs/cds/rtcds/caltech/c1/medm/c1sus/master/C1SUS_ITMX_INMATRI
X_MASTER.adl',
# The channel name of the matrix element
# ($V and $H are replaced to the numbers i.e. "_3_4")
'${MATRIX_CHAN}':'C1:SUS-ITMX_INMATRIX_$V_$H'
};
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Attachment 1: kissel_button.png
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4820
|
Wed Jun 15 00:50:11 2011 |
Koji | HowTo | Computer Scripts / Programs | Kissel Button Generator |
Now the Kissel-button generator takes the command line arguments and options.
The script is fully documented by the usage message of the script itself.
It still needs the external supporting files "MATRIX*.adl_parts ".
Now the LSC screen has these buttons for the input and output matrices.
The command lines to generate those buttons are listed at the end of this entry as the examples.
>pwd
/opt/rtcds/caltech/c1/medm/c1lsc_tst/master/KisselButtonGenerator
>./generate_KisselButton.py -h
usage:
generate_KisselButton.py [options] end_row end_column matrix_ch_name
This generates an MEDM screen of a button with the style designed by
Jeff Kissel for his ISI screens. This button has a display of a matrix
elements. If the matrix element is non-zero it glows in green. Otherwise
its color is dark. Usually the button created by this script
is to be copy-pasted to other screens.
Three arguments have to be given:
end_row the number of the row at the end
end_column the number of the column at the end
matrix_ch_name the channel name of the matrix to be monitored
e.g. give C1:LSC-OUTPUT_MTRX for C1:LSC-OUTPUT_MTRX_1_1, ...
There are options prepared in order to control the parameters of the button.
example:
generate_KisselButton.py 6 6 C1:LSC-OUTPUT_MTRX
6x6 matrix for C1:LSC-OUTPUT_MTRX
options:
-h, --help show this help message and exit
--sr=START_ROW specify the starting row number for the button array.
[default: 1]
--sc=START_COLUMN specify the starting column number for the button array.
[default: 1]
--bw=BUTTON_WIDTH specify the pixel width of the small button. [default:
8]
--bh=BUTTON_HEIGHT specify the pixel height of the small button. [default:
8]
--dl=DISPLAY_LABEL specify the button label. [default: channel name]
--sn=SCREEN_NAME specify the file name of the screen opened when one
click the button. The relative or absolute path can be
included. [default: a name guessed from the channel
name. e.g. C1LSC_OUTPUT_MTRX.adl for C1:LSC-OUTPUT_MTRX]
>./generate_KisselButton.py --bw=3 --bh=4 --dl="RFPD InMTRX" 16 8 C1:LSC-PD_DOF_MTRX > rfpd_mtrx.adl
>./generate_KisselButton.py --sc=21 --bw=6 --bh=4 --dl="DCPD InMTRX" 27 8 C1:LSC-PD_DOF_MTRX > dcpd_mtrx.adl
>./generate_KisselButton.py --bw=4 --bh=4 --dl="Trig MTRX" 11 8 C1:LSC-TRIG_MTRX > trig_mtrx.adl
>./generate_KisselButton.py --bw=4 --bh=4 --dl="Out MTRX" 9 10 C1:LSC-OUTPUT_MTRX > output_mtrx.adl
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4826
|
Thu Jun 16 00:39:08 2011 |
Koji | Update | PEM | PEM AA Board has been diagnosed and fixed |
As seen in the photo, the board has a strange bulge on the board,
and the color of the internal line around the bulge got darkened.
I don't trust this board any more. We should switch to the alternative one.
Quote: |
Steve will re-install the board in the rack in the morning.
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|
4827
|
Thu Jun 16 00:43:36 2011 |
Koji | Update | SUS | Vertex SUS Binary Output Boxes were turned off / need investigation |
- I was investigating the SUS whitening issue.
- I could not find any suspension which can handle the input whitening switch correctly.
- I went to 1X5 rack and found that both of the two binary output boxes were turned off.
As far as I know they are pulling up the lines which are switched by the open collector outputs.
- I tried to turn on the switch. Immediately I noticed the power lamps did not work. So I need an isolated setup to investigate the situation.
- The cables are labelled. I will ask steve to remove the boxes from the rack. |
4829
|
Thu Jun 16 23:19:09 2011 |
Koji | Update | SUS | Vertex SUS Binary Output Boxes removed |
[Jamie, Koji]
- We found the reason why some of the LEDs had no light. It was because the LEDs were blown as they were directly connected to the power supply.
The LEDs are presumably designed to be connected to a 5V supply (with internal current-limiting resistor of ~500Ohm). The too much current
with the 15V (~30mA) made the LED blown, or the life-time of them shorter.
- Jamie removed all of the BO modules and I put 800Ohm additional resister such that the resultant current is to be 12mA.
The LEDs were tested and are fine now.
- The four BO boxes for C1SUS were restored on the rack. I personally got confused what should be connected where
even though I had labeled for BO0 and BO1. I just have connected CH1-16 for BO0. The power supplies have been connected only to BO0 and BO1.
- I tested the whitening of PRM UL sensor by exciting PRM UL sensor. The transfer function told us that the pendulum response can be seen
up to 10-15Hz. When the whitening is on, I could see the change of the transfer function in that freq band. This is good.
So the main reason why I could not see theis was that the power supply for the BOs were not turned on.
- I suppose Jamie/Joe will restore all of the BO boxes on the racks tomorrow. I am going to make a test script for checking the PD whitenings. |
4834
|
Fri Jun 17 23:20:05 2011 |
Koji | Update | LSC | Some updates of the LSC screen |
Some updates of the LSC screen
- Signal amplitude monitor for the PD signals (--> glows red for more than 1000)
- Kissel Buttons for the main matrices
- Trigger display at the output of the DOF filters
- Signal amplitude monitor for the SUS LSC output (--> glows red for more than 10000)
ADC Over flow monitor is showing some unknown numbers (as ADCs are handled by IOPs).
I asked Joe for the investigation (and consideration for the policies) |
Attachment 1: screen.png
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|
4841
|
Mon Jun 20 13:48:25 2011 |
Koji | Update | ABSL | I-P curve of LightWave M126-1064-700 |
Hmm. Was the current within the operating range? (i.e. Is it a 700mW laser or a 1W one?)
You can obtain the nominal operating current from the old EPICS values (or some elog entries).
Note that NPROs are designed to be healthy only at around the nominal pumping power
(i.e. thermal gradient, and thermal lensing of the crystal, etc.)
ALSO:
Be aware that this laser should be used under the old SOP. So the appropriate interlocking is mandatory.
And probably we need to modify the SOP such that it reflects the latest situation.
Quote: |
The I-P curve of the LightWave NPRO, which was taken out from the MOPA box, was measured. It looks healthy.
The output power can go up to about 1 W, but I guess we don't want it to run at a high power to avoid any further degradation since the laser is old.
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4873
|
Thu Jun 23 23:54:29 2011 |
Koji | Omnistructure | Environment | We are saved |
Sonali, Ishwita, and another anonymous SURF saved the long-lasted water shortage of the 40m |
Attachment 1: IMG_0023.jpg
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4905
|
Wed Jun 29 00:35:36 2011 |
Koji | Update | LSC | new LSC overview screen 80% done |
New LSC screen is 80% completed.
It is now accessible from the LSC menu of "sitemap".
Most of the part in the screen is clickable such that it launches another screen depending on the location of the click.
The bottom part of the screen still need some work.
RFPD screen is temporary
LSC control screen is also temporary
DAC overflow indicators are still broken.
Channel assignment of the whitening filters are arbitrary so far.
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Attachment 1: LSC_OVERVIEW.png
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4912
|
Wed Jun 29 14:43:12 2011 |
Koji | Update | LSC | LSC model updated |
LSC model has been updated and running,
- Now the power and signal recycling cavity lengths are named "PRCL" and "SRCL" in stead of three letter names without "L".
- Names for the trigger monitor were fixed. They are now "C1:LSC-DARM_TRIG_MON", etc., instead of "...NORM"
- Channel order of the DC signals for PDDC_MTRX and TRIG_MTRX were changed.
It was "TRX, TRY, REFL, AS, POP, POX, POY" but now "AS, REFL, POP, POX, POY, TRX, TRY".
We should change the locking script to accomodate these changes. |
4915
|
Thu Jun 30 00:58:19 2011 |
Koji | Summary | LSC | LSC whitening filter test |
[Jenne, Koji]
We have tested the LSC whitening filters. In summary, they show the transfer functions mostly as expected (15Hz zerox2, 150Hz pole x2).
Only CH26 (related to the slow channel "C1:LSC-PD9_I2_WhiteGain. VAL NMS", which has PD10I label in MEDM) showed different
phase response. Could it be an anti aliasing filter bypassed???
The 32 transfer functions obtained will be fit and summarized by the ZPK parameters.
Method:
The CDS system was used in order to get the transfer functions
- For this purpose, three filter modules ("LSC-XXX_I", "LSC-XXX_Q", "LSC-XXX_DC") were added to c1lsc
in order to allow us to access to the unused ADC channels. Those filter modules have terminated outputs.
The model was built and installed. FB was restarted in order to accomodate the new channels.
- Borrow a channel from ETMY UL coil output mon. Drag the cable from the ETMY rack to the LSC analog rack.
- Use 7 BNC Ts to split the signal in to 8 SMA cables.
- Put those 8 signals into each whitening filter module.
- The excitation signal was injected to C1:SUS-ETMY_ULCOIL_EXC by AWGGUI.
- The transfer functions were measured by DTT.
- The excitation signal was filtered by the filter zpk([150;150],[15;15],1,"n")
so that the whitened output get flat so as to ensure the S/N of the measurement.
- For the switching, we have connected the CONTEC Binary Output Test board to the BIO adapter module
in stead of the flat cable from the BIO card. This allow us to switch the individual channels manually.
- The whitening filters of 7 channels were turned on, while the last one is left turned off.
- We believe that the transfer functions are flat and equivalent if the filters are turned off.
- Use the "off" channel as the reference and measure the transfer functions of the other channels.
- This removes the effect of the anti imaging filter at ETMY.
- Once the measurement of the 7 channels are done, switch the role of the channels and take the transfer function for the remaining one channel.
Result:
- We found the following channel assignment
- The ADC channels and the PDs. This was known and just a confirmation.
- The ADC channels and the WF filter on MEDM (and name of the slow channel)
- We found that the binary IO cable at the back of the whitening filter module for ADC CH00-CH07 were not connected properly.
This was because the pins of the backplane connector were bent. We fixed the pins and the connector has been properly inserted.
- CH26 (related to the slow channel "C1:LSC-PD9_I2_WhiteGain. VAL NMS", which has PD10I label in MEDM) showed different
phase response from the others although the amplitude response is identical.
Summary of the channel assignment (THEY ARE OBSOLETE - SEPT 20, 2011)
ADC Whitening Filter
CH PD name in medm related slow channel name for gain
---------------------------------------------------------------------------
00 POY11I PD1I C1:LSC-ASPD1_I_WhiteGain. VAL NMS
01 POY11Q PD1Q C1:LSC-ASPD1_Q_WhiteGain. VAL NMS
02 POX11I PD2I C1:LSC-SPD1_I_WhiteGain. VAL NMS
03 POX11Q PD2Q C1:LSC-SPD1_Q_WhiteGain. VAL NMS
04 REFL11I PD3I C1:LSC-POB1_I_WhiteGain. VAL NMS
05 REFL11Q PD3Q C1:LSC-POB1_Q_WhiteGain. VAL NMS
06 AS11I PD4I C1:LSC-ASPD2_I_WhiteGain. VAL NMS
07 AS11Q PD4Q C1:LSC-ASPD2_Q_WhiteGain. VAL NMS
08 AS55I AS55_I C1:LSC-ASPD1DC_ WhiteGain. VAL NMS
09 AS55Q AS55_Q C1:LSC-SPD1DC_ WhiteGain. VAL NMS
10 REFL55I PD3_DC C1:LSC-POB1DC_ WhiteGain. VAL NMS
11 REFL55Q PD4_DC C1:LSC-PD4DC_ WhiteGain. VAL NMS
12 POP55I PD5_DC C1:LSC-PD5DC_ WhiteGain. VAL NMS
13 POP55Q PD7_DC C1:LSC-PD7DC_ WhiteGain. VAL NMS
14 REFL165I PD9_DC C1:LSC-PD9DC_ WhiteGain. VAL NMS
15 REFL165Q PD11_DC C1:LSC-PD11DC_ WhiteGain. VAL NMS
16 NC (named XXX_I) PD5I C1:LSC-SPD2_I_WhiteGain. VAL NMS
17 NC (named XXX_Q) PD5Q C1:LSC-SPD2_Q_WhiteGain. VAL NMS
18 AS165I PD6I C1:LSC-SPD3_I_WhiteGain. VAL NMS
19 AS165Q PD6Q C1:LSC-SPD3_Q_WhiteGain. VAL NMS
20 REFL33I PD7I C1:LSC-POB2_I_WhiteGain. VAL NMS
21 REFL33Q PD7Q C1:LSC-POB2_Q_WhiteGain. VAL NMS
22 POP22I PD8I C1:LSC-ASPD3_I_WhiteGain. VAL NMS
23 POP22Q PD8Q C1:LSC-ASPD3_Q_WhiteGain. VAL NMS
24 POP110I PD9I C1:LSC-PD9_I1_WhiteGain. VAL NMS
25 POP110Q PD9Q C1:LSC-PD9_Q1_WhiteGain. VAL NMS
26 NC (named XXX_DC) PD10I C1:LSC-PD9_I2_WhiteGain. VAL NMS
27 POPDC PD10Q C1:LSC-PD9_Q2_WhiteGain. VAL NMS
28 POYDC PD11I C1:LSC-PD11_I_WhiteGain. VAL NMS
29 POXDC PD11Q C1:LSC-PD11_Q_WhiteGain. VAL NMS
30 REFLDC PD12I C1:LSC-PD12_I_WhiteGain. VAL NMS
31 ASDC ASDC C1:LSC-PD12_Q_WhiteGain. VAL NMS
---------------------------------------------------------------------------
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Attachment 1: chans_24_31_WeirdPhase.pdf
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Attachment 2: Octopus.jpg
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Attachment 3: Test_Inputs_Plugged_In.jpg
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Attachment 4: Contec_Tester_Board.jpg
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4970
|
Fri Jul 15 01:11:21 2011 |
Koji | Summary | SUS | Photosensor Head Lessons |
Rotate the PDs and the LED so that you can put them as close as possible.
This is to increase the sensitivity of the sensor. Think why the closer the better. |
5003
|
Wed Jul 20 18:44:54 2011 |
Koji | Summary | SUS | Weekly Summary |
Find Frank and ask him about those components. |
5064
|
Sat Jul 30 00:33:33 2011 |
Koji | Update | PSL | ABSL Laser crystal temp left largely excited & left unattended for more than 3hours |
I found that the ref cav trans CCD view was blinking with 30-50 fringe amplitudes. This meant the laser freq was swinging ~50GHz.
I checked the ABSL laser and the SG out of a lock-in amplifier was connected to the slow input.
This was shaking the laser temp from 29degC to 46degC. This was the cause of the fringe swinging.
This big excitation changing the output power too as the temp was changed across it mode-hop region.
I have disconnected the excitation from the laser no matter how useful experiments were took place as there was no e-log entry about this.
I need the explanations
1. Why our precious laser is exposed to such a large swing of temperature?
2. Why the excitation is left like that without any attendance?
3. Why there was no elogging about this activity? |
5086
|
Mon Aug 1 23:26:32 2011 |
Koji | Update | LSC | REFL33 PD |
Old MZ PD (InGaAs 2mm, @29.5MHz) has been modified for REFL33.
There has been no choice for the 11MHz notch other than putting it on the RF preamp
as the notch in parellel to the diode eats the RF transimpedance at 33MHz.
I wait for judgement of Rana if the notch at the MAX4107 feedback is acceptable or not.

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Attachment 1: REFL33_schematic_110801_KA.pdf
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5101
|
Wed Aug 3 02:20:33 2011 |
Koji | Update | LSC | REFL165 PD |
REFL165 PD has been made from the old 166MHz PD.
As the required inductance was ~10nF level, the stray inductance of the circuit pattern was significant.
So, I am not so confident with the circuit functionality before the optical transfer function test.
I will test REFL33 and REFL165 with the Jenne laser to see how they work.


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Attachment 1: REFL165_schematic_110802_KA.pdf
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5108
|
Wed Aug 3 12:37:57 2011 |
Koji | Summary | SUS | Weekly Summary |
I vote for making an adapter plate between the sliding plate and the bottom base.
Quote: |
This morning, I realized that the current set-up of the horizontal shaker does not allow for the TT to be securely mounted. I was going to change the drill holes in the horizontal slider base (1 inch pitch). Jamie has suggested that it is better to make a pair of holes in the base larger. The circled holes are the ones that will be expanded to a 0.26" diameter so that I can mount the mirror securely to the horizontal slider base. There is a concern that a bit of the TT suspension base will hang over the edge of the horizontal sliding plate. We are not sure if this will cause problems with shaking the mirror evenly. Suggestions/advice are appreciated.
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5112
|
Wed Aug 3 22:22:47 2011 |
Koji | Update | LSC | REFL165 PD |
This REFL165 was good in terms of RF, but I forgot to make the DC path functioning.
I will try some ideas to fix this tomorrow. |
5113
|
Wed Aug 3 22:31:38 2011 |
Koji | Update | LSC | REFL33 PD |
REFL33 is ready for the installation
Characterization results of REFL33 is found in the PDF attachment.
Resonance at 33.18MHz
Q of 6.0, transimpedance 2.14kOhm
shotnoise intercept current = 0.52mA (i.e. current noise of 13pA/rtHz)
Notch at 10.97MHz
Q of 22.34, transimpedance 16.2 Ohm
Notch at 55.60MHz
Q of 42.45, transimpedance 33.5 Ohm
|
Attachment 1: REFL33_test_110801_KA.pdf
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5117
|
Thu Aug 4 09:42:19 2011 |
Koji | Update | ABSL | ABSL Laser shutter closed |
The shutter of the ABSL laser is closed for the vent work. |
5121
|
Fri Aug 5 04:03:16 2011 |
Koji | Update | LSC | REFL165 PD |
REFL165 PD was made and tested. The characterization results are in the PDF file.
Resonance at 166.12MHz
Q of 7.3, transimpedance 667Ohm (Series Resistance = Z/Q2 = 2.5Ohm)
shotnoise intercept current = 4.3mA (i.e. current noise of 36pA/rtHz)
As the circuit pattern had ~10nH level strain inductance, some technique was needed.
- The diode was pushed in so as to reduce the lengths of the legs as short as possible.
- The inductor for the resonant circuit has been located as close to the photodiode as possible
- The other side of the inductor was needed to be bypassed by a large (0.1uF) capacitor, as the original circuit pattern (D1-L5-C33//R22) was too skinny and long.
- C32 is also moved next to the diode.
- The path of the photo current circuit was made thicker by Cu tapes.
Now the size of the loop for the resonant circuit is comparable with the size of SOIC-8 opamp.
(Left-Top corner of the photo)
This improved the resonant gain by factor of 8.5dB at the test with TEST INPUT. (Analyzer photo)
There is no tunable component.
The resonant freq was adjusted by a parallel inductance (270nH) to the main inductor (15nH).


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Attachment 3: REFL165_test_110804_KA.pdf
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5155
|
Tue Aug 9 15:14:46 2011 |
Koji | Update | General | in-vac work plan today |
This morning Kiwamu and I have aligned the MC. Kiwamu aligned the last steering (on the OMC table) to recover the touch last week.
Then I have aligned the MC with MC1 and MC3 as the last steering did not help to get TEM00.
Before
C1:SUS-MC1_PIT_COMM = 2.6587
C1:SUS-MC1_YAW_COMM = 2.7471
C1:SUS-MC2_PIT_COMM = 3.486
C1:SUS-MC2_YAW_COMM = -1.1592
C1:SUS-MC3_PIT_COMM = -1.876
C1:SUS-MC3_YAW_COMM = 1.2829
After
C1:SUS-MC1_PIT_COMM = 2.7596
C1:SUS-MC1_YAW_COMM = 2.6627
C1:SUS-MC2_PIT_COMM = 3.486
C1:SUS-MC2_YAW_COMM = -1.1592
C1:SUS-MC3_PIT_COMM = -1.697
C1:SUS-MC3_YAW_COMM = 1.2901
Quote: |
We will move on to the vertex region today.
The goal of the vertex region work is to get the pick-off beams out the chambers, including POX/Y and POP.
The work will be in parallel to the ETM woks.
The first step will be : lock and align MC with the IR beam.
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|
5163
|
Wed Aug 10 01:40:40 2011 |
Koji | Update | SUS | ETMY exploration |
[Rana Koji Jenne Jamie]
- The situation of the ETMY suspension is improved.
- The damping servos except for Pitch are now functional.
- We intentionally turned off the damping servos for the matrix measurements.
- Opened the light door of the ETMY chamber.
- We set up the CDS SUS lockin:
Excite UL/UR/LL/LR equally [by setting the output matrix (1, 1, 1, 1, 0)] at 3.12Hz with 2000 cnts
Put the OSEM PD outputs into lockin one by one. For the image rejection, 0.1Hz 4th order LPF has been used though we like to use a faster settling LPF.
- Found only UL was responding to the excitation. After fitzing with the cables and connectors, it was found that the DAC card was loose from the bus.
By pushing the card the responses have been back. [Note we had the reboot of c1iscey almost at the same time.]
- Checked the response in the I channel of the lockin.
UL -8ish / UR +7ish / LR +5ish / LL +2ish
- Tweaked LL sensor to get better response ==> in vain. Decided to move the lower OSEM plate for the better positioning of the LR/LL.
- Got reasonable (+5ish) response for LL.
- Confirmed that the POS/YAW/SIDE damping works with positive gains. PITCH did not work with the negative gain (but that could be a good sign.)
- Let the suspension freely swinging for a while (~30min). Checked the side/pos separation. They are not perfect but seemed diagonalizable.
- Closed the light door.
- Jenne will make a better kick/free-swing test later. |
5192
|
Thu Aug 11 14:32:12 2011 |
Koji | Summary | SUS | Photosensor Head Calibration Curve for TT Frame |
The entry was quite confusing owing to many misleading wordings.
- The PS2 should be calibrated "as is". (i.e. should be calibrated with the frame)
- The previous calibrations with the highly reflective surface were 0.32V/mm and 0.26V/mm, respectively.
This time you have 0.10V/mm (with an undescribed surface). The ratio is not 32 but 3.2.
- The DC output of PS2 on the shaking setup was 2.5V. The DC output seen in the plot is 3.5V-ish.
This suggests the possibiliteies:
1) The surface has slightly higher reflectivity than the frame
2) The estimation of the distance between the frame and the PS2 during the TF measurement was not accurate.
- The word "DC coupling level" is misleading. I guess you mean the DC value of the vbration isolation transfer function
of the suspension.
Quote: |
I have re-calibrated the photosensor I used to measure the displacements of the TT frame (what I call "Photosensor 2").
As before, the linear region is about 15.2mm to 25.4mm. It is characterized by the slope -0.0996 V/mm (-0.1 V/mm). Recall that photosensor 1 (used to measure mirror displacements) has a calibration slope of -3.2V/mm. The ratio of the two slopes (3.2/0.1 = 32). We should thus expect the DC coupling level to be 32? This is not what we have for the DC coupling levels in our data (2.5 for flexibly-supported, fully-assembled TT (with EDC, with bar), 4.2 for EDC without bar, 3.2 for rigid EDC without bar, 3.2 for no EDC, with bar, 3.2 for no EDC without bar) . I think I may need to do my calibration plot for the photosensor at the frame?

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5198
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Thu Aug 11 18:30:40 2011 |
Koji | Update | SUS | ITMY OSEM adjustment |
[Jamie, Koji]
ITMX OSEMs were adjusted so as to have the right DC numbers and the more uniform response to POS excitation.
It is waiting for the free-swinging test.
- ITMX was moved from its position to the north side of the table.
- The table was rebalanced.
- We found that the output of the LR OSEM has an excess noise compared with the other OSEMs.
We tried to swap the LR and SD OSEMs, but the SD OSEM (placed at the LR magnet) showed
the same excess noise at around 10-50Hz.
- We found that one of the EQ stops was touching the mirror. By removing this friction, all of the OSEMs
come to show similar power spectra. Good!
- Then we started to use LOCKIN technique to measure the sensitivity of the OSEMs to the POS excitation.
Originally the response of the OSEMs was as follows
UL 3.4 UR 4.3
LL 0 LR 2.5
After the adjustment of the DC values, final values became as follows
UL 3.9 UR 4.4
LL 3.9 LR 3.2
- We decided to close the light door. |
5224
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Sat Aug 13 19:08:01 2011 |
Koji | Summary | SUS | TT Optimization Curves |
What are the parameters you are using? As you have the drawings of the components, you can calculate the masses of the objects.
Reducing the ECD resonance from 10Hz->6Hz looks nice.
The resonant freq of the ECDs are not (fully) determined by the gravitational energy but have the contribution of the elastic energy of the wire.
Q1: How much is the res freq of the ECDs if the freq is completely determined by the grav energy? (i.e. the case of using much thinner wires)
Q2: How thin should the wires be? |
5226
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Sat Aug 13 21:48:17 2011 |
Koji | Summary | SUS | TT Optimization Curves |
1) Drawing has the dimensions => You can calculate the volume => You can calculate the mass
Complicated structure can be ignored. We need a rough estimation.
2) Your restoring force can have two terms:
- one comes from the spring constant k
- the other from the gravity
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5336
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Fri Sep 2 15:56:32 2011 |
Koji | Update | IOO | triple resonant box : ready to install |
What are the reflected RF powers for those frequencies?
Is the 29.5MHz more problem than the 55MHz, considering the required modulation depth?
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5431
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Fri Sep 16 11:15:12 2011 |
Koji | Update | IOO | PZT1 situation |
[Koji Kiwamu]
- We have checked the situation of the broken Piezo Jenna PZT (called PZT1)
- Tested PZT1 by applying a dc voltage on the cables. Found that pitch and yaw reasonably moving and the motions are well separated each other.
The pitch requires +20V to set the IPPOS spot on the QPD center.
- Made a high-voltage (actually middle voltage) amp to convert +/-10V EPICS control signal into -5 to +30V PZTout. It is working on the prototype board and will be put into the actual setup soon.
Details:
- The Piezo Jenna driver box has 4 modules. From the left-hand side, the HV module, Yaw controller, Pitch controller, and Ben abbot's connector converter.
- We checked the voltage on Ben's converter board. (Photo1)
It turned out that the red cable is the one have the driving voltage while the others stays zero.
- We hooked a 30V DC power supply between the red cable and the shield which is actually connected to the board ground.
- Applying +/-10V, we confirmed the strain gauge is reacting. If we actuated the pitch cable, we only saw the pitch strain gauge reacted. Same situation for yaw too.
- Kiwamu went to IPPOS QPD to see the spot position, while I change the voltage. We found that applying +20V to the pitch cable aligns the spot on the QPD center.
------------------------
- I started to make a small amplifier boards which converts +/-10V EPICS signals into -5V to +30V PZT outs.
- The OPAMP is OPA452 which can deal with the supply voltages upto +/-40V. We will supply +/-30V. The noninerting amp has the gain of +2.
- It uses a 15V zener diode to produce -15V reference voltage from -30V. This results the output voltage swing from -5V to +35V.
The actual maximum output is +30V because of the supply voltage.
- On the circut test bench, I have applied +/-5V sinusoidal to the input and successfully obtained +5V to +25V swing.
- The board will be put on Ben's board today. |
Attachment 1: P9151574.JPG
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Attachment 2: P9161576.JPG
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Attachment 3: P9161577.JPG
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5447
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Sat Sep 17 14:04:45 2011 |
Koji | Update | IOO | PZT1 driver in place |
The PZT driver is now in place. The actual PZTs are not connected yet!
It is accommodated on Ben's connector adapter board.
The panel has additional connectors now: two inputs and a power supply connector.
The supply voltage is +/-30V (actual maximum +/-40V), and the input range is +/-10V
which yields the output range of -5V to 30V. The gain of the amplifier is +2.
It is confirmed that the HV outputs react to the epics sliders although the PZT connector is not connected yet
so as not to disturb the locking activity.
When we engage the PZT connector, we should check the HV outputs with an oscilloscope to confirm they
have no oscillation with the capacitances of the PZTs together with the long cable. |
Attachment 1: P9171579.JPG
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Attachment 2: P9171580.JPG
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5449
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Sun Sep 18 15:34:09 2011 |
Koji | Update | Adaptive Filtering | Modifications to LSC, RFM models, added OAF model |
[Koji Kiwamu]
This modification of the LSC model made the rows of the LSC output matrix shifted. This caused the ASS scripts nonfunctional.
Kiwamu fixed the channel names in the ASS script.
Quote: |
[Jenne, Mirko, with supervision from Jamie]
I modified the c1lsc model to have shmem outputs that go from the degrees of freedom to the OAF, and shmem inputs from the OAF's output to sum into the DoFs, just like Yoichi's FF stuff. I also removed the old OAF_OUT, because it would only allow me to select one DoF at a time, and I will eventually want the ability to do multiple amounts of OAFing at the same time. Hopefully.
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5450
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Sun Sep 18 15:57:00 2011 |
Koji | Update | IOO | The PZT driver engaged to PZT1 |
[Koji Kiwamu]
The pzt driver for PZT1 has been installed.
As there was unknown resistive connection in the vacuum chamber as described below,
the PZT out cable at the PJ driver module should always be disconnected.
The sensor cables have no problem to be connected to the controller.
In fact, they are a good monitor for the state of the PZTs.
In this configuration, Pitch and Yaw direction of PZT1 is under the control of the EPICS value as we expected.
Details:
- At the beginning, we tested the PZT driver output with low voltage level (~10V). We did not see any oscillation of the opamps.
The pitch output was observed to be OK, while the YAW output exhibited a half of the expected output voltage.
The opamp was holding correct voltage, however the voltage after the 1K output resister was about a half.
This indicated there was a voltage division happening.
- The cause of the voltage division was tracked. We found that the yaw red (=hot) line is connected to pitch black
in the vacuum chamber with a resistance of 1.4kOhm. The black cables are shorted to the ground level in the PJ driver.
- We decided to unplug the PJ's cable so that we can isolate the black cables while hoping the PZTs were drived only
by the red and white cables. And they did.
- This means that we should not connect the PZT driving cable to the PJ's driver. The sensors have no problem to be connected.
- Pinouts:
DSUB25
|. .|
|. .|
|. o| 5
|o | 17
| o| 4
|o | 16 Yaw Black
| o| 3 Pitch Black
|o | 15 Yaw White
| o| 2 Yaw Red
|o | 14 Pitch White
\ o| 1 Pitch Red
\-+
* Pitch White and Yaw White are connected to the ground at the amplifier side.
* Yaw Red and Pitch Black is connected with 1.4kOhm and isolated from the others.
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5451
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Sun Sep 18 16:42:00 2011 |
Koji | Bureaucracy | Environment | Clean up your mess |
Mess in the lab is increasing. Kiwamu and I had to clean up some stuffs to continue our work.
(i.e. some components were disturbing to open the lid of the tables.)
Basically the tools/equipments/component/cables/digital cameras/lens caps/IR viewers
you have used for the day should be cleaned up at the end of the day.
If one likes to leave a temporary stuff, leave a note to indicate by whom, for what, how long
it will be kept like that, and when one is going to back there with contact info like the cell phone #. |
5473
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Tue Sep 20 02:21:10 2011 |
Koji | Update | LSC | LSC MEDM screen cleaning up |
I have made some cleaning up of the LSC-related MEDM screens.
- LSC overview screen: ADC OVFL and WFAA indicators are now correctly matched to it associated PD signals.
- Whitening screens now have the correct indication of the associated PD signals.
- LSC Ctrl screen, which is invoked from the overview screen by clicking the servo filters, now has the switches of the servo filters.
- LSC tab of the sitemap was cleaned up by removing the broken links. |
5481
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Tue Sep 20 15:39:57 2011 |
Koji | Update | SUS | free swinging test in vacuum condition |
Can't we use Yuta's auto-Q adjust script?
http://nodus.ligo.caltech.edu:8080/40m/3723
Edit by KI :
Of course we can use it but first we have to fix some pynds sentences since his script was written for the OLD pynds. |
5492
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Tue Sep 20 23:59:53 2011 |
Koji | Summary | LSC | Plan to update the LSC code for multiple lock-ins |
DRMI team needs to use at least three lockins on LSC
Increase the number of the lockin matrix done
Duplicate lockin modules in the LSC code done
modify the main LSC screen done
modify the lockin screen done
modify the lockin matrix screen done
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5498
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Wed Sep 21 14:28:25 2011 |
Koji | Summary | LSC | The LSC code/screen modification for LSC LOCKINs |
The LSC code has been modified
- The code was modified, compiled, and installed.
- The code is now running. FB was restarted to deal with the change of the channel names.
- Now we have LOCKIN1, 2, and 3. This required the change of the names from C1:LSC-LOCKIN_.... to C1:LSC-LOCKIN1_...
- The LSC screen has also modified. It has three lockins on the screen.
- The corresponding matrix screens have been modified/created and linked from the main screen.
- I need to make the screens more cool but the locking team can start to use those lockins. |
5516
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Thu Sep 22 11:50:37 2011 |
Koji | Update | LSC | Locking status update |
Both loops basically have no phase margins. i.e. unstable. How can you lock PRMI with these servos?
Quote: |
The following rough swept sine plots are the OLTs for MICH and PRCL. The gain setting was -10 and 0.5 for MICH and PRCL, respectively. Integrators were off. Looking at the measured plots, MICH has about 300 Hz UGF, when the gain is -20, and PRCL has about 300 HZ UGF, too, when the gain is 0.8.
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5522
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Thu Sep 22 18:33:01 2011 |
Koji | Summary | LSC | The LSC screen modification |
As per the request of Anamaria, I have added the slider of the demodulation phase for each RF PD screens. |
Attachment 1: PD_screen.png
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5528
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Thu Sep 22 23:18:51 2011 |
Koji | Summary | LSC | The LSC screen modification |
C1LSC_RFPD.adl screen was modified to have more information. |
Attachment 1: C1LSC_RFPD.png
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5539
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Sat Sep 24 17:12:54 2011 |
Koji | Update | LSC | Realignment of REFL / Some 3f PRMI locking / Recycling Gain |
[Koji Suresh]
Activity on Friday evening
- The REFL path has been thoroughly aligned
As I did not like the REFL spot misaligned on the REFL CCD, we went to the AP table.
Many optics had the spots not on the middle of the optic, including the PBS whose post was not fixed on the post holder.
We aligned the optical paths, the RF PDs, and the CCD. The alignment of the PD required the use of the IR viewer.
One should not trust the DC output as a reference of the PD alignment as it is not enough sensitive to the clipping.
We aligned the optical paths again after the reasonable alignment of PRM is established with the interferometer.
"Next time when you see REFL spot is not at the center of the camera, think what is moved!"
- The REFL165 PD is disconnected from the power supply
I found that the REFL165 PD is producing 7.5V output at the DC monitor no matter how the beam is blocked.
As I could not recover this issue by swapping the power connector at the LSC rack, I disconnected the cable
at the RFL165 PD side. I need to go through the PD power supply circuit next week.
- PRMI alignment policy of the night
Kiwamu has aligned Y-arm some time ago (Thursday evening?). I decided not to touch ITMY.
So the Michelson is aligned by ITMX, PRC is aligned by PRM.
- Michelson locking
The short Michelson was locked with AS55Q and the MICH filter. We could use the gain of +/-20 for locking,
and could increase it up to ~+/-250. At the max gain, the all three integrators and the two resonant gains
could be activated. The sign depends on which fringe you want at the AS port (bright or dark).
In this condition, the output of the POXDC channel (which is actually the POY DC out -- c.f. This entry)
is used to determine the internal power. It was ~70cnt.
- PRMI locking
Then the PRMI was locked. There was some confusion of the gains because of the limitters at the servo filters
(which yielded the locking with 1bit outputs no matter how much the gains were....)
After all, I decided to use REFL33I for the PRCL for the test. The PRCL gain was -0.3~-1.0 for the carrier lock, but
was highly dependent on the alignment. i.e. if accidentally hit the high power recycling gain, it oscillated easily
and the lock was lost. Probably this was the first 3f locking at the 40m in the current optical config, if
Kiwamu did not do that secretly. The SB lock was also obtained by flipping the sign of the PRCL servo.
The difficulty we had was the instability when the recycling gain became big. We were monitoring the POXDC
(i.e.DCout of the POY PD). When this exceeds 5000, many glitches appears in the LSC signals and disturbs the lock.
This was not the fringes from neither the arms nor the SRC.
The observed POY DC with the carrier resonant PRMI was 5000~8000vcnt (momentary). |
5541
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Sat Sep 24 20:14:36 2011 |
Koji | Update | LSC | Rough estimation of the PR gain |
POXDC (i.e. POY DCout)
PRM misaligned: 70cnt
CA resonant PRMI: ~8000cnt (max)
REFLDC
PRMI antiresonant = 5200cnt
PRMI resonant = ~3000cnt
==> Visivility = 0.6
PRM
Transmissivity: TR=0.0575, tR=sqrt(TR)
Rough estimation of the power recycling gain (assuming perfect mode matching)
PPRM_mialign = Pin tR2
PPRM_resonant = Pin [tR/(1-rR rMI)]2
G = tR2 PPRM_resonant / PPRM_mialign = 8000/70*0.0575 = 6.5
This is way too low compared with the design (G>40)
This corresponds to rMI2=0.885 (loss of 10%) in the power recycling cavity.
But this yields visibility of 16%, instead of 60% which we saw. This is inconsistent.
If mode matching is not perfect, effective incident power of PRMI decreases
and this discrepancy may be explained
Pin = Pjunk + (Pin-Pjunk)
PPRM_mialign = Pin tR2
PPRM_resonant = (Pin-Pjunk) [tR/(1-rR rMI)]2
PREFL_antires ~ Pin
PREFL_resonant = Pjunk+(Pin-Pjunk)[-rR+(tR2 rMI)/(1-rR rMI)]2
===>
PPRM_resonant / PPRM_mialign = (1-Rmm) /(1-rR rMI)2=8000/70
PREFL_resonant /PREFL_antires= Rmm+(1-Rmm)[-rR+(tR2 rMI)/(1-rR rMI)]2=0.6
here Rmm= Pjunk/Pin is the mode matching ratio
Solving the last two equations, we obtain
Rmm=0.6,
rMI2= 0.939 (loss of 4-5%)
Can we believe that the mode matching is 60% and the loss is 5%??? |
5549
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Mon Sep 26 17:49:51 2011 |
Koji | Update | PSL | c1psl |
[Koji Suresh]
c1psl has got frozen during our ezcaread/write business.
After the target was rebooted and we lost the previous setting as there was no burt snapshot for the slow targets since Dec 13, 2010.
It seems that burtrestore is essential for the bootstrapping of the MC servo, as the auto locker script refers the locking parameters
from the PSL setting values (C1PSL_SETTINGS_SET.adl).
Jenne is working on the recovery of the snap-shotting for the slow targets. |
5551
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Mon Sep 26 20:04:03 2011 |
Koji | Update | PSL | MC lock has been recovered |
[Kiwamu Suresh Koji]
Some main parameters of the PSL has been recovered using Dataviewer and some screen snapshots, as seen in the screenshots below. |
Attachment 1: snapshot1.png
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Attachment 2: snapshot2.png
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Attachment 3: snapshot3.png
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5559
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Tue Sep 27 20:02:19 2011 |
Koji | Update | SUS | Watchdog rearmed |
I came to the control room and found the PMC and IMC were unlocked. ==> Relocked
I found the watch dogs of the vertex suspensions are tripped.
I checked the data for the past 6 hours and found they are independent events.
The unlock of the MCs occured 4 hours ago and the watchdogs tripped 2 hours ago.
The suspension damping was restored at around 7:50PM PDT. |
5584
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Fri Sep 30 08:40:02 2011 |
Koji | Update | LSC | length fluctuations in MICH and PRCL |
Tip-Tilts has almost no isolation up to 3Hz, and isolation of about 0.5 up to 10Hz.
They have vertical resonances at around 20Hz.
See Nicole's entry
Quote: |

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