ID |
Date |
Author |
Type |
Category |
Subject |
5785
|
Wed Nov 2 14:07:25 2011 |
Zach | Update | elog | restarted |
Elog was hanging, restarted with the script. |
5902
|
Wed Nov 16 01:45:37 2011 |
Zach | Update | elog | restarted |
Elog was hanging. Restarted it with script. |
5903
|
Wed Nov 16 02:36:35 2011 |
Koji | Update | elog | restarted |
Basically, elog hangs up by the visit of googlebot.
Googlebot repeatedly tries to obtain all (!) of entries by specifying "page0" and "mode=full".
Elogd seems not to have the way to block an access from the specified IP.
We might be able to use http-proxy via apache. (c.f. http://midas.psi.ch/elog/adminguide.html#secure )
Or can we tweak the source of elod such that it does not accept "page0"?
GET /40m/page0?mode=full&new_entries=1 HTTP/1.1
Host: 131.215.115.52:8080
Connection: Keep-alive
Accept: */*
From: googlebot(at)googlebot.com
User-Agent: Mozilla/5.0 (compatible; Googlebot/2.1; +http://www.google.com/bot.html)
Accept-Encoding: gzip,deflate
Quote: |
Elog was hanging. Restarted it with script.
|
|
5908
|
Wed Nov 16 10:13:13 2011 |
jamie | Update | elog | restarted |
Quote: |
Basically, elog hangs up by the visit of googlebot.
Googlebot repeatedly tries to obtain all (!) of entries by specifying "page0" and "mode=full".
Elogd seems not to have the way to block an access from the specified IP.
We might be able to use http-proxy via apache. (c.f. http://midas.psi.ch/elog/adminguide.html#secure )
|
There are much more simple ways to prevent page indexing by googlebot: http://www.google.com/support/webmasters/bin/answer.py?answer=156449
However, I really think that's a less-than-idea solution to get around the actual problem which is that the elog software is a total piece of crap. If google does not index the log then it won't appear in google search results.
But if there is one url that when requested causes the elog to crash then maybe it's a better solution to cut of just that url. |
5936
|
Fri Nov 18 00:25:10 2011 |
Zach | Update | elog | restarted |
with script. |
3453
|
Sun Aug 22 16:20:24 2010 |
Zach | Update | elog | restarted (with my phone this time) |
|
4001
|
Tue Nov 30 19:35:09 2010 |
Zach | Update | elog | restarted again |
Restarted the elog again, this time using .../elog/start-elog.csh, which Joe pointed out works just fine. I have amended the wiki instructions to point to this script, instead. |
16234
|
Thu Jul 1 11:37:50 2021 |
Paco | Update | General | restarted c0rga |
Physically rebooted c0rga workstation after failing to ssh into it (even as it was able to ping into it...) the RGA seems to be off though. The last log with data on it appears to date back to 2020 Nov 10, but reasonable spectra don't appear until before 11-05 logs. Gautam verified that the RGA was intentionally turned off then. |
6091
|
Thu Dec 8 19:48:23 2011 |
kiwamu | Update | CDS | restarted c1lsc machine and daqd |
Since the c1lsc machine became frozen I restarted the c1lsc machined and daqd.
Then I burtrestored c1lsc, c1ass and c1oaf to this evening. They seem running okay. |
3989
|
Mon Nov 29 17:45:28 2010 |
Zach | Update | elog | restarted elog |
The elog was down so I restarted it. The instructions on the wiki do not work as the process has some complicated name (i.e. it is not just 'elogd'). I used kill and the pid number.
I will get around to updating the restart script to work with 2.8.0. |
4897
|
Tue Jun 28 11:25:56 2011 |
Alastair | Bureaucracy | Computers | restarted elog |
The manual instructions on the 40m wiki for restarting wouldn't work. I killed the process okay, but then I got an error saying it "couldn't bind to port 8080, please try again using -p to select port". The automated script worked though. |
5855
|
Wed Nov 9 19:08:18 2011 |
Suresh | Update | elog | restarted elog |
Elog was not responding and was restarted. |
5870
|
Fri Nov 11 00:58:19 2011 |
Den | Update | elog | restarted elog |
Elog suspended 2 times for 1 hour. Too high frequency.
Restarted. |
4741
|
Wed May 18 18:33:46 2011 |
Aidan | Update | elog | restarted elog with script |
|
7435
|
Mon Sep 24 20:28:13 2012 |
rana | Summary | elog | restarted elog: was unresponsive |
|
1932
|
Fri Aug 21 17:05:04 2009 |
Jenne | Update | General | restarted the elog |
[Kevin, Jenne]
Kevin's awesome final report/elog entry was so awesome that it crashed the elog. It has been restarted. We're going to put his pictures and documentation in the wiki, with a link from the elog to prevent re-crashing. |
2028
|
Wed Sep 30 12:21:08 2009 |
Jenne | Update | Computers | restarted the elog |
I'm blaming Zach on this one, for trying to upload a pic into the ATF elog (even though he claims it was small....) Blame assigned: check. Elog restarted: check. |
5002
|
Wed Jul 20 17:43:33 2011 |
suresh | Update | Computers | restarted the frame builder |
I restarted the frame builder in the last 15mins.
I was making a change to a DAC channel in the C1IOO model. |
5021
|
Sat Jul 23 02:24:10 2011 |
Suresh | Update | IOO | restarted the frame builder |
I restarted the fb twice during the last 15mins. This was after I added test points into the C1IOO/WFS1.mdl and C1IOO/WFS2.mdl. |
6443
|
Mon Mar 26 12:50:24 2012 |
Zach | Update | elog | restarted with script |
On the plus side, it was the first time I've had to do it in a while.. |
11838
|
Wed Dec 2 15:52:28 2015 |
yutaro | Update | LSC | restoration of POXDC |
I disconnected the cable that was connected to CH6 of the whitening filter in 1Y2, then connected POXDC cable to there (CH6). This channel is where POXDC used to connect.
Then I turned on the whitening filter for POXDC and POYDC (C1:LSC-POXDC FM1, C1:LSC-POYDC FM1) and changed the gain of analog whitening filter for POXDC and POYDC from 0 dB to 45 dB and from 0 dB to 39 dB, respectively (C1:LSC-POXDC_WhiteGain, C1:LSC-POYDC_WhiteGain). |
11930
|
Wed Jan 13 18:36:00 2016 |
gautam | Update | LSC | restoration of green beat electronics |
In preparation for tonight's work, I did the following:
On the PSL table:
- Powered the RF amplifiers for the green beat signal on
- Reconnected the outputs of the Green beat PDs to the RF amplifiers
- Restored wiring in the fiber box such that both IR beats go to the frequency counter.
At the IOO Rack area:
- Restored wiring to the frequency counter module such that the IR beats from both arms go to the respective channels
- Partially cleaned up the setup used for measuring AUX laser frequency noise - moved the SR785 to the X end along with one SR560 so that we can measure the end PDH OLTF
- Brought the HP network analyzer back to the control room so that we can view the green beatnotes.
At the X-end:
- Turned the function generator used for PDH locking back on
- Checked that the AUX laser diode current is 1.90 A, and the crystal temperature is ~47.5 degrees, both of which I think are "good" values from our AUX laser frequency noise measurements
- Did some minor manual alignment of the PZT mirrors
At the Y-end:
- Restored the BNC connection from the PDH box to the laser's "FAST" control input. The long BNC cable used for the PLL is still running along the Y-arm, I will clean this up later.
Having done all this, I checked the green transmission levels for both arms (PSL green shutter closed, after running ASS to maximize IR transmission). GTRY is close to what I remember (~0.40) while the best I could get GTRX to is ~0.12 (I seem to remember it being almost double this value - maybe the alignment onto the beat PD has to be improved?). Also, the amplitudes of the beatnotes on the network analyzer are ~-50dBm, and I seem to remember it being more like -25dBm, so maybe the alignment on the PD is the issue? I will investigate further in the evening. It remains to measure the OLTF of the X-end PDH as well. |
727
|
Wed Jul 23 21:48:30 2008 |
rob | Configuration | General | restore IFO when you're done with it |
when you are done with the IFO, please click "Restore last auto-alignment" on the yellow IFO portion of the C1IFO_CONFIGURE.adl screen. Failure to comply will be interpreted as antagonism toward the lock acquisition effort and will be met with excoriation. |
7378
|
Thu Sep 13 07:36:41 2012 |
Steve | Update | General | restore conditions |
Quote: |
Summary: Recorded the presence of higher order modes in IMC
What I did: Misaligned the flat mirror MC1 by small amount in both pitch and yaw (it was needed to be done cause at the beginning of the experiment no higher order modes were present) and scanned the cavity for frequency-range 32MHz to 45MHz.
I found the presence of higher order modes around 36.7MHz (1st order) and 40.6MHz (2nd order) along with two other strong modes near 35MHz and 42.5MHz.
|
Please, restore condition after you finished and update elog right away! People wasted hours yesterday not knowing the condition of the MC |
1510
|
Thu Apr 23 16:35:23 2009 |
Yoichi | Summary | Computer Scripts / Programs | restoreWatchdog script |
When the IFO loses lock during the lock acquisition steps, it often kicks the MC2 (through the CM servo) and trips the watchdog.
I wrote a script to restore the tripped watchdog (/cvs/cds/caltech/scripts/SUS/restoreWatchdog).
The script takes the name of a mirror (such as MC2) as an argument.
It will enable the coils and temporarily increase the watchdog threshold to a value higher than the current OSEM RMS signals.
Then it will bring the watchdog back to the normal state and wait for the mirror to be damped. After the mirror is damped enough, the
watchdog threshold will be restored to the original value.
The script will do nothing if the watchdog is not tripped.
I put this script in the drdown_bang so that the MC2 watchdog will be automatically restored when a lock loss kicks out the MC2. |
10035
|
Fri Jun 13 09:20:37 2014 |
Steve | Update | SUS | restored damping at PRM and ETMY |
ETMX medm screen values are blank. |
474
|
Tue May 13 10:15:52 2008 |
steve | Update | SUS | restored damping of BS & PRM |
I think our janitor was cleaning too heavy handedly.
The BS and PRM sus damping were lost.
They were restored. |
1553
|
Thu May 7 10:28:20 2009 |
steve | Update | VAC | retrofitted maglev's needs |
Our spare Osaka maglev purchased in Oct 2005 turned out to be having a viton o-ring seal connection on the intake.
It was shipped back to San Jose for retrofitting it with 6" conflat flange ( CF ) This CF is using copper gasket so there will be no permeation of He when you leak check the IFO
The digital controller and cable are here. The controller needs to be interfaced with the interlocks and computer system; those have been in a neglected condition lately.
see elog #1505 Historically after every REBOOT of c1vac2 the readbacks works for 3-4 days only. Fixing of this was postponed many times in the past as low priority or lack of knowledgeable
enthusiast.
The maglev TG390MCAB wil be back on Tuesday, May 4, 2009. The mourning of our fateful 360 will only end at the first levitation of the 390.
|
4562
|
Sun Apr 24 21:37:40 2011 |
kiwamu | Update | IOO | review of triple resonant EOM : model looks fine |
To design a new resonant EOM box I started reviewing the prototype that I've built.
As a part of reviewing I checked an important thing that I haven't carefully done so far :
I compared the measured input impedance with that of predicted from a circuit model. I found that they show a good agreement.
So I am now confident that we can predict / design a new circuit performance.
* * * (input impedance) * * *
Performance of a resonant circuit is close related to its input impedance and hence, in other words, determined by the input impedance.
Therefore an investigation of input impedance is a way to check the performance of a circuit. That's why I always use impedance for checking the circuit.
The plot below is a comparison of input impedance for the measured one and one predicted from a model. They show a good agreement.
(Note that the input impedance is supposed to have 50 Ohm peaks at 11, 29.5 and 55 MHz.)

* * * (circuit model) * * *
To make the things simpler I assume the following three conditions in my model:
1. inductor's loss is dominated by its DC resistance (DCR)
2. capacitor's loss is characterized only by Q-value
3. Transformer's loss is dominated by DCR and its leakage inductance
All the parameters are quoted from either datasheet or my measurement. The model I am using is depicted in the schematic below.
Basically the Q-vaules for the capacitors that I used are quite low. I think higher Q capacitors will improve the performance and bring them to more 50 Ohm.

|
3813
|
Thu Oct 28 20:08:26 2010 |
yuta | Update | Green Locking | revised RF amp cascading |
Background:
Yesterday, I said I will use ZHL-32A for amplifying beat note signal, but as Koji pointed out, ZHL-32A is for medium high power.
So I changed my mind to use ZFL-1000LN instead. ZFL-1000LN is a low noise RF amp whose maximum power is 3dBm.
Also, we included a splitter in our consideration.
What I did:
1. Set up a new setup. ZFL-1000LN has a gain of +24dB at 80MHz and splitter ZFRSC-42 has a loss of -6dB. So;
beat note signal -> ZFL-1000LN -> ZFL-1000LN -> ZFRSC-42 => SR620 and VCO
2. Measured frequency-output relation. When the input signal was 80MHz -48dBm, the output was -8.7dBm. For other frequencies;
60MHz -3.3dBm
70MHz -5.7dBm
80MHz -8.7dBm
90MHz -5.5dBm
100MHz -3.5dBm
So, we can see frequency up to >100MHz by SR620 using this setup.
3. Checked harmonics peak levels of the output using an RF spectrum analyzer. When the input signal was 80MHz -48dBm, the height of the peaks were;
80MHz -8.8dBm
160MHz -30dBm
240MHz -42dBm
Other peaks were smaller than the 3rd harmonics. Also, RF PD that detects beat note signal has a cut-off frequency at around 100MHz. So, we don't need to worry about wave transformation for this setup.
Quote: |
ZHL-32A is a high power (well..., actually middle power) amplifier with the max output power of +29dBm (~1W!).
It seems to be overkill.
Your signal is so small so you don't need ZHL-32A, but can use small amp which we may have somewhere in the lab.
And the description:
"RF amplifier ZHL-32A has around +28dBm gain at 80MHz"
The unit is wrong.
|
Yes. I corrected my previous elog. |
13282
|
Thu Aug 31 18:36:23 2017 |
gautam | Update | CDS | revisiting Acromag |
Current status:
- There is a single Acromag ADC unit installed in 1X4
- It is presently hooked up to the PSL NPRO diagnostic connector channels
- I had (re)-started the acquisiton of these channels on August 16 - but for reasons unknown, the tmux session that was supposed to be running the EPICS server on megatron seems to have died on August 22 (judging by the trend plot of these channels, see Attachment #1)
- I had not set up an upstart job that restarts the server automatically in such an event. I manually restarted it for now, following the same procedure as linked in my previous elog.
- While I was at it, I also took the opportunity to edit the Acromag channel names to something more appropriate - all channels previously prefixed with C1:ACRO- have now been prefixed with C1:PSL-
Plan of action:
- Hardware - we have, in the lab, in addition to the installed ADC unit
- 3x 8 channel differential input ADC units
- 2x 8 channel differential output DAC units
- 1x 16 channel BIO unit
- 2U chassis + connectors + breakout boards + other misc hardware that I think Johannes and Lydia procured with the original plan to replace the EX slow controls.
- Some relevant elogs: Panel designs, breakout design, sketch for proposed layout, preliminary channel list.
So on the hardware side, it would seem that we have everything we need to go ahead with replacing the EX slow controls with an Acromag system, although Johannes probably knows more about our state of readiness from a hardware PoV.
- Software
- We probably want to get a dedicated machine that will handle the EPICS channel serving for the Acromag system
- Have to figure out the networking arrangement for such a machine
- Have to figure out how to set up the EPICS server protocol in such a way that if it drops for whatever reason, it is automatically restarted
|
Attachment 1: Acromag_EPICS.png
|
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13422
|
Thu Nov 9 15:33:08 2017 |
johannes | Update | CDS | revisiting Acromag |
Quote: |
We probably want to get a dedicated machine that will handle the EPICS channel serving for the Acromag system
|
http://www.supermicro.com/products/system/1U/5015/SYS-5015A-H.cfm?typ=H
This is the machine that Larry suggested when I asked him for his opinion on a low workload rack-mount unit. It only has an atom processor, but I don't think it needs anything particularly powerful under the hood. He said that we will likely be able to let us borrow one of his for a couple days to see if it's up to the task. The dual ethernet is a nice touch, maybe we can keep the communication between the server and the DAQ units on their separate local network. |
13536
|
Thu Jan 11 21:09:33 2018 |
gautam | Update | CDS | revisiting Acromag |
We'd like to setup the recording of the PSL diagnostic connector Acromag channels in a more robust way - the objective is to assess the long term performance of the Acromag DAQ system, glitch rates etc. At the Wednesday meeting, Rana suggested using c1ioo to run the IOC processes - the advantage being that c1ioo has the systemd utility, which seems to be pretty reliable in starting up various processes in the event of the computer being rebooted for whatever reason. Jamie pointed out that this may not be the best approach however - because all the FEs get the list of services to run from their common shared drive mount point, it may be that in the event of a power failure for example, all of them try and start the IOC processes, which is presumably undesirable. Furthermore, Johannes reported the necessity for the procServ utility to be able to run the modbusIOC process in the background - this utility is not available on any of the FEs currently, and I didn't want to futz around with trying to install it.
One alternative is to connect the PSL Acromag also to the Supermicro computer Johannes has set up at the Xend - it currently has systemd setup to run the modbusIOC, so it has all the utilities necessary. Or else, we could use optimus, which has systemd, and all the EPICS dependencies required. I feel less wary of trying to install procServ on optimus too. Thoughts?
|
475
|
Tue May 13 10:38:28 2008 |
steve | Update | Computers | rfm network is down |
The RFM network went down yesterday around 5pm
Only c1susvme1 is alive but it's timing is off.
Andrey is bringing the network up.
Andrey wants to make an addition first that our situation is very much similar to that described by Rana in his elog entry # 353 (March 03). All of the rectangular boxes are red, except for SUS1-c1susvme1 and AWG (only these two rectangles are green). |
322
|
Tue Feb 19 10:14:13 2008 |
steve | Update | VAC | rga logging needs help |
The rga head and controller are running fine, but the data logging is not. |
129
|
Wed Nov 28 08:47:29 2007 |
steve | Omnistructure | VAC | rga is out of order |
The rga is not working since Nov 10
The controller is broken.
pd65-m-d23 |
Attachment 1: pd65d23.jpg
|
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1085
|
Fri Oct 24 15:05:13 2008 |
steve | Update | VAC | rga is out of order |
The old Dycor RGA is out of order.
I'm getting ready to purchase an SRS instrument. |
344
|
Thu Feb 28 13:04:59 2008 |
rob | Update | VAC | rga logging working again |
Quote: | The rga head and controller are running fine, but the data logging is not. |
It should run tonight at 1:25 AM. To get the cron job to work properly on op340m, I had to make wrapper sh script which defines the perl library before calling the actual RGAlogger script. |
76
|
Wed Nov 7 09:38:01 2007 |
steve | Update | VAC | rga scan |
pd65-m-d2 at cc1 6e-6 torr |
Attachment 1: pd65d2.jpg
|
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887
|
Tue Aug 26 15:06:16 2008 |
steve | Configuration | VAC | rga scan |
Pumpdown 66 PRM-maglev vac normal -day 11
short form: pd66PRM-m-d11 |
Attachment 1: RGA-0808260125.png
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14291
|
Tue Nov 13 16:15:01 2018 |
Steve | Update | VAC | rga scan pd81 at day 119 |
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Attachment 1: pd81-d119.png
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Attachment 2: pd81-560Hz-d119.png
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14229
|
Thu Oct 4 08:25:50 2018 |
Steve | Update | VAC | rga scan pd81 at day 78 |
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Attachment 1: pd81d78.png
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351
|
Mon Mar 3 09:25:33 2008 |
steve | Update | VAC | rga scan logging is working now |
Quote: |
Quote: | The rga head and controller are running fine, but the data logging is not. |
It should run tonight at 1:25 AM. To get the cron job to work properly on op340m, I had to make wrapper sh script which defines the perl library before calling the actual RGAlogger script. |
Thanks to Rob, it is working !
The baked, calibrated rga head
model# M206M, s/n #c128035 was reinstalled at the 40m ifo on Feb. 8, 2008
Faraday mode dwell time was increased from 2 to 16 sec
Rga head temp at top silver gaskit 45.2 C
The noise floor is at 1E-12 Torr
There is more detail in logbook VMI-14 p 107
pd65-m-d119 |
Attachment 1: rgalogworks.jpg
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Attachment 2: cc1.jpg
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1227
|
Wed Jan 14 10:59:06 2009 |
steve | Bureaucracy | VAC | rga waiting to be "connected" |
We have no RGA data since old Dycor passed away in the middle of Oct, 2008
New SRS-RGA200 was installed on the vac envelope on Nov 14, 2008
It is waiting to be software connected to the 40m logging |
1452
|
Fri Apr 3 10:01:50 2009 |
steve | Update | VAC | rgascan with temp plot |
Rga scan of day 231 since pumpdown pd66-m-d231
m stands for maglev pumping speed, vacuum normal condition of valves,
cc4 cold cathode gauge at the rga location,
cc1 is real ifo pressure from the 24" tube at the pumpspool,
PEM-count temp: vac envelope temp at the top of IOO chamber
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Attachment 1: pd66tempow.jpg
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Attachment 2: rga-090403scan.png
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7029
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Wed Jul 25 15:33:55 2012 |
janosch | Update | LSC | ringdown measurement |
We did our first ringdown measurement on the Y arm. First we tried to keep the arm locked in green during the ringdown, but for some reason it was not possible to get the cavity locked in green. So we decided to do the first measurement with infrared locked only.
For the measurement we had to change the LSC model to acquire the C1:LSC-TRY_OUT_DQ at higher sampling frequency. We changed the sampling frequencies of C1:LSC-{TRX,TRY}_OUT_DQ from 2048Hz to 16384Hz.
The measurement was done at GPS 1027289507. The ringdown curve looks very clean, but there seem to be two time constants involved. The first half of the curve is influenced by the shutter speed, then curvature is changing sign and the ringdown is likely taking over. We will try to fit a curve to the ringdown part, but it would certainly be better to have a faster shutter and record a more complete ringdown.

|
7033
|
Wed Jul 25 22:16:36 2012 |
Koji | Update | LSC | ringdown measurement |
Is this the step response of the single pole low pass???
It should have an exponential decay, shouldn't it? So it should be easier to comprehend the result with a log scale for vertical axis...
I think you need a fast shutter. It is not necessary to be an actual shutter but you can use faster thing
which can shut the light. Like PMC or IMC actuators.
Another point is that you may like to have a witness channel like the MC transmission to subtract other effect. |
7301
|
Tue Aug 28 18:28:21 2012 |
janosch | Metaphysics | Ringdown | ripples |
Let's see if the ripples observed in the MC ringdown can be due to tilt motion of the mirrors.
The time it takes to produce a phase shift corresponding to N multiples of 2*pi is given by:
t = sqrt(2*N*lambda/(L*omega_T^2*(alpha_1+alpha_2)))
L is the length of the MC (something like 13m), and alpha_1, alpha_2 are the DC tilt angles of the two mirrors "shooting into the long arms of the MC" produced by the MC control with respect to the mechanical equilibrium position. omega_T is the tilt eigenfrequency of the three mirrors (assumed to be identical). lambda = 1.064e-6m;
The time it takes from N=1 to N=2 (the first observable ripple) is given by: tau1 = 0.6/omega_T*sqrt(lambda/L/(alpha_1+alpha_2))
The time it takes from N=2 to N=3 is given by: tau2 = 0.77*tau1
etc
First, we also see in the measurement that later ripples are shorter than early ripples consistent with some accelerated effect. The predicted ripple durations tau seem to be a bit too high though. The measurements show something like a first 14us and a late 8us ripple. It depends somewhat on the initial tilt angles that I don't know really.
In any case, the short ripple times could also be explained if the tilt motions start a little earlier than the ringdown, or the tilt motion starts with some small initial velocity. The next step will be to program a little ringdown simulation that includes mirror tilts and see what kind of tilt motion would produce the ripples exactly as we observe them (or maybe tilt motion cannot produce ripples as observed). |
7302
|
Tue Aug 28 19:06:32 2012 |
Koji | Metaphysics | Ringdown | ripples |
Isn't it just a ringing of the intracavity power as you shifted the laser frequency abruptly?
Quote: |
Let's see if the ripples observed in the MC ringdown can be due to tilt motion of the mirrors.
The time it takes to produce a phase shift corresponding to N multiples of 2*pi is given by:
t = sqrt(2*N*lambda/(L*omega_T^2*(alpha_1+alpha_2)))
L is the length of the MC (something like 13m), and alpha_1, alpha_2 are the DC tilt angles of the two mirrors "shooting into the long arms of the MC" produced by the MC control with respect to the mechanical equilibrium position. omega_T is the tilt eigenfrequency of the three mirrors (assumed to be identical). lambda = 1.064e-6m;
The time it takes from N=1 to N=2 (the first observable ripple) is given by: tau1 = 0.6/omega_T*sqrt(lambda/L/(alpha_1+alpha_2))
The time it takes from N=2 to N=3 is given by: tau2 = 0.77*tau1
etc
First, we also see in the measurement that later ripples are shorter than early ripples consistent with some accelerated effect. The predicted ripple durations tau seem to be a bit too high though. The measurements show something like a first 14us and a late 8us ripple. It depends somewhat on the initial tilt angles that I don't know really.
In any case, the short ripple times could also be explained if the tilt motions start a little earlier than the ringdown, or the tilt motion starts with some small initial velocity. The next step will be to program a little ringdown simulation that includes mirror tilts and see what kind of tilt motion would produce the ripples exactly as we observe them (or maybe tilt motion cannot produce ripples as observed).
|
|
7303
|
Tue Aug 28 19:21:37 2012 |
janosch | Metaphysics | Ringdown | ripples |
Hmm. I don't know what ringing really is. Ok, let's assume it has to do with the pump... I don't see how the pump laser could produce these ripples. They have large amplitudes and so I always suspected something happening to the intracavity field. Therefore I was looking for effects that would change resonance conditions of the intracavity field during ringdown. Tilt motion seemed to be one explanation to me, but it may be a bit too slow (not sure yet). Longitudinal mirror motion is certainly too slow. What else could there be?
Quote: |
Isn't it just a ringing of the intracavity power as you shifted the laser frequency abruptly?
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Let's see if the ripples observed in the MC ringdown can be due to tilt motion of the mirrors.
The time it takes to produce a phase shift corresponding to N multiples of 2*pi is given by:
t = sqrt(2*N*lambda/(L*omega_T^2*(alpha_1+alpha_2)))
L is the length of the MC (something like 13m), and alpha_1, alpha_2 are the DC tilt angles of the two mirrors "shooting into the long arms of the MC" produced by the MC control with respect to the mechanical equilibrium position. omega_T is the tilt eigenfrequency of the three mirrors (assumed to be identical). lambda = 1.064e-6m;
The time it takes from N=1 to N=2 (the first observable ripple) is given by: tau1 = 0.6/omega_T*sqrt(lambda/L/(alpha_1+alpha_2))
The time it takes from N=2 to N=3 is given by: tau2 = 0.77*tau1
etc
First, we also see in the measurement that later ripples are shorter than early ripples consistent with some accelerated effect. The predicted ripple durations tau seem to be a bit too high though. The measurements show something like a first 14us and a late 8us ripple. It depends somewhat on the initial tilt angles that I don't know really.
In any case, the short ripple times could also be explained if the tilt motions start a little earlier than the ringdown, or the tilt motion starts with some small initial velocity. The next step will be to program a little ringdown simulation that includes mirror tilts and see what kind of tilt motion would produce the ripples exactly as we observe them (or maybe tilt motion cannot produce ripples as observed).
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