ID |
Date |
Author |
Type |
Category |
Subject |
226
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Mon Jan 7 09:01:39 2008 |
steve | Update | SUS | BS sus damping restored |
The BS sus damping was lost at 8am Sunday morning. |
Attachment 1: bssdl.jpg
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232
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Thu Jan 10 10:38:02 2008 |
steve | Update | SUS | etmy damping restored |
The IST building onstruction has really started yesterday and continuing today with big heavy ground breaking
machinary. The MC is holding lock and the suspentions are hanging on.
ETMY does not like this.
SUS-MC2_LLPD_VAR monitor is a good indicator of seismic activity on this 12 days plot |
Attachment 1: etmysus.jpg
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Attachment 2: sustrend16d.jpg
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233
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Thu Jan 10 12:08:23 2008 |
steve | Update | SUS | why did the BS move? |
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Attachment 1: bshopped.jpg
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235
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Thu Jan 10 15:04:04 2008 |
steve | Update | SUS | illuminator light effect on BS position |
The bs chamber illuminator light was turned on this morning and left on.
Earlier on Rana noticed that the bs moved.
I follwed up to see what happened. I turned off oplev servo and tried to recenter on oplev pd
by adjusting pitch and yaw biases. It did not move. I looked at suspention and realized that the
illuminator was still on. I turned it off and to my amazement the the AP spot started flashing
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Attachment 1: bssusilum.jpg
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237
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Mon Jan 14 14:41:09 2008 |
steve | Update | SUS | etmy sus damping restored & mz relocked |
Tree days trend of MZ HV drift is typical these days.
So as the etmy sus inability to hold damping for longer then 2-3 days. |
Attachment 1: etmysus&mzhvtrend.jpg
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254
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Wed Jan 23 09:27:55 2008 |
steve | Update | | etmy sus damping restored |
Seismis event trips etmy |
Attachment 1: etmysus.jpg
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255
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Wed Jan 23 11:41:06 2008 |
steve | Update | PEM | sulfur smell in 40m |
Led - acid car batteries were overcharged in the machine shop next door
and sulfuric acid smell is coming over to the ifo room.
Entry room 103 is specially bad. |
258
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Thu Jan 24 11:52:56 2008 |
steve | Update | PEM | the mud is cleaned up & MOPA shutter is opened |
Safety glasses are required again!
I have just opened the mopa shutter.
One janitor came to help with muddy floor.
Rack 1x1 toward ITMX chamber and the south wall of these area
were completely covered by mud. I wiped the floor of bottom of the rack
with towels. The cables were lifted and still should be wiped.
The bottom of LSC rack got less water, only on the west side.
We are ready to bring up the computers.
Thanks to ALL with the clean up, including Alan Rice
who was really helpful.
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264
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Fri Jan 25 09:22:21 2008 |
steve | Update | PEM | burned toast award goes to |
DYM for collaborating with the enemy.
In order to minimize the number of ants visiting our lab we have to take out side the lab
all food left over and organic waste. If you are eating here do not expect someone else
to clean up after you.
Thanks for your cooperation. |
299
|
Wed Feb 6 09:17:31 2008 |
steve | Update | PEM | IST building construction continoues |
The bulldosers at work |
Attachment 1: seismic8d.jpg
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Attachment 2: seisioo.jpg
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308
|
Mon Feb 11 14:24:19 2008 |
steve | Update | PEM | more earthquakes |
ITMX and ITMY sus damping restored after Baja earthquake 5.1 mag at 10:29 this morning.
The ground preparation for The ITS building is almost finished.
Activity is winding down, however the Baja California_ Mexico earthquake zone
"Guadala Victoria" started acting up on Friday.
http://earthquake.usgs.gov/eqcenter/recenteqsus/Maps/special/California_Nevada_eqs.php |
Attachment 1: eqfeb11.jpg
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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. |
325
|
Wed Feb 20 11:34:17 2008 |
steve | Update | PSL | laser head temp is up |
MOPA head temp is running at 20.3C now
Nomally it is at 18.5C |
Attachment 1: htempup.jpg
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326
|
Wed Feb 20 16:24:37 2008 |
steve | Update | PSL | the laser is recovering slowly |
Head temp is still 20.5C and decreasing slowly.
Power output 2.9W
NPRO power 22 mW is increasing as head is cooling down |
Attachment 1: laserecoverring.jpg
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327
|
Thu Feb 21 09:56:26 2008 |
steve | Update | PSL | the laser is back |
The laser and the psl recovered.
The water chiller temp is 19.98C and head temp 18.4C
Power 3.2W
PMC_T 3.1
c1iovme was restarted and the mc is locking now |
Attachment 1: laserisback.jpg
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335
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Fri Feb 22 14:45:06 2008 |
steve | Update | MOPA | laser power levels |
At the beginning of this 1000 days plot shows the laser that was running at 22C head temp
and it was send to LLO
The laser from LHO PA#102 with NPRO#206 were installed at Nov. 29, 2005 @ 49,943 hrs
Now,almost 20,000 hrs later we have 50% less PSL-126MOPA_AMPMON power |
Attachment 1: lpower1000d.jpg
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351
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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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352
|
Mon Mar 3 13:58:10 2008 |
steve | Update | Computers | RFM Network are down |
The CODAQ_RFNETWORK are down, except C1SUSVME & AWG |
365
|
Fri Mar 7 19:04:39 2008 |
steve | Omnistructure | PSL | laser pointer |
Green laser pointer was found in my desk.
I blamed Rana for not returning it to me after a conference talk.
It is surprisingly bright still.
I will bring sweets for Wednesday meeting. |
385
|
Thu Mar 20 15:28:20 2008 |
steve | Update | VAC | tp2 's drypump replaced |
The fore pump of tp2 was replaced at fore line pressure 998m Torr |
388
|
Fri Mar 21 09:02:03 2008 |
steve | Update | VAC | tp 2 failed |
Small turbo #2 is the forepump of the maglev.
It failed last night, shut down the maglev and interlock closed V1
Ifo pressure is 20 mTorr now. The Yarm was still locked at 8am this morning.
The PSL beam to MC was blocked just before the output periscope.
The psl mechanial shutter did not work from epic screen. |
409
|
Wed Apr 2 15:03:51 2008 |
steve | Update | General | reflectivity of black glass |
The reflectivity of black glass, shade 12 was supplied by Donald O'Shea
of Emerald Glass Inc., Westlake, OH 44145
The reflectivity of this glass was measured as shown
Old 1064 nm Crysta Laser with poor beam quality was the source. |
Attachment 1: bg12refl.pdf
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Attachment 2: bg12refsetup.pdf
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417
|
Mon Apr 7 18:58:49 2008 |
steve | Update | General | reflectivity of SS304 |
The reflectivity of stainless steel 304 super polished # 8 was measured the same way as elog entry 409
The reflectivity: 74 +- 1 % from incident angle 10 to 80 degrees |
Attachment 1: ss304s8refl.pdf
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418
|
Tue Apr 8 09:08:54 2008 |
steve | Configuration | PEM | weather station disconnected |
We can not leave cables in the walkways and go on vacation.
I disconnected the weather station from the DAQ
Every Tuesday is janitor day in the 40m.
We have to give him free space for doing a good job.
Burned toast award goes to Andrey. |
Attachment 1: toast.jpg
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423
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Thu Apr 17 15:00:59 2008 |
steve | Update | VAC | vac controller computer to be replaced |
Now that Rosalba is up and running someone should step forward to volunteer for this job.
Old desk top at the Vacuum Rack should be replaced by a functional less old computer so
the vacuum controller can count on an emergency situation. It's only has to be able to run medm
The existing one is dying. |
443
|
Thu Apr 24 15:57:53 2008 |
steve | Configuration | SAFETY | Safety at AP-ISCT |
I measured the output power of the psl after the mechanical shutter.
It was 1.1 W with Ophir power meter, than unlocked the MC and measured
the power at the MC-REFL Beam Dump at the AP-ISCT 0.9 W
Power on MC-REFL photodiode 92 mW
High power metal beam shields were installed around the beam path of
MC-REFL between AP-Viewport and MC-REFL Beam Dump.
Placed HIGH POWER LASER BEAM PATH warning signs on table frame and top
covers.
Last week I placed a small monitor on the top of the OOC that
monitors the resonant spot of MC2. Please keep an eye on this monitor
when working on the AP-ISCT
AP table should NOT be left uncovered. One experienced laser operator
has to be present if the top is removed and IR-viewer scan required.
We need your full cooperation to keep this lab safe. |
Attachment 1: P1020197.JPG
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Attachment 2: mcrefl3.JPG
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450
|
Fri Apr 25 15:44:21 2008 |
steve | Update | PSL | scattering measurments |
In pursuit of a low back scattering, high power beam dump we looked at materials such:
polished copper, polished aluminum, diamond cut aluminum, variety of polished & heat treated stainless steel and shades of black glasses.
Black glass is ideal at low power. Superpolished SS 304 #8 is the only material that measures close to bg
We are still looking for a conductive low back scattering material that would be ideal for a good high power beam trap.
Black glass-shade 12, ss304 superpolished #8 and white paper-B98-24lbs back scattering were compared at 1064 nm
Atm 1: data plot numbers from front panel of SR830 display,
sensitivity: 1x1 mV for bg and ss
1x1 V for wp
Atm 2: drawing of measurement set up
Atm 3: SR830 lock.amp settings
Atm 4: view from steering mirror
Atm 5: view from black glass trap
Atm 6: white paper |
Attachment 1: scatmeas20080425.xls
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Attachment 2: scattring_set_up_20080425.ppt
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Attachment 3: sr830settings.pdf
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Attachment 4: viewfmirror.pdf
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Attachment 5: viewfbgtrap.pdf
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Attachment 6: wpnmount.pdf
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462
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Thu May 1 08:31:51 2008 |
steve | Update | SUS | earthquake trips etmy & mc1 |
Earthquake at Lake Isabel magnitude 4.4 at 1am today shakes the 40m
ETMY and MC1 watchdogs tripped.
Sus damping restored. |
465
|
Mon May 5 15:53:14 2008 |
steve | Update | VAC | drypump replaced & readbacks are out |
The small turbo pump of the annulus system is tp3
It's drypump was replaced at 1.4 Torr after 8 months of operation.
The rebuilding cost of this SH100 drypump is getting ridiculously high $1349.
I'll look for a replacement.
Joseph rebooted c1vac2 card on Apr 24 entry#441
This restarted the readbacks of the turbos and ion pumps for a while.
That was nice. The readbacks are not working again
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472
|
Fri May 9 08:40:24 2008 |
steve | Update | SUS | ETMY sus damping restored |
ETMY lost damping at 19:10 last night.
There was no seismic event than.
Sus damping was restored this morning. |
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. |
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). |
478
|
Thu May 15 10:40:21 2008 |
steve | HowTo | General | Lisa Goggin, PhD |
Lisa Goggin successfully defended her thesis on May, 13 2008
"A Search For Gravitational Waves from Perturbed Black Hole Ringdowns in Ligo Data"
She started out as a surf student in the 40m.
Congratulation! |
Attachment 1: lisa.JPG
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487
|
Mon May 19 11:49:57 2008 |
steve | Update | SUS | etmy oplev laser replaced |
The 9 years old Uniphase HeNe was replaced by a new JDSU 1103P
Power output ~3.5 mW, reflected light back on qpd ~140 microW, 12,800 counts
Andrey will get the ~2.5 mm od spot on the qpd smaller by replacing
the f1000 lens |
488
|
Tue May 20 09:28:42 2008 |
steve | Bureaucracy | SAFETY | safety traning for 40m |
Tara Chalernsongsak, new gradstudent for K. Libbrecht was introduced to the basics of the 40m operations. |
491
|
Thu May 22 11:21:45 2008 |
steve | Bureaucracy | SAFETY | early surf sudent |
Caltech under grad Eric Mintun received the 40m safety training.
Now he has to read and sign SOP of laser and ifo.
He'll be working with GigE cameras with Joe |
502
|
Wed May 28 14:19:47 2008 |
steve | Update | PSL | kaleidoscope of psl |
atm 1: scattering psl table optics from the top of the output periscope f4, 60s @MOPA 3 W
atm 2: scattering psl table optics from the top of the output periscope f4, 20s
atm 3: competing GigE cameras on the north end of psl table
atm 4: yellow "soft" washer to be replaced on psl output periscope
atm 5: ETMY-ISCT in disarray |
Attachment 1: pslscat.png
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Attachment 2: pslscat2.png
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Attachment 3: 2GigEs.png
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Attachment 4: perwash.png
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Attachment 5: etmydisarray.png
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504
|
Thu May 29 16:32:09 2008 |
steve | Update | SUS | etmy oplev is back |
I relayed the optics for ETMY-oplev as shown in pictures below.
The reflected beam goes directly to the qpd |
Attachment 1: P1020417.png
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Attachment 2: P1020420.png
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505
|
Thu May 29 16:49:49 2008 |
steve | Bureaucracy | Photos | Yoichi has arrived |
Yoichi had his first 40m meeting. We welcomed him and Tobin, who is visiting, by sugar napoleons that
Bob made. |
Attachment 1: yoichi.png
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Attachment 2: bobsn.png
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516
|
Wed Jun 4 10:18:52 2008 |
steve | Update | PSL | wedged SS beam trap |
I moved the SS trap over to the psl table.
Texas super # 8 was used from the large shipment.
TXs#8 scattering measured as before, meaning the polishing is good.
Go's squeezing power pick up 350 mW was used.
I made two ~30 degrees wedge traps using 6" x 4" and 12" x 4" SS 0.039" thick
with copper backing of similar size.
There was too much scattering and I could not minimize them all.
It is very helpful to have so much space on the psl table.
It shows more of the weakness of this kind of trap.
I did not dare to turn up the power. |
Attachment 1: trap1.png
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Attachment 2: trap2.png
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523
|
Fri Jun 6 15:56:00 2008 |
steve | Bureaucracy | SAFETY | Yoichi received safety training |
Yoichi Aso received 40m specific safety training. |
524
|
Fri Jun 6 16:10:51 2008 |
steve | Update | PSL | HEPA filters are running at 100% |
The psl HEPA filters were turned up to run at 100% to accommodate beam trap work on Tuesday, June 3, 2008 |
528
|
Tue Jun 10 08:37:18 2008 |
steve | Update | PSL | beam trap is being tested |
High power beam trap is being tested just west of FSS area on psl enclosure.
When the pmc is operating at low power that means that the rest of the 3W is going into the
circular SS trap.
Please beware of the high power beam trap test |
Attachment 1: trapss3w.png
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529
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Wed Jun 11 11:45:25 2008 |
steve | Update | PSL | ss trap works |
The trap works well at 3 W level. No back reflected beam coming out of the trap on low power
sensing card level. The back scattering was not measured. The trap is insensitive to small pointing variations.
The SS surface did not show any visible degradation after 16 hrs of 3w exposure at elliptical beam size 4x8 mm
It is ready to be placed into the 35 W beam. |
Attachment 1: P1020534.png
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Attachment 2: P1020533.png
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550
|
Fri Jun 20 17:42:48 2008 |
steve | Update | PSL | SS trap scattering compared to black glass trap |
Circular SS304 trap was compared to wedged black glass trap.
The measurement set up of entry 529 was changed to define polarization.
CrystaLaser was remounted in horizontal position and half wave plate was placed after it.
These measurements were done in horizontal polarization.
atm1: the cSSt and wBGt was moved horizontally, ~90 degrees of the incident beam
atm2: traps were rotated around the incident beam, ~20 degrees each direction
atm3: set up
atm4: top view of traps
atm5: side view of trap |
Attachment 1: cSSt_1.png
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Attachment 2: cSSt_2.png
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Attachment 3: scatset_61908.png
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Attachment 4: cSSt&wBGt.png
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Attachment 5: cSStbeam.png
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581
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Fri Jun 27 09:20:15 2008 |
steve | Frogs | PEM | dust particle count is up & alarm handler is on |
This 3 years plot show the trend of seasons.
When outside air quality goes bad ( 0.5 micron > 1 million ) the lab follows.
I will demonstrate this effect with a 4th of July fire works calibration.
Let's do not forget the construction activity next door either.
The alarm handler is busy:
It's sound level were reset to a modest level yesterday.
It would be nice to change the alarm sound so it can play Wagner:Der Ring des Nibelungen:
Das Rheingold, Die Walkure & Siegfried and Gotterdammerung
or something more appropriate than the present frog call
1, half micron count is climbing ( it's close to 16k now )
2, MZ refl signal is too high
3, MC lenght servo LO is too |
Attachment 1: dust3y.jpg
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600
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Mon Jun 30 08:59:23 2008 |
steve | Update | IOO | IOO-MC_DEMOD_LO is low |
The alarm handler is beeping relentlessly: asking for help in high partical count and low demod signal |
Attachment 1: demlo.jpg_____
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608
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Tue Jul 1 09:26:33 2008 |
steve | Update | Computers | RFM network is down |
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609
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Tue Jul 1 10:15:22 2008 |
steve | Update | PSL | eventfull two days |
The laser recovered from a short temp rise. The MZ was aligned and realigned. The suspentions were kicked up accidentally.
Now the computers are down. |
Attachment 1: 2d.jpg
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624
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Wed Jul 2 15:14:42 2008 |
steve | Update | General | added beam traps |
I placed baked razor beam trap after INJ_SM1 and flipper in the injection path on the AP table
Quote: | I have constructed the beam injection optics for the abs length measurement.
The injection beam was coarsely aligned to the interferometer. The reflected beam from SRM was already seen at AS CCD.
I have attached the optical configration for this measurement and the optics layout at the AP table.
I am going to go to LHO for three weeks. During the absence Alberto tunes the mode matching and the alignment of the interferometer.
In the process of making this report, I noticed that one of the iris apertures is about disturbing the beam for OMCR CCD. I will check this before I go to Hanford. Also an RF spectrum analyzer is at the AP table. I try to return this near the PSL on Monday morning.
Attachment 1: Optical configuration for the abs length measurement.
1) One of the arms is locked to the PSL beam by the main control system (red).
2) A laser beam is injected from the AS port (blue). This laser essentially has different frequency from that of PSL.
3) The injected beam and the outgoing PSL beam appear at the output of the faraday in the injection system.
4) They beat each other at the frequency difference of those two lasers.
5) A PLL is used to lock the frequency difference to a local oscillator (LO).
6) The LO frequency is swept at around 3.87MHz, that is the approximate FSR frequency of the arm cavity.
7) If the LO frequency hits the FSR within the resonant width, the beating also appears at the transmitted light as the injected beam also becomes resonant to the arm cavity.
8) Amplitude of the beating at the transmitted light is measured by a RF spectrum analyzer as a function of the LO frequency. We get the FSR frequency (= the arm cavity length) from the top of the resonance.
Attachment 2: Optics at the AP table for the laser injection
700mW NPRO, laser source. vertically polarized.
Periscope, to raise the beam 1 inch to make the beam at the 4 inch elevation.
INJ_SM1/INJ_SM2, steering mirrors to align the injection beam to the IFO beam.
HWP1, half wave plate to make the beam to the farady horiz-polarized. nominal 42deg on the readout.
FI, Faraday isolator for protection of the NPRO from the returning light, for obtaining the returning light.
HWP2, to make the beam from the Faraday horiz-polarized. nominal 357deg on the readout.
MM_Lens, f=125mm to match the laser mode to the IFO beam.
SM1/SM2, steering mirrors to align the IFO beam to the Farady Isolator.
IRIS1/IRIS2, for the coarse alignment of the injection beam.
FLIP, flipper mount to turn on/off the injection optics.
Alignment procedure of the injection system
0) Ignite NPRO several hours before the experiment so that the laser frequency can be stable.
1) Turn up FLIP. Close the shutter of NPRO.
2) Adjust SM1/SM2 so that the ifo beam can appear at the output of FI.
3) Adjust height and position of IRIS1/IRIS2 with regard to the ifo beam so that the ifo beam goes through IRIS1/IRIS2 even when they are closed.
4) Turn down FLIP. Open the shutter of NPRO.
5) Adjust INJ_SM1/INJ_SM2 so that the injection beam can go through IRIS1/IRIS2 even when they are closed.
6) At this time, it is expected that the reflection of the injection beam from SRM appears at AS CCD, if SRM is aligned.
7) Adjust INJ_SM1/INJ_SM2 so that the injection beam at AS CCD can overlap to the IFO beam.
8) Confirm the beam at the output of the FI also overlaps.
---- We are here ----
9) Change the ifo configuration to the X or Y arm only.
10) Scan the crystal temperature of the 700mW NPRO in order to try to have the beating of the two beams at the PD. AS OSA may be useful to obtain the beating.
11) Once the beating is obtained, adjust INJ_SM1/INJ_SM2 such that the beating amplitude is maximized. |
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