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[[#EveryWeek|Every Week]] [[#ComingWeeks|Coming Weeks]] <<Anchor(EveryWeek)>> == Every Week == === Facilities === * Vacuum and roll floor. * Wipe ladders. * Tidy tools, parts. * Get stuff from ../WishList <<Anchor(ComingWeeks)>> === 2019-02-04 === ==== Etc ==== * --(Get additional two camera viewports.)-- * --(Get rid of SRM cable reel.)-- * --(Run cables for cameras (with Kokeyama-san).)-- * --(Install BIO config boards on OL whitening filters for SR2, SR3, SRM)-- * Get rid of SR2 cable reel (shutdown FE and rack, replug everything into new power strip, start up rack and FE). * Wipe inside tanks with Vectra-Alpha wipes and IPA. ==== BS ==== * --(Install BNC cables for stepper remote enable.)-- * Debug stepper remote enable. * Debug BS camera. ==== SR2 ==== * --(Release LBB; add approximate final ballast.)-- * --(Install IM control loops.)-- * --(Decide buoyancy correction and pre-apply as much as possible, leaving optic at nominal height.)-- * --(Install BNC cables for stepper remote enable.)-- * --(Install camera viewport.)-- * --(Install camera.)-- * Install GAS filter control loops. * Debug stepper remote enable. * Split model. ==== SR3 ==== * --(Release the optical table again.)-- * --(Adjust LBB damper and rods to give correct height and gap at mid-range on the blades.)-- * --(Add approximate final ballast.)-- * --(Install camera viewport.)-- * --(Install camera.)-- * Debug stepper remote enable. * Split model. ==== SRM ==== * --(Decide buoyancy correction and pre-apply as much as possible, leaving optic at nominal height.)-- * --(Install camera (with Kokeyama-san).)-- * --(Set up TILT OL.)-- * --(Adjust LBB damper and rods to give correct height and gap at mid-range on the blades.)-- * --(Add approximate final ballast.)-- * --(Split model.)-- * Set up LEN OL. * Debug stepper remote enable. * Check BIO connections for possible swap of GAS/IP. == Tasks To Be Scheduled == ==== BS ==== * Tune BS LBB (adjust table height, damper height) - DON'T BOTHER (unless there's an excuse to open the lower half of the tank). * Replace BS F0 thrust bearing and yaw adjuster - BIG JOB, DON'T BOTHER (unless lack of yaw adjustment becomes a major problem). ==== SR2 ==== ==== SR3 ==== ==== SRM ==== * Install Enomoto-kun's beam target plate (if/when available). * 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. * Put FC on SRM-W and install it in its holder with 1.4 mm shims ready for possible use. === Tunnel === * Replace chipped magnets (12x12x12 mm) in SR3 IP, H1 and H2. === Mitaka or remotely === * (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? === Real-Time Model === * Restart k1vissrmt (Wednesday during maintenance??): * Stop SRM Guardian (just stop it dead - don't transition to SAFE; don't let it meddle at all). * Make fresh safe.snap. * Note all TEST and OPTIC ALIGN offsets. * Put large ramp times (≈30++ s) in all DAMP, TEST and OPTICALIGN filters. * Turn off all DAMP, TEST, and OPTICALIGN filter offsets and master switch. * Restart k1vissrmt. If there are gross problems, consider restarting the whole FE. * Restore safe.snap. * Debug OVERVIEW and IP screens (check for white channels etc). * Restore OPTICALIGN offsets (if necessary), transfer TEST offsets to new ALIGN filters and set long ramp times. * Set new WD thresholds for IP LVDT and ACC. * Enable all DAMP, ALIGN, and OPTICALIGN offsets. * Make sure SRM Guardian is pointing to generic Type B Guardian. * Adjust Type B Guardian code to set long ramp times on all DAMP, ALIGN and OPTICALIGN filters. Wrap the * Reenable Guardian if/when satisfied. * Rebuild and restart k1visbst and initialize/test as for SRM. * Create new k1vissr2t, k1vissr2p, k1vissr3t, k1vissr3p based on k1vissrmt and k1vissrmp. * Update DCUID numbers in /opt/rtcds/userapps/release/vis/common/medm/vissr2_overview_macro.txt and vissr3_overview_macro.txt. * SR2 FECT=54, FECT=55 * SR3 FECT=56, FECT=57 * (SRM FECT=58, FECP=59) * Rebuild, restart k1vissr2t, k1vissr2p, k1vissr3t, k1vissr3p and initialize/test as for SRM/BS. === 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. === Minor Tasks === ==== Mechanical ==== |
=== Noise budget === * Inject bandwidth limited noise into the BS payload degrees of freedom in order to identify peaks in DARM. There's a list of resonance frequencies in the control room. * Measure transfer functions from BS payload to DARM and calculate noise budget. Yamada-kun has already measured some and, as far as I rememeber from the commissionig meeting on Tuesday, Shoda-san has been assigned to measure more after the engineering run. === Real-time model === * Install BS real-time model. Changes are one additional filter output monitor for the bandpass filters (for the OBSERVATION state) and the path for ASC Terrences's method for control. * Compile and install SR's real-time models. Similar modifications as for the BS. * Medm screens have nor been modified for the implemetation of Terrence's method. === Guardian === * Edit Guardian in order to speed up the engaging and disegaging of the control loop in the different stages. In TYPEB.py file comment out some calls to waitForRamp function: * In '''beginControlSequence''', lines 159, 160, 162, 163. * In '''disengageControlSequence''', lines 218, 219, 224, 225. * Apparently when the payload trips Guardian doesn't turn the IM optic align block gain back to 1 after recovery. (Reported by Sheila for the BS in klog [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=12110|12110]]). === Medm screens === * '''The IM-H coil drivers with disabled hardware watchdog produce a false trip signal.''' From the medm screens remove the hardware watchdog indicator for IM-H. This is common for all Type B suspensions. The ideal solution would be to disable the hardware warning signal system instead but there's no time for that now. * '''The BS TM coil driver with disabled hardware watchdog produces a false trip signal.''' This is harder to solve because only BS is affected by this. == 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 == Tunnel == * Tidy up. * Move charging station to more convenient location (e.g., near -X entrance). * Find and inventory all gluing tools. |
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<<Anchor(elec)>> ==== Electrical ==== |
* 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 [[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. == 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. == 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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==== 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. |
* --(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). |
VIS Type B To-Do List
Archived items are at ../ToDoOld.
Noise budget
- Inject bandwidth limited noise into the BS payload degrees of freedom in order to identify peaks in DARM. There's a list of resonance frequencies in the control room.
- Measure transfer functions from BS payload to DARM and calculate noise budget. Yamada-kun has already measured some and, as far as I rememeber from the commissionig meeting on Tuesday, Shoda-san has been assigned to measure more after the engineering run.
Real-time model
- Install BS real-time model. Changes are one additional filter output monitor for the bandpass filters (for the OBSERVATION state) and the path for ASC Terrences's method for control.
- Compile and install SR's real-time models. Similar modifications as for the BS.
- Medm screens have nor been modified for the implemetation of Terrence's method.
Guardian
- Edit Guardian in order to speed up the engaging and disegaging of the control loop in the different stages. In TYPEB.py file comment out some calls to waitForRamp function:
In beginControlSequence, lines 159, 160, 162, 163.
In disengageControlSequence, lines 218, 219, 224, 225.
Apparently when the payload trips Guardian doesn't turn the IM optic align block gain back to 1 after recovery. (Reported by Sheila for the BS in klog 12110).
Medm screens
The IM-H coil drivers with disabled hardware watchdog produce a false trip signal. From the medm screens remove the hardware watchdog indicator for IM-H. This is common for all Type B suspensions. The ideal solution would be to disable the hardware warning signal system instead but there's no time for that now.
The BS TM coil driver with disabled hardware watchdog produces a false trip signal. This is harder to solve because only BS is affected by this.
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 "Damping Time"
- 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.
- 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
- 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).