Differences between revisions 1 and 79 (spanning 78 versions)
Revision 1 as of 2019-01-04 15:26:07
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Editor: MarkBarton
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Revision 79 as of 2019-06-26 14:47:24
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Editor: MarkBarton
Comment:
Deletions are marked like this. Additions are marked like this.
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Archived items are at ../ToDoOld.
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[[#EveryWeek |Every Week]] == Paper ==
 * --(Review Type Bp paper)--
 * --(Choose paper title)-- -> "Vibration isolation systems for the beam splitter and signal recycling mirrors of the KAGRA gravitational wave detector"
 * --(Create JGWDoc number for paper)-- -> [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=9836|P1909836]]
 * --(Decide paper author list)-- -> KAGRA Author List 2019?
 * --(Write Type B paper abstract)--
 * --(Write paper outline)--
 * --(Write Type B paper "Introduction")--
 * Vibration isolation systems in KAGRA
  * --(Write "Overview")--
   * Steal or reproduce Type Bp Figure 1 (optic layout)
   * Steal or reproduce Type Bp paper Figure 2 (suspension comparison)
 * Write Requirements for Type B
 * Write "Design of the Type-B suspension"
  * --(Write "Mechanical")--
   * Choose photo of Type B suspension in mid-air
   * Make diagram of Type B in vacuum chamber
  * Write "Sensors and Actuators"
   * Write "Optical Levers"
  * Write "Control and Damping"
   * Make controls diagram like Type Bp paper Figure 7
 * Write "Measured performance"
  * Write "Damping Time"
   * Make decay time plot like Type Bp paper Figure 8
  * Write "Residual Velocity"
  * Write "Residual Angular Fluctuations"
  * Write "Vibration Isolation Performance"
 * Write "Summary"
 * --(Write "Acknowledgments")-- -> Used 2018-09 version - need to check if there's a newer one.
 * Compile "References"
  * --(Find NS-NS detection reference)--
  * --(Find initial detection reference)--
  * Find Type A reference
  * Find cryogenic payload reference
  * Find bKAGRA reference
  * Find LIGO-India reference
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[[#ComingWeeks |Coming Weeks]] == Tunnel ==
 * Tidy up.
 * Move charging station to more convenient location (e.g., near -X entrance).
 * Find and inventory all gluing tools.
 * Put pointy-tipped screw in RM trolley for BS
 * Put First Contact on SRM-W optic and install it in its holder with 1.4 mm shims ready for possible use.
 * --(Check all pico drivers are on extension cords that can be unplugged from outside the cleanbooth (in case reset is needed).)--
=== BS ===
 * '''Get parts for F0 yaw adjuster - ASAP.'''
 * Add Tanaka-san's LVDT signal card.
=== SR2 ===
 * Add Tanaka-san's LVDT signal card.
=== SR3 ===
 * Add Tanaka-san's LVDT signal card.
=== SRM ===
 * Add Tanaka-san's LVDT signal card.
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<<Anchor(EveryWeek)>> == Shakedown/Characterization ==
=== BS ===
 * Measure decay time, rms with and without control.
 * Do geophone blending.
=== SR2 ===
 * --(Measure decay time, rms with and without control.)--
 * Do FEA model of IRM side plates.
 * --(Do geophone blending.)--
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== Every Week ==
=== Facilities ===
 * Vacuum and roll floor.
 * Wipe ladders.
 * Tidy tools, parts.
 * Get stuff from [[../WishList]]
=== SR3 ===
 * Measure decay time, rms with and without control.
 * Put SR3 cleanbooth electronics in minirack.
 * Check pico adapter cables.
 * Do geophone blending.
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== December 2018 vent ==
 * Look for cracks in F0 blades.
 * Install new yaw F0 stepper mechanism (if available).
 * Install new double-sided F0 fishing rod (have all parts except blades).
 * Add more mass to IP to get a lower frequency.
 * Service geophones (one has high noise, one has DC offset).
 * Re-calibrate F0 GAS LVDT.
 * Confirm the positions of the IP LVDTs and Actuators.
 * Tune LBB (adjust table height, damper height) - DON'T BOTHER (unless there's an excuse to open the lower half of the tank).
=== SRM ===
 * Check where SRM pico cables came from and make sure there isn't one missing somewhere else.
 * Debug 240 Hz noise in LVDT.
 * Measure decay time, rms with and without control.
 * Check keystone lock screws in BF (on next vent).
 * Do geophone blending.
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<<Anchor(ComingWeeks)>> == SDF ==
  * Document SDF in Operations Manual
  * Make SDF states for Type B, e.g.:
   * SAFE
   * DCCTRL-ONLY
   * ALIGNED-IN-AIR
   * ALIGNED-IN-VACUUM
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=== 2018-12-17 ===
==== SRM ====
 * Install/test new yaw mechanism.
 * Adjust height.
 * Check/adjust optic pitch; release LED to SR2.
 * Install Enomoto-kun's beam target plate (if available).
 * Install extension cord for pico drivers.
 * Find two geophone cables used by Okutomi-san. (I looked in the second floor EXV room but didn't find them - Mark.)
 * Find one geophone cable ordered for SRM but missing.
 * Rearrange miswired geophone cable.
 * Rebuild defective geophone cable.
 * Seal geophones.
 * Install geophones and arc weights.
 * Center IP.
==== SR3 ====
 * Install/test new yaw mechanism.
 * Adjust height.
 * Realign OL.
== MEDM ==
 * Fix DAC screen (split model issue).
 * Move overview.txt files from common to k1, edit screens
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==== SR2 ====
 * Install/test new yaw adjuster.
 * Adjust height.
 * Get top plate reduced?
 * Set up OL cabling.
 * Set up OL.
 * Remove tape, writing etc on PI and PI items.
 * Add new feedthrough to lower part of tank (with Izumi-san-tachi)?
 * Install cable for MIF pico on LBB (with Izumi-san-tachi)?
 * Add ballast mass to LBB.
== Guardian/RTM ==
 * Rethink Guardian to avoid going back to SAFE for minor problems.
 * Consider splitting Type B Guardian into tower and payload sections with possible third monitor Guardian overseeing both.
 * Make cycle times of BS models the same as for SRx.
 * Change the DAQ channel lists per [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=10294|Shoda-san's final design]].
 * Remove TM_OSEM subsystem from payload model.
 * Remove GEOWHITEN from IP of top model.
 * Remove ISIINF->CART2EUL->ISIWIT from IM.
 * Add temperature alarms.
 * Add alarms for LVDT actuation near limit (especially for GAS).
 * Add alarm for integral runaway in DCCTRL loops.
 * Change value of nominal in Guardian to 'ALIGNED' or the like.
 * Add secondary watchdog with lower threshold that puts all outputs to HOLD and then gets Guardian to ramp them down.
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<<Anchor(SRPrepTasks)>> == Simulation ==
 * Create controls design description (cf [[https://dcc.ligo.org/LIGO-T1100378/public|LIGO-T1100378]]).
 * --(Get a good set of TFs and put them in a common directory:)--
  * --(Directory: /kagra/Dropbox/Subsystems/VIS/TypeBData/SR2/simulation/TF/ )--
  * --(Content: diaggui xml files and regular text files.)--
 * --(Compare the Matlab prediction with the measurements.)--
  * --(In a reasonable way tune the parameters of the simulation in ordet to get a good agreement.)--
  * --(It should include resonant peaks not predicted by the simulation.)--
  * --(Write a klog about this. )--
 * --(Given the fact that Takanori's Matlab simulation provides the TFs in units of [m/N] calculate a calibration factor for each GAS LVDT and IP and IM virtual actuator, which are in units of [µm/cnt]. )--
 * Collect the measurements of LVDT and OSEM readout noise and put them in a common directory:
  * Location: /kagra/Dropbox/Subsystems/VIS/TypeBData/SR2/simulation/sensor_readout_noise/
  * Content: duaggui xml files and regular text files.
 * Check Panwei's measurements of OSEM noise. Pay special attention to the conversion into m/rtHz from V/rtHz.
 * Calculate the readut noise of the virtual sensors from the readout noise of the real ones.
  * --(IP LVDT.)--
  * --(IP Geo: where's the data for SR2 geophones?)-- There's information in entry [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=6106|6106]]. For SRM the plots are at [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=8177|8177]] but where's the data?
  * --(GAS LVDT (no virtual sensors) )--
  * --(IM OSEMS )--
  * Oplev
 * Estimate coil driver noise. It seems this is not expected to contribute significantly but we should still know.
 * Convert real actuation noise to virtual actuation noise.
 * --(Check whether the Matlab simulation implements the output of the length sensing oplev)--.
 * Extract the filters designed by Enzo, Terrence and Lucia from the filter bank using Foton and write them in a format compatible with Takanori's simulation: --(IP LVDT)--, IP GEO, --(blending filters)--, --(GAS)--, --(IM)--, optic.
 * Check the whether the oplev takes into account the ground motion movement in
  * --(longitudinal displacement: NO)--
  * Pitch and yaw
 * In the simulation, what are the assumed coupling between
  * LVDT-L ==> OpLev-PTM.
  * IP GEO-L ==> OpLev-PTM.
  * Longitudinal ground motion ==> OpLev-PTM.
  * OSEM-L ==> OpLev-PTM
  * And the above quantities with Oplev-YTM.
 * Does the simulation take into account the 1/300 rads of the tunnel slope?
 * In the software modify the control feedback loop topology in order to have the same as in the real system.
 * Tune the filters in order to account for the differences between simulation and measurement.
 * As sanity check for the simulation, check the stability criteria and compare with Enzo's.
 * Ask whether there is a recent measurement of seismic motion at the the central room.
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== SR Prep Tasks - To Be Scheduled ==
=== Tunnel ===
 * Get at least one BIO Converter chassis fully connected (CONTEC BIO card, WD and stepper motor chassis) for implementation and test of stepper motor reset function.
 * Check SR2, SR3 TM coil gains for magnet polarity compensation.
 * Replace chipped magnets (12x12x12 mm) in SR3 IP, H1 and H2.

=== Mitaka or remotely ===
 * Write generic Type B Guardian; make BS and SR3 inherit from it; make analog WD optional for now (all suspensions will get them eventually).
 * (Continue to) soak the sapphire prisms off the dummy BS for reuse on the SRM metal mass.
 * Install damping filters for SR2.
 * Review DAC channel requests.
 * Split SRx real-time models?

== ASAP ==
 * --(Get picomotor drivers back on line.)--
 * --(Debug BS BIO connections, especially PI IP.)--

=== Main Assembly Sequence ===
 * Necessary for phase-I★★★
  * --(Modify IP LVDT damping filters to include set point.)--
  * --(TFs.)--
  * '''''EXCHANGE YAW/VERT FRs at F0'''''

 * Necessary for phase-II★★
  * Debug BS geophones.
  * Flip circuit boards in BS geophones to make them the same as SRx.
  * Calibrate IP LVDT actuation against IP LVDT sensing. (Klog 3553? http://klog.icrr.u-tokyo.ac.jp/osl/?r=3553)
  * Design PI Sensor blending filter.
  * Tune the LVDT sensitivity
  * Measure IP period; adjust ballast mass.

 * At some point (remotely)★
  * Improve OL offloading.
  * Improve GAS offloading.
  * Spectral analysis of Oplev.
  * Design, install angular lock servo using OL. (Almost done for phase-I)
  * Adjust gains and debug damping for IM OSEMs and GAS LVDTs. (Almost done for phase-I)
  * Subtract DC level of Geophones.
  * Spectra analysis of PI sensors (PI LVDTs and Geophones).
  * Calibrate IP LVDT sensing against IP LVDT actuation, IP FRs.
  * Set all EQ stops to TBD clearance.
  * Modify the model for IP coil driver control

=== Documentation and Operation Manual ===
 * Add useful info from Enzo's notebook to BSData.

<<Anchor(RealBSHang)>>
== Tasks Not To Forget ==
=== Major Tasks ===
 * --(Move safety bars from BS AF area to SR2 area.)--
 * Update circuit diagram.
 * (Time permitting) Try adding mass to IP.
 * Update BS Install Procedure with screenshots from new on-assembly-frame 3D CAD.
 * Finish assembly drawing for LBB and LBB damper ring and post on JGWDoc (Hirata-san).
 * Figure out how to make PI yaw adjustment reliable.

=== Minor Tasks ===
==== Mechanical ====
 * Put pointy-tipped screw in RM trolley for BS
 * --(Return/replace temporary ballast mass (dog clamps).)--
 * Characterize replacement F0.
 * --(Wipe/clean arc weights that were rained on.)--

<<Anchor(elec)>>
==== Electrical ====
== Electronics ==
 * Pick better resistor values for sat amps (to give closer to 32K open-light values).
 * Install Tanaka-san's LVDT sig gen cards when available). Update [[KAGRA/Subgroups/VIS/TypeB/Status|Status]] and electronic item lists.
 * Install Tanaka-san's hardware watchdogs. Update [[KAGRA/Subgroups/VIS/TypeB/Status|Status]] and electronic item lists.
 * Enable stepper remote enable system (flip enable switches on stepper drivers) and do final test.
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  * --(Make generic to Type B.)--
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  * Organize stepper reset system and watchdog BIO.
  * Include information on assignment of channels to feedthrough positions.
  * Reflect gender-changers and non-flipping feedthrough adapters.
  * Reflect actual cable lengths.
  * Include LVDT pin size (1 mm).
  * Include Stepper pin size (1.6 mm).
  * --(Add stepper remote enable system.)--
  * --(Add note about gender-changers and non-flipping feedthrough adapters.)--
  * --(Correct default stepper channel assignments and link to wiki for changes.)--
  * --(Remove note about steppers with limit switches (we didn't use them).)--
  * --(Include LVDT pin size (1 mm).)--
  * --(Include Stepper pin size (1.6 mm).)--
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  * --(Include blank page for watchdog.)--
  * Include ''actual'' watchdog.
  * Include information on assignment of channels to feedthrough positions (or summarize on wiki and add link).
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==== Real-time and SUMCON models ====
 * Create SUMCON models for full BS and major installation milestones.
 * Create controls design description (cf [[https://dcc.ligo.org/LIGO-T1100378/public|LIGO-T1100378]]).
 * Make table of ADC/DAC assignments and check for consistency with D1503600 and k1visbs (Enzo, Mark)
 * Understand/document/debug Kokeyama-san's DIO stuff.
 * Measure LPCD and HPCD output filter response.
 * Design and install software compensation filters for LPCD and HPCD output filters.
== Documentation and Operation Manual ==
 * Get scan of Enzo's notebook and post to JGWDoc.
 * Get scan of Terrence's notebook and post to JGWDoc.
 * Add useful info from notebooks to BSData/etc.'
 * Improve Thermometers page of Operations Manual.
 * Improve SDF page of Operations Manual.
 * Improve vistools.py page of Operations Manual (Mark).
 * Add Cameras page to Operations Manual.
 * Add ndscope page to Operations Manual.

== OLs ==
 * Design/procure/install permanent hard protective covers.
 * Consider getting camera covers as well (to stop light getting in and IR getting out).
 * Tweak whitening filter gains.

== One Day (Next Vent, or O4) ==
=== BS ===
 * Tune BS LBB (adjust table height, damper height) - do as part of Mid-Sized Baffle installation.
 * Tune IP to slightly lower frequency (better than current 0.08 Hz, but not as risky as original 0.04 Hz). Experiment with different amounts of mass over each IP leg to reduce L/T/Y cross coupling. Do at same time as Mid-Sized Baffle installation.
 * Replace BS F0 yaw adjuster - Do at same time as Mid-Sized Baffle installation, if parts are available.
 * Replace BS F0 thrust bearing - BIG JOB - NOT WORTH IT.
 * Consider flipping sign of H2 coil actuator (there is a -1 in COILOUTF for it).

=== SR3 ===
 * Replace chipped magnets (12x12x12 mm) in SR3 IP, H1 and H2.

=== SRM ===
 * Install Enomoto-kun's beam target plate (if/when available).

VIS Type B To-Do List

Archived items are at ../ToDoOld.

Paper

  • Review Type Bp paper

  • Choose paper title -> "Vibration isolation systems for the beam splitter and signal recycling mirrors of the KAGRA gravitational wave detector"

  • Create JGWDoc number for paper -> P1909836

  • Decide paper author list -> KAGRA Author List 2019?

  • Write Type B paper abstract

  • Write paper outline

  • Write Type B paper "Introduction"

  • Vibration isolation systems in KAGRA
    • Write "Overview"

      • Steal or reproduce Type Bp Figure 1 (optic layout)
      • Steal or reproduce Type Bp paper Figure 2 (suspension comparison)
  • Write Requirements for Type B
  • Write "Design of the Type-B suspension"
    • Write "Mechanical"

      • Choose photo of Type B suspension in mid-air
      • Make diagram of Type B in vacuum chamber
    • Write "Sensors and Actuators"
      • Write "Optical Levers"
    • Write "Control and Damping"
      • Make controls diagram like Type Bp paper Figure 7
  • Write "Measured performance"
    • Write "Damping Time"
      • Make decay time plot like Type Bp paper Figure 8
    • Write "Residual Velocity"
    • Write "Residual Angular Fluctuations"
    • Write "Vibration Isolation Performance"
  • Write "Summary"
  • Write "Acknowledgments" -> Used 2018-09 version - need to check if there's a newer one.

  • Compile "References"
    • Find NS-NS detection reference

    • Find initial detection reference

    • Find Type A reference
    • Find cryogenic payload reference
    • Find bKAGRA reference
    • Find LIGO-India reference

Tunnel

  • Tidy up.
  • Move charging station to more convenient location (e.g., near -X entrance).
  • Find and inventory all gluing tools.
  • Put pointy-tipped screw in RM trolley for BS
  • Put First Contact on SRM-W optic and install it in its holder with 1.4 mm shims ready for possible use.
  • Check all pico drivers are on extension cords that can be unplugged from outside the cleanbooth (in case reset is needed).

BS

  • Get parts for F0 yaw adjuster - ASAP.

  • Add Tanaka-san's LVDT signal card.

SR2

  • Add Tanaka-san's LVDT signal card.

SR3

  • Add Tanaka-san's LVDT signal card.

SRM

  • Add Tanaka-san's LVDT signal card.

Shakedown/Characterization

BS

  • Measure decay time, rms with and without control.
  • Do geophone blending.

SR2

  • Measure decay time, rms with and without control.

  • Do FEA model of IRM side plates.
  • Do geophone blending.

SR3

  • Measure decay time, rms with and without control.
  • Put SR3 cleanbooth electronics in minirack.
  • Check pico adapter cables.
  • Do geophone blending.

SRM

  • Check where SRM pico cables came from and make sure there isn't one missing somewhere else.
  • Debug 240 Hz noise in LVDT.
  • Measure decay time, rms with and without control.
  • Check keystone lock screws in BF (on next vent).
  • Do geophone blending.

SDF

  • Document SDF in Operations Manual
  • Make SDF states for Type B, e.g.:
    • SAFE
    • DCCTRL-ONLY
    • ALIGNED-IN-AIR
    • ALIGNED-IN-VACUUM

MEDM

  • Fix DAC screen (split model issue).
  • Move overview.txt files from common to k1, edit screens

Guardian/RTM

  • Rethink Guardian to avoid going back to SAFE for minor problems.
  • Consider splitting Type B Guardian into tower and payload sections with possible third monitor Guardian overseeing both.
  • Make cycle times of BS models the same as for SRx.
  • Change the DAQ channel lists per Shoda-san's final design.

  • Remove TM_OSEM subsystem from payload model.
  • Remove GEOWHITEN from IP of top model.
  • Remove ISIINF->CART2EUL->ISIWIT from IM.

  • Add temperature alarms.
  • Add alarms for LVDT actuation near limit (especially for GAS).
  • Add alarm for integral runaway in DCCTRL loops.
  • Change value of nominal in Guardian to 'ALIGNED' or the like.
  • Add secondary watchdog with lower threshold that puts all outputs to HOLD and then gets Guardian to ramp them down.

Simulation

  • Create controls design description (cf LIGO-T1100378).

  • Get a good set of TFs and put them in a common directory:

    • Directory: /kagra/Dropbox/Subsystems/VIS/TypeBData/SR2/simulation/TF/

    • Content: diaggui xml files and regular text files.

  • Compare the Matlab prediction with the measurements.

    • In a reasonable way tune the parameters of the simulation in ordet to get a good agreement.

    • It should include resonant peaks not predicted by the simulation.

    • Write a klog about this.

  • Given the fact that Takanori's Matlab simulation provides the TFs in units of [m/N] calculate a calibration factor for each GAS LVDT and IP and IM virtual actuator, which are in units of [µm/cnt].

  • Collect the measurements of LVDT and OSEM readout noise and put them in a common directory:
    • Location: /kagra/Dropbox/Subsystems/VIS/TypeBData/SR2/simulation/sensor_readout_noise/
    • Content: duaggui xml files and regular text files.
  • Check Panwei's measurements of OSEM noise. Pay special attention to the conversion into m/rtHz from V/rtHz.
  • Calculate the readut noise of the virtual sensors from the readout noise of the real ones.
    • IP LVDT.

    • IP Geo: where's the data for SR2 geophones? There's information in entry 6106. For SRM the plots are at 8177 but where's the data?

    • GAS LVDT (no virtual sensors)

    • IM OSEMS

    • Oplev
  • Estimate coil driver noise. It seems this is not expected to contribute significantly but we should still know.
  • Convert real actuation noise to virtual actuation noise.
  • Check whether the Matlab simulation implements the output of the length sensing oplev.

  • Extract the filters designed by Enzo, Terrence and Lucia from the filter bank using Foton and write them in a format compatible with Takanori's simulation: IP LVDT, IP GEO, blending filters, GAS, IM, optic.

  • Check the whether the oplev takes into account the ground motion movement in
    • longitudinal displacement: NO

    • Pitch and yaw
  • In the simulation, what are the assumed coupling between
    • LVDT-L ==> OpLev-PTM.

    • IP GEO-L ==> OpLev-PTM.

    • Longitudinal ground motion ==> OpLev-PTM.

    • OSEM-L ==> OpLev-PTM

    • And the above quantities with Oplev-YTM.
  • Does the simulation take into account the 1/300 rads of the tunnel slope?
  • In the software modify the control feedback loop topology in order to have the same as in the real system.
  • Tune the filters in order to account for the differences between simulation and measurement.
  • As sanity check for the simulation, check the stability criteria and compare with Enzo's.
  • Ask whether there is a recent measurement of seismic motion at the the central room.

Electronics

  • Pick better resistor values for sat amps (to give closer to 32K open-light values).
  • Install Tanaka-san's LVDT sig gen cards when available). Update Status and electronic item lists.

  • Install Tanaka-san's hardware watchdogs. Update Status and electronic item lists.

  • Enable stepper remote enable system (flip enable switches on stepper drivers) and do final test.
  • Update BS Circuit diagram, D1503600
    • Make generic to Type B.

    • Note removal of LED/PD on TM OSEMs.

    • Add stepper remote enable system.

    • Add note about gender-changers and non-flipping feedthrough adapters.

    • Correct default stepper channel assignments and link to wiki for changes.

    • Remove note about steppers with limit switches (we didn't use them).

    • Include LVDT pin size (1 mm).

    • Include Stepper pin size (1.6 mm).

    • Undo renumbering of IP items.

    • Page 10: "DIO Card # 0" should be "DIO Card # 1"

    • Include OutConfigBoards on OL page (Sheet 18).

    • Update HPCD section to reflect:

      • All three GAS channels are on HPCD #1 and DIO Card #2, CNB cables, Sheet 13.

      • Three IP channels are on HPCD #0 and DIO Card #2, CNA cables, Sheet 15.

    • Include blank page for watchdog.

    • Include actual watchdog.

    • Include information on assignment of channels to feedthrough positions (or summarize on wiki and add link).

Documentation and Operation Manual

  • Get scan of Enzo's notebook and post to JGWDoc.
  • Get scan of Terrence's notebook and post to JGWDoc.
  • Add useful info from notebooks to BSData/etc.'
  • Improve Thermometers page of Operations Manual.
  • Improve SDF page of Operations Manual.
  • Improve vistools.py page of Operations Manual (Mark).
  • Add Cameras page to Operations Manual.
  • Add ndscope page to Operations Manual.

OLs

  • Design/procure/install permanent hard protective covers.
  • Consider getting camera covers as well (to stop light getting in and IR getting out).
  • Tweak whitening filter gains.

One Day (Next Vent, or O4)

BS

  • Tune BS LBB (adjust table height, damper height) - do as part of Mid-Sized Baffle installation.
  • Tune IP to slightly lower frequency (better than current 0.08 Hz, but not as risky as original 0.04 Hz). Experiment with different amounts of mass over each IP leg to reduce L/T/Y cross coupling. Do at same time as Mid-Sized Baffle installation.
  • Replace BS F0 yaw adjuster - Do at same time as Mid-Sized Baffle installation, if parts are available.
  • Replace BS F0 thrust bearing - BIG JOB - NOT WORTH IT.
  • Consider flipping sign of H2 coil actuator (there is a -1 in COILOUTF for it).

SR3

  • Replace chipped magnets (12x12x12 mm) in SR3 IP, H1 and H2.

SRM

  • Install Enomoto-kun's beam target plate (if/when available).

KAGRA/Subgroups/VIS/TypeB/ToDo (last edited 2019-12-18 12:38:30 by fabian.arellano)