MICE Collaboration Meeting RAL 31 May – 3 June 2009 AFC status By Wing Lau, Oxford University.

Slides:



Advertisements
Similar presentations
1 AFSWG Mtg 15 Aug 2003 Elwyn Baynham RAL Safety Overview Work done by RAL Group Contributors Elwyn Baynham Tom Bradshaw Iouri Ivaniouchenkov.
Advertisements

Liquid H 2 Absorber Production Contents (1)MICE Absorber Status (2)MICE Absorber Modification (3)Plan/Schedule (4)Summary MICE CM-23 in HARBIN Shigeru.
MICE RF and Coupling Coil Module Outstanding Issues Steve Virostek Lawrence Berkeley National Laboratory MICE Collaboration Meeting October 26, 2004.
First Wall Heat Loads Mike Ulrickson November 15, 2014.
Status of the AFC at RAL Tom Bradshaw John Cobb Wing Lau Matt Hills Elwyn Baynham Mike Courthold Victoria Bayliss MICE Project Board 28 th June 2011.
4m Undulator Design Concepts Amanda J Brummitt CCLRC RAL On behalf of the HeLiCal Collaboration.
MICE Superconducting Solenoids: Status and Update RAL: T W Bradshaw M Courthold J Rochford M Hills D Baynham Oxford: J Cobb W Lau S Yang MICE.
Integration of Cavities and Coupling Coil Modules Steve Virostek Lawrence Berkeley National Laboratory MICE Collaboration Meeting March 28 – April 1, 2004.
Action Who Progress made status Implement central repository for drawings -- need detector information to add to official drawing WL Progress on-going.
Agreement on scope of supply and extent of interface among different suppliers of the AFC module This talk covers the scope of supply on the Absorber Focus.
Spectrometer Solenoid Update Steve Virostek Lawrence Berkeley National Lab MICE Video Conference 114 September 18, 2008.
Progress on the MICE Cooling Channel Solenoid Magnet System
Spectrometer Solenoid Design and Procurement Review Steve Virostek Mike Green Mike Zisman Lawrence Berkeley National Lab MICE Collaboration Meeting October.
MICE Collaboration meeting at CERN March 28 – April 1, 2004 MICE Cooling Channel --- AFC Module work group report Wing Lau – Oxford.
23 October 2005MICE Meeting at RAL1 MICE Tracker Magnets, 4 K Coolers, and Magnet Coupling during a Quench Michael A. Green Lawrence Berkeley Laboratory.
1 Update on Focus Coil Design and Configuration M. A. Green, G. Barr, W. Lau, R. S. Senanayake, and S. Q. Yang University of Oxford Department of Physics.
Tracker Solenoid Module Design Update Steve VirostekStephanie Yang Mike GreenWing Lau Lawrence Berkeley National LabOxford Physics MICE Collaboration Meeting.
Status of VLPC Cryo-Cooler Cryostat Design Russ Rucinski (Alan Bross) Fermilab.
Spectrometer Solenoid Update Steve Virostek - LBNL MICE Video Conference #129 February 25, 2010.
MICE AFCSWG Safety Review Summary Mary Anne Cummings Dec. 17, 2003 MICE Video Conference.
Background to the current problem 1. As a result of the high stresses in the bobbin due to the magnet load, the bobbin end plate needs to be increased.
Talk outline 1 st talk: –Magnetic forces –Quench in the absorber cryostat 2 nd talk: –Shielding of magnetic fringe fields.
MICE Collaboration Meeting March 29 - April 1, CERN MICE alignment, tolerances and supports Tuesday March 30 Room Edgar Black/IIT March17-
MICE absorber and Window / flow Design Wing Lau, Giles Barr & Stephanie Yang Oxford University MICE Meeting Berkeley, Oct 2002.
1 Infrastructure at RAL Iouri Ivaniouchenkov, RAL MICE Collaboration CERN, 29 March 2003.
bobbin Thermal radiation shield Magnet cryostat Large End Flange The leading dimensions.
Summary of the change request from KEK KEK suggested 4 changes to be made on the AFC. We have looked into the request carefully and discussed the implications.
1 Status of infrastructure MICE Video Conference, August 17, 2005 Yury Ivanyushenkov Applied Science Division, Engineering and Instrumentation Department.
A reminder of the outstanding action list:- Implement central repository for drawings – need detector information to add to official drawing Instrumentation.
MICE Collaboration meeting at CERN March 28 – April 1, 2004 MICE Cooling Channel --- AFC Module progress update Wing Lau – Oxford.
MICE Collaboration Meeting Harbin, China 13 – 17 January 2009 Progress on AFC since the PRR By Wing Lau, Oxford University.
Spectrometer Solenoid Fabrication & Testing Update Steve Virostek Lawrence Berkeley National Lab MICE Collaboration Meeting #26 University of California.
MICE Collaboration Meeting Harbin, China 13 – 17 January 2009 Integration Issues By Wing Lau, Oxford University.
Assembly, Installation and Interfaces Steve Virostek Lawrence Berkeley National Lab RFCC Module Design Review October 21, 2008.
Fcal upgrade for sLHC: Cryogenics modifications – TE-CRG/ C.Fabre 1 ATLAS FCal Upgrade for sLHC: Modifications to the Calorimeter Cryogenic.
Spectrometer Solenoid Update Steve Virostek Lawrence Berkeley National Lab Roy Preece Rutherford Appleton Lab October 28, 2011 MICE Collaboration Meeting.
Status and Integration of the Spectrometer Solenoid Magnets Steve Virostek Lawrence Berkeley National Lab MICE RAL June 15, 2007.
1 UK PM Report Costs & Schedule Alan Grant, STFC.
1 Progress On The Design And Manufacture Of The New Stator Geoff Barber Imperial College.
Hydrogen system R&D. R&D programme – general points Hydrogen absorber system incorporates 2 novel aspects Hydrogen storage using a hydride bed Hydrogen.
MICE Collaboration meeting (CM20) At RAL 10 – 13 Feb 2008 AFC Magnet – Status and Progress W. Lau, Oxford University.
Spectrometer Solenoid: Plans to Fix Magnet 2 Steve Virostek Lawrence Berkeley National Lab Spectrometer Solenoid Review November 18, 2009.
NCSX VACUUM VESSEL PL Goranson Thermal Insulation Final Design Review July 31, 2006 WBS12 NCSX.
Spectrometer Solenoid Fabrication & Testing Update Steve Virostek Lawrence Berkeley National Lab MICE CM25 at RAL November 6, 2009.
Spectrometer Solenoid Fabrication Status and Schedule Steve Virostek Lawrence Berkeley National Lab MICE RAL October 20, 2008.
UK Update Package Managers Meeting 001 Roy Preece 13 th January 2014.
CM27 – 8 th July 2010 LH2 System Progress and Future Plans M Hills T Bradshaw M Courthold I Mullacrane P Warburton.
Spectrometer Solenoid Fabrication Update Steve Virostek Lawrence Berkeley National Lab NFMCC at LBNL January 25, 2009.
Main features of PETS tank J. Calero, D. Carrillo, J.L. Gutiérrez, E. Rodríguez, F. Toral CERN, 17/10/2007 (I will review the present status of the PETS.
22 October 2005MICE Meeting at RAL1 Tracker Solenoid Overview Michael A. Green Lawrence Berkeley Laboratory MICE Collaboration Meeting 22 October 2005.
MICE RF Coupling Coil Magnets Update Derun Li Center for Beam Physics Lawrence Berkeley National Laboratory October 6, 2010 Sofia, Bulgaria.
Cavity support scheme options Thomas Jones 25/06/15 1.
NCSX VACUUM VESSEL PL Goranson Final Design Review November 17, 2005 Man Access Port /Lateral Supports NCSX.
1 Small Coolers for MICE Michael A. Green University of Oxford Department of Physics Oxford OX1 3RH, UK MICE Collaboration Meeting RAL.
Spectrometer Solenoid Design and Test Results Steve Virostek Lawrence Berkeley National Lab Spectrometer Solenoid Review November 18, 2009.
Mike Struik / LHC-CRI INSTRUMENTATION FEEDTHROUGH SYSTEM FOR LHC MACHINE ARC QUADRUPOLE MAGNETS. 123rd LHC Vacuum Design Meeting 19 April 1999.
Status of the MICE Construction Project Resource Loaded Schedule Review 29 th April 2014 Roy Preece.
1 Status of infrastructure MICE Collaboration Meeting, Frascati, June 26-29, 2005 Yury Ivanyushenkov Applied Science Division, Engineering and Instrumentation.
CLOSING REMARKS. Following the Review Charge Cryo-Design  Review and comment on the overall cooling circuit and overall cryo-design. u Temperature Margin.
MICE Spectrometer Solenoid Recovery Review - December 3-4, Steve Virostek MICE Spectrometer Solenoid Design and Assembly.
MICE CC Magnet Cryostat Design Overview Derun Li Center for Beam Physics Lawrence Berkeley National Laboratory MICE CC Cryostat Design Review LBNL, February.
Thermal screen of the cryostat Presented by Evgeny Koshurnikov, GSI, Darmstadt September 8, 2015 Joint Institute for Nuclear Research (Dubna)
Update on PANDA solenoid design and analysis Gabriella Rolando Helder Pais Da Silva Herman ten Kate Alexey Dudarev 3 November
Progress on AFC Procurement T W Bradshaw Rutherford Appleton Laboratory Harwell Science and Innovation Campus Didcot, OX11 0QX, UK
Update on PANDA solenoid design
Ti/SS transitions A.Basti INFN-PISA*
Internal review of IR2 LEP cryostats (WP11/WP5) Close out session
MICE Meeting at RAL, Oct-23, 2005
A. Vande Craen, C. Eymin, M. Moretti, D. Ramos CERN
Spectrometer Solenoid Update
Presentation transcript:

MICE Collaboration Meeting RAL 31 May – 3 June 2009 AFC status By Wing Lau, Oxford University

Everything you want to know about the AFC, but didn’t know how to ask. Let me unfold this to you in the following sequence. Issues, Hiccups & points of interest Progress since last reported Current schedule Contract variance

Quench Issue on the AFC Module There has been some discussion in the context of the AFC module as the best method to control quench. There are basically two approaches were considered: Active system The use of an active system where there are heaters embedded in the coils. Upon detection of a quench electronics provide power to these heaters which dissipate the stored energy. Pros Doesn’t rely on thermal contact between the coils and the former – a slip plane can be used. Cons Expensive More complex as heaters have to be installed in the coils The price tag – over £100K!!! Issues:-

Quench Issue on the AFC Module (cont.) Passive (Quenchback) This relies on there being good thermal contact between the coils and the former. A quench induces currents in the former which heat the inner surface of the coils and dissipates the energy. Pros Simple construction No complicated electronics Passive Cons Need good and reliable thermal contact between the coils and the former For MICE we will need a separate power supply for each module Baseline solution The systems above were reviewed in the context of MICE and as a baseline, the passive system was chosen. Tesla have been charged with coming up with a design that ensures there is adequate thermal contact between the coils and the former

The Hiccups

Hiccups so far:- Space envelope clashes:- This came about when we agreed to Tesla increasing the bobbin end plate thickness from 25mm to 35mm. As a result, the following happened:

bobbin Thermal radiation shield Magnet cryostat Large End Flange The leading dimensions shown on the interface drawing to both KEK and Tesla

bobbin Thermal radiation shield Magnet cryostat Large End Flange Hydrogen Absorber and the feed pipes are already made and tested. The constraint from KEK: Constraint from Tesla:- Tesla needs 10mm for the extra thickness for the bobbin end plate. They also increased the gap at and thicken up the thermal radiation shield sheet metal. This extends their space envelope by as much as 15.4mm. Foul!! Clash between LH2 pipe and magnet cryostat !!! The design as it stands

If nothing done, the following will happen:

bobbin Thermal radiation shield Magnet cryostat Large End Flange The absorber has to be shifted by 15.9 mm upstream 15.9mm 12.5 The Large End Plate will stick out of the AFC cryostat flange face by 15.9mm

The solution:

Agreed change with Tesla:- 1) Reduce space between Magnet cryostat & radiation shield; 2) Local thinning of Large End flange to give H2 pipe a clearance gap of 47.5mm bobbin Thermal radiation shield Magnet cryostat Large End Flange Agreed change with KEK:- The LH2 feed pipe to be extended by 10mm 0.4mm Large End Flange locally thinned down to 2.5mm 39.0 Absorber stays at coil centre Negligible stick out

Details of the local thinning of the large flange end plate at the LH2 pipe area

Arrangement for the local hatch of the Large Flange end plate

Justification for the local thinning on the large end plate – by FEA

Applied pressure:- 1 bar Local peak stress: MPa Max. bending stress:- 62 MPa Pro-rata to the design pressure of 1.5 bar ( Table 1.8 of tech,spec ), the max. bending stress = 93 MPa. Allowable bending stress for Al T6061 at room temp = 1.5 x 78 = 117 MPa. Stress in the thinned down area does not seem to be affected – mainly because of the reinforcement effect from the rest of the plate which is 12.5mm thick. This area has a thickness of only 2.5mm End load effect (from Safety window) is accounted for and is applied onto this area

The issue has been addressed by the Technical Board who has accepted the technical proposal for the change.

Issues of interests

Points worth highlighting here:- Cryocooler:- Power supply - we opted for 280 / 420VAC; 3 phase at 50 Hz. Beam height Now fixed at +1544mm from mounting platform. AFC support to be made with a tolerance of +0,-30mm. This allows the module to be shimmed at site. HTS Leads SS shunts are incorporated. Each is 225mm long and has an area of between 38.2mm2 and 59.6mm2. We still need to establish how long will it take for the power supply to react in the case of a lead quench Coil Cooling Indirect cooling is now incorporated. SS banding wire on the outside any space outside the coil is filled up with epoxy to ensure good thermal contact between coil and bobbin – a requirement for the passive

Progress on PRR

1 Current lead thermal analysis The current design uses a lead with a high RRR (around 50). The use of copper with a lower RRR of 10 or less is safer and will prevent thermal runaway. Tesla will re-model the lead with a lower RRR material Completed 2 Thermal model The coil has been modelled as an isotropic block of copper. Tesla will re-model the copper block assuming different and more realistic conductivities in the three directions (note that this data is already in the quench modelling) Tesla modelled with the thermal boundary conditions as noted above – the maximum temperature of the coil is 4.56 which leaves only 0.25K margin. Issues: Need to ensure that there is good thermal contact between the coil and the bobbin/former, this ensuring reliable quenchback. If MICE power all the coils individually then the requirement for active quench protection is removed. Thermal contact can be ensured by overwinding/increased tension to 170 MPa and filling the outside volume with epoxy, as well as using banding wire. Tesla has agreed. This will be confirmed once the re-run of the thermal model takes place

2 Thermal model The coil has been modelled as an isotropic block of copper. Tesla will re-model the copper block assuming different and more realistic conductivities in the three directions (note that this data is already in the quench modelling) Tesla modelled with the thermal boundary conditions as noted above – the maximum temperature of the coil is 4.56 which leaves only 0.25K margin. Issues: Need to ensure that there is good thermal contact between the coil and the bobbin/former, this ensuring reliable quenchback. If MICE power all the coils individually then the requirement for active quench protection is removed. Thermal contact can be ensured by overwinding/increased tension to 170 MPa and filling the outside volume with epoxy, as well as using banding wire. Tesla has agreed. This will be confirmed once the re-run of the thermal model takes place

3 Thermal model The contact resistance on the cryocooler first stage looks optimistic. How is the load applied and what load can be applied ? - Tesla to confirm that the values used are realistic including the contact area. Reply from Tesla: “.... We have a customer with over 200 turrets in the field using this method, therefore we do not believe it will be an issue” This item was closed but will be revisited in view of the issue raised due to the extended length of the bobbin 4Conductor Tesla to demonstrate satisfactory splice technique. Tesla has proposed superconductor splice overlap of around 350 mm. This would have been done be in April but the superconductor delivery was late. This is not a hold point for the PRR, but we will monitor its progress. 5 Configuration Tesla to evaluate the direct and indirect cooling option and propose the preferred solution. Note that the MICE team will allow an increase in the coil inner radius to reduce the stresses. This could be increased to 268mm. MICE will provide a simple sketch showing the relevant dimensions. Revised dimensions have been agreed. This item is closed. 6 Configuration The aim will be to reach a decision on the bobbin dimensions within two weeks from the meeting (20 th November). Bobbin dimensions agreed. Bobbin forging has been ordered since. This item is closed

7 Mechanical Issues on Indirect Cooled Bobbin Design Loads to be considered  Winding load  Cool-down static loads  Magnetic load  Cool down transient  Quench  Transport  Self weight  Pre-load on suspension straps Tesla will estimate the level of these loads and apply to a set of scenarios including normal operation, quench, cool- down and transport. This was discussed as part of action #2. Tesla will be reviewing the winding tension as part of the investigation into improving the thermal contact. The cool down transient load needs to be estimated and is still outstanding. This item remains open. 8 Quench protection Tesla will consider the issues of redundancy in the active quench protection system Active quench back design was proposed and a price tag of well over £100K was submitted by Tesla. As a result of discussion on #2 and #7, it is now agreed that Tesla will adapt the quench back design. Tesla will model the former assuming there is sufficient contact between coil and bobbin, We have not heard from Tesla opposing the use of Quench back design. A formal clarification is needed to close this item.

9 Worst Case One of the cases considered in the thermal model gave a force of 90t. How was this arrived at and what were the MICE conditions ? Item resolved and is now Closed 10 Vent line The configuration of the vent line was discussed at the meeting. Issues raised were the size of the line and a possible heat load at a critical area. The layout has changed and this has been incorporated in MN’s thermal model. There are no problems with the new design. This item is closed 11 Critical Items List The beam height will be checked, confirmed and documented by RAL RAL replied and this item is now closed 12 Critical Items List The meeting highlighted the importance of the tolerances on the vessel flanges that connect to neighbouring modules and the magnet alignment. Tesla to confirm the adequacy of the approach. This was done and a few items were spotted, e.g. the clocking of the flange bolt holes. All the critical items have now been looked at. The remaining issue is the boundary space envelop which resulted in a commercial variance raised – to extend KEK’s LH2 feed pipes and the local machining of the large end plate to give back KEK its 47.5 mm space. 13 Cryocooler For indirect cooling there are issues associated with the size and configuration of the condensing lines and the sensitivity to impurities at the bottom of the cryostat. Tesla to consider these issues in the design. As a result, a sump has been added and an expansion tank included on the top.

14 HTS Leads Tesla will confirm that there is flexibility in the installation to accommodate thermal contractions Tesla confirmed that a shunt has been incorporated. Shunt is 225mm long and has an area of between 38.2mm 2 and 59.6mm 2. In the case of a lead quench, it is important to know how long will it take for the power supply to react. Tesla to confirm. 15 HTS Leads Tesla will confirm that there is adequate thermal clamping in the region of the G10 block near to the coil Issue resolved and is now closed. 16 HTS Leads and Cryocooler Tesla will check orientation and position of the HTS leads (and the magnetic shielding thickness) and the cryocooler motor with respect to the magnetic field. Action completed 17 Radiation shield At the moment 6063 is being used - it has been suggested that a better grade may be Tesla to consider its use TBD at the right time 18 Support straps Tesla to confirm the actual UTS values achieved with the S-glass straps Action completed

19 Support for current leads The weight of the current leads needs supporting to avoid damage to the feedthroughs. RAL will advise on the routing and where to place supports Still open, awaiting reply from RAL. 20 Instrumentation and services Tesla will provide an inventory of the pipes, services and instrumentation to the AFC module for external routing. MC (RAL) to advise. 21 Hydrogen system Tesla will move interconnects higher up into the turret In new design may be moved even further up where there is more room– This is now done. 22 Hydrogen system RAL will advise on the heat exchanger required on the cryocooler first stage Pipework pre-assembled on to copper bobbin – approximately 2.5m incorporated. Condensing line enters condensing pot through main condensing line. Action complete 23 Hydrogen system Tesla will confirm that the two vacuum systems are able to withstand atmospheric/vacuum combinations Action completed 24 Hydrogen system The instrumentation wires on the hydrogen system are routed through a vacuum port. Tesla to check that the pumping is not compromised by this. Inventory from KEK was passed onto Tesla. Action completed.

25 Fault cases Fault cases need consideration e.g. over- current, wrong polarity both in the AFC and external components. MICE to provide feedback. TB to coordinate 26 Mechanical Some of the weld qualifications need adding (this does depend on final mechanical solution) On Tesla QIPP plans, and has been address through there. Item closed 27 Hydrogen system Check if a dummy outer (safety) window flange is available to check fit. Also, MICE to provide a go-nogo gauge for the warm bore. No dummy is available but OU will provide a go-nogo gauge (wooden). 28 Disassembly Tesla to check that critical items can be removed and replaced in case of failure. Items could be HTS leads, feedthroughs, cryocoolers, etc… Item closed

The schedule

Money issues

Contract variance:- Two contract variance were raised by Tesla so far; On the Bobbin design and indirect cooling etc. This has resulted in a cost variance of £16K and a schedule delay of 2 months. This has been resolved and MICE has accepted the request. On the space envelope Tesla has submitted a cost variance in the region of £11K and a schedule delay of a further 2 months. It is not clear what the £11K include. Clarification is being sought. Approval is needed from the MICE PM board to accept the variance request.