Differences between revisions 339 and 367 (spanning 28 versions)
Revision 339 as of 2018-10-28 19:16:53
Size: 4354
Editor: MarkBarton
Comment:
Revision 367 as of 2019-01-11 14:17:35
Size: 3962
Editor: MarkBarton
Comment:
Deletions are marked like this. Additions are marked like this.
Line 6: Line 6:
==== Report for week of 10/22 ====
===== SRM =====
 * We borrowed the TM HPCDs from SR2 and SR3 so that SRM had HPCDs for IM-H, IM-V and GAS.
 * Fabian adjusted the last two OSEMs (IM-H2 and H3).
 * We closed the BF and weighed the BF/... section.
 * Fabian and Hirata-san routed all the BF/... cables via the BF cap (except for the four TM OSEM cables, where we're still waiting for extensions).
 * We built up the assembly frame and security structure to the SF level and craned in the SF.
 * We installed the SF-BF rod and flying saucer, and suspended the BF/... section. We will need about 600 g on the BF cap for balance and SF keystone height, which is as expected and not a problem.
 * Hirata-san collected a suitable CuBe spring and bracket parts from Type A. He ultrasonically cleaned the bracket and then installed the bracket and spring on the F0. The frequency increased from 0.5 Hz to 0.625 Hz, so he did another round of compression, from 30 mm to 31.3 mm.
 * Enzo soldered some short and/or broken cables to make longer cables that we need urgently. He got in touch with Yamamoto-san to arrange bringing them to Toyama University and ultrasonically cleaning them.
 * We pulled out cables running to the OMMT area that were used for the old OSEM/geophone testing setup and started a new geophone testing setup in the SR3 area using the optical table from the SR2 assembly frame.
 * Hirose-san reported results from his astigmatism test on the second SRM small optic and metal mass. With the tight shims (1.0 mm thickness, as used for the installed SRM) there was substantial astigmatism, but with the next looser available size (1.5 mm) there was no astigmatism but the optic is held very poorly and rattles. Hirose-san is ordering some intermediate thicknesses and will make a recommendation. However he will almost certainly suggest that we change the shims on the hanging SRM, so we need to think about whether that is feasible.

===== SR2 =====
 * Akutsu-san gathered the parts we will need for the SR2 OL so that Terrence can install it next week.
 * Hirata-san supervised the disassembly of the assembly frame. The pieces are now in the IMMT area, although we may need to move them again because they're a bit in the way.

==== Plan for week of 10/29 ====
 * Mark, Enzo, Hirata-san, Fabian and Terrence at Kamioka Mon-Fri.
===== SR2 =====
 * Set up OL.
 * Possibly do a measurement of how much torque is required on the F0 keystone to move the system in yaw. (This will help Sato-san choose a suitable stepper driver for the new design.)
 * Possibly add more arc weights, to get below 0.1 Hz.
===== SRM =====
 * Electronics
  * More cable soldering?
  * Get soldered cables ultrasonically cleaned.
  * Collect unused cables for return to AEL.
 * PI
  * Finalize tuning.
  * Add more cable clamps.
  * Prepare SF magnet ring.
 * Main sequence
  * Cable/test SF LVDT and FR.
  * Decide and install SF internal ballast mass (probably 1 Promec).
  * Reinstall SF cap.
  * Weigh SF/... section.
  * Install #353 poles
  * Move NB-03 jacks down.
  * Crane PI into AF.
  * Install F0-SF rod (#331) and flying saucer.
  * Route SF/... cables up to underside of F0.
  * Do vertical height budget.
  * Adjust SF trim mass for balance and keystone height.
==== Report for week of 12/17 ====
 * BS
  * We opened the top of the BS tank after the vent.
  * We inspected the BS F0 blades for cracks but still didn't find any.
  * We removed the arc weights and geophones, and added new longer studs for the arc weights and new cables for the geophones. We then put back the original arc weights and new geophones.
  * We measured the geometry of the various IP items to check the IP diagonalization matrices.
  * We installed the new double-sided F0 FR. We were not close to needing to add the optional !CuBe spring. Unfortunately the FR had rather less friction but still didn't work. After checking a bunch of possibilities and comparing against SRM (also non-working) and SR2/SR3 (working), we suspect the carriage may be assembled upside down, with the metal plate below and the PEEK plate above. We will try changing it next week.
 * We adjusted the F0 keystone trim mass and were able to get it to sit at CAD nominal height at nominal temperature (24.9°C) with mid-range FR and modest extra mass (413 g). Interestingly, we noticed that removing the arc weights and/or geophones reduced the load capacity by a few hundred grams.
 * We measured the total range of the IP FRs in steps and set them to mid-range in preparation for tuning the IP frequency and (re-)centering the IP.
 * SRM
  * We borrowed an LED from SR2 and set the pitch of the SRM optic.
  * We found the SRM front end had crashed and could not be properly reset by cycling the power from the web interface. Yamamoto-san eventually got it working for us, although it didn't seem to take more than restarting the user and IOP models.
  * We sealed and retested the new geophones originally intended for SRM, but decided to use them on BS instead.
  * We installed the two OL viewports. We also tried to install the camera viewport but we couldn't get the Cu gasket to sit in the recess, so we gave up and will probably reallocate the camera viewport to SR3 for now (where it will go on a different type of flange which we've had success with. Saito-san says that we can get help with the SRM flange from Mirapro on 1/28.
 * SR3
  * We opened the top of the tank briefly to inspect the configuration of the F0 FR, but didn't do any significant work.
  * Hirose-san inspected inside the bottom part of the chamber and found some dust, so he recommended we wipe with Vectra-Alpha wipes (IPA-resistant type) and IPA. he gave us a powerful LED flashlight array and asked us to use it to look for dust in all the chambers.
 * Etc
  * We gave Simon a list of items we still need for the SRM OL. He seemed to think that they should be in stock at Kamioka and will help us look for them next Tue 1/15.
  * Mark and Enzo booked flights for the KAGRA International Workshop.
  * Mark had to schedule a trip to Australia for the week of 1/21 to attend to family business.
Line 56: Line 32:
==== Plan for week of 10/29 ====
 * Mark, Enzo, Hirata-san and Fabian at Kamioka Mon-Fri (except Hirata-san to take compensation day Friday or Monday (TBD)).
===== SRM =====
 * Main sequence
  * Cable/test IP LVDTs.
  * Cable/test IP FRs.
  * Unlock IP and center roughly.
  * Calibrate IP LVDTs.
  * Check/adjust alignment of SS.
  * Add arc weights and geophones (or extra mass equivalent to geophones).
  * Cable/test geophones.
  * Improve centering/tuning of IP and SS alignment.
 * LBB
  * Move KOACH filters
  * Put LBB damper rings in tank.
  * Set tank jacks to nominal height.
==== Plan for week of 1/7 ====
 * Make sure BS is floating, recenter OL to capture current yaw position.
 * Vent BS.
 * Inspect BS F0 blades for cracks.
 * Install new BS F0 FR, and (if necessary) auxiliary CuBe spring.
 * Confirm geometry of LVDTs, geophones, FRs etc and update T1707205 if necessary.
 * Replace geophone preamps and cables (to fix noise, offset, pinout flip issues).
 * Add more mass to IP to get lower frequency.
 * Adjust all GAS filters to near mid-range (using keystone mass for F0 as much as possible, and FR+LVDT for SF and BF).
Line 73: Line 42:
==== Vacation/Visitor Info ====
 * Terrence: 10/29-11/2 at Kamioka.
==== Vacation/Etc Info ====
 * Mark and Enzo: KAGRA International Workshop in Perugia, 2/14-16.
 *
Terrence: back at Kamioka from 1/7.

Scraps of text for incorporation in the VIS Meeting Minutes

KAGRA/Subgroups/VIS/MeetingNAOJ

Type B (Mark)

Report for week of 12/17

  • BS
    • We opened the top of the BS tank after the vent.
    • We inspected the BS F0 blades for cracks but still didn't find any.
    • We removed the arc weights and geophones, and added new longer studs for the arc weights and new cables for the geophones. We then put back the original arc weights and new geophones.
    • We measured the geometry of the various IP items to check the IP diagonalization matrices.
    • We installed the new double-sided F0 FR. We were not close to needing to add the optional CuBe spring. Unfortunately the FR had rather less friction but still didn't work. After checking a bunch of possibilities and comparing against SRM (also non-working) and SR2/SR3 (working), we suspect the carriage may be assembled upside down, with the metal plate below and the PEEK plate above. We will try changing it next week.

  • We adjusted the F0 keystone trim mass and were able to get it to sit at CAD nominal height at nominal temperature (24.9°C) with mid-range FR and modest extra mass (413 g). Interestingly, we noticed that removing the arc weights and/or geophones reduced the load capacity by a few hundred grams.
  • We measured the total range of the IP FRs in steps and set them to mid-range in preparation for tuning the IP frequency and (re-)centering the IP.
  • SRM
    • We borrowed an LED from SR2 and set the pitch of the SRM optic.
    • We found the SRM front end had crashed and could not be properly reset by cycling the power from the web interface. Yamamoto-san eventually got it working for us, although it didn't seem to take more than restarting the user and IOP models.
    • We sealed and retested the new geophones originally intended for SRM, but decided to use them on BS instead.
    • We installed the two OL viewports. We also tried to install the camera viewport but we couldn't get the Cu gasket to sit in the recess, so we gave up and will probably reallocate the camera viewport to SR3 for now (where it will go on a different type of flange which we've had success with. Saito-san says that we can get help with the SRM flange from Mirapro on 1/28.
  • SR3
    • We opened the top of the tank briefly to inspect the configuration of the F0 FR, but didn't do any significant work.
    • Hirose-san inspected inside the bottom part of the chamber and found some dust, so he recommended we wipe with Vectra-Alpha wipes (IPA-resistant type) and IPA. he gave us a powerful LED flashlight array and asked us to use it to look for dust in all the chambers.
  • Etc
    • We gave Simon a list of items we still need for the SRM OL. He seemed to think that they should be in stock at Kamioka and will help us look for them next Tue 1/15.
    • Mark and Enzo booked flights for the KAGRA International Workshop.
    • Mark had to schedule a trip to Australia for the week of 1/21 to attend to family business.

To-Do Lists, Schedule

Plan for week of 1/7

  • Make sure BS is floating, recenter OL to capture current yaw position.
  • Vent BS.
  • Inspect BS F0 blades for cracks.
  • Install new BS F0 FR, and (if necessary) auxiliary CuBe spring.

  • Confirm geometry of LVDTs, geophones, FRs etc and update T1707205 if necessary.
  • Replace geophone preamps and cables (to fix noise, offset, pinout flip issues).
  • Add more mass to IP to get lower frequency.
  • Adjust all GAS filters to near mid-range (using keystone mass for F0 as much as possible, and FR+LVDT for SF and BF).

Vacation/Etc Info

  • Mark and Enzo: KAGRA International Workshop in Perugia, 2/14-16.
  • Terrence: back at Kamioka from 1/7.

KAGRA/Subgroups/VIS/TypeB/Minutes (last edited 2022-10-28 10:02:46 by fabian.arellano)