1 Search for Worst-Case Forces MICE Video Conference, September 8, 2004 Yury Ivanyushenkov Applied Science Division, Engineering and Instrumentation Department,

Slides:



Advertisements
Similar presentations
Emittance definition and MICE staging U. Bravar Univ. of Oxford 1 Apr Topics: a) Figure of merit for MICE b) Performance of MICE stages.
Advertisements

MICE Absorber cryostat Forces and power dissipation - for normal operation and during a magnet quench Elwyn Baynham James Rochford MICE Meeting November.
Magnet quench during a training run Magnet electrical circuit schematic PROGRESS ON THE MODELING AND MODIFICATION OF THE MICE SUPERCONDUCTING SPECTROMETER.
Cooling channel issues U. Bravar Univ. of Oxford 31-Mar-2004.
Action Who Progress made status Implement central repository for drawings -- need detector information to add to official drawing WL Progress on-going.
On MICE Coordinate System Yury Ivanyushenkov RAL.
October, 2003 P. Fabbricatore and S. Farinon Spectrometer magnets – Possible layout of cryostat in the end region In order to define the cryostat layout.
Progress on the MICE Cooling Channel Solenoid Magnet System
Changing the absorbers: how does it fit in the MICE experimental programme? Besides the requirement that the amount of multiple scattering material be.
23 October 2005MICE Meeting at RAL1 MICE Tracker Magnets, 4 K Coolers, and Magnet Coupling during a Quench Michael A. Green Lawrence Berkeley Laboratory.
Alain Blondel MICE: Constraints on the solenoids 2.Field Homogeneity: or ? this will be dictated by the detector requirements. TPG will be.
OPTICS UPDATE Ulisse Bravar University of Oxford 3 August 2004.
MICE Collaboration meeting at LBNL: 9 ~13 th Feb, 2005 Force reaction analysis Stephanie Yang Feb 10 th, 2005.
Tracker Solenoid Module Design Update Steve VirostekStephanie Yang Mike GreenWing Lau Lawrence Berkeley National LabOxford Physics MICE Collaboration Meeting.
18 June 2004AFC meeting1 MICE  functions and so on Work in progress…. Observation by Ulisse Bravar at CERN meeting that beam not matched in baseline (Proposal.
1 G4MICE studies of PID transverse acceptance MICE video conference Rikard Sandström.
Downstream transversal sizes Rikard Sandström University of Geneva MICE detector meeting.
10 October 2006 MICE CM-16 at RAL 1 Distributed versus Lumped Coupling Magnets Michael A. Green and Soren Prestemon Lawrence Berkeley Laboratory, Berkeley.
1 RAL Integration Issues MICE Collaboration Meeting, Osaka, August 1-3, 2004 Elwyn Baynham, Paul Drumm, Yury Ivanyushenkov, Tony Jones RAL.
MICE Magnetic forces James Rochford Elwyn Baynham AFC working group meeting RAL 23 April 2004.
PID Detector Size & Acceptance Chris Rogers Analysis PC
9 June 2006MICE CM-15 Fermilab1 Progress on the MICE Cooling Channel and Tracker Magnets since CM-14 Michael A. Green Lawrence Berkeley Laboratory.
1 Quench Protection and the Power Supplies for the MICE Focusing and Coupling Magnets Michael A Green Lawrence Berkley Laboratory 10 February 2005.
1 OPTICS OF STAGE III Ulisse Bravar University of Oxford 6 October 2004.
MICE CM - Fermilab, Chicago - (11/06/2006) 1 A (short) history of MICE – step III M. Apollonio – University of Oxford.
1 On MICE Coordinate System Yury Ivanyushenkov RAL MICE Collaboration CERN, 29 March - 2 April 2004.
1. Optical matching in MICE Ulisse Bravar University of Oxford 2 June 2004 Constraints Software MICE proposal mismatch MICE Note 49 (September 2004, Bob.
Talk outline 1 st talk: –Magnetic forces –Quench in the absorber cryostat 2 nd talk: –Shielding of magnetic fringe fields.
30 June 2004MICE VC1 MICE  functions Since last VC report: –New Mike Green configurations for decreased spacing between focus and matching coils of 400mm,
1 Superconducting Magnets for the MICE Channel Michael A. Green Oxford University Physics Department Oxford OX1-3RH, UK.
MICE analysis meeting Alain Blondel 5 August MICE -- what running strategy? disclaimer: of course we will evolve the running strategy as problems.
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.
MRI Magnets in MICE Initial Scoping Study Minfeng Xu Feb. 15, 2005.
12 March 2006NFMCC Meeting, IIT, Chicago1 Progress on the MICE Cooling Channel and Tracker Magnets Michael A. Green Lawrence Berkeley Laboratory.
1 Progress on the MICE Cooling Channel Magnets Michael A. Green Lawrence Berkeley National Laboratory 28 June 2005.
1 Effect of staging on module connection and support arrangement Yury Ivanyushenkov RAL.
04/01/2006MICE Analysis Meeting1 MICE phase III M. Apollonio, J. Cobb (Univ. of Oxford)
MICE AFC Group phone conference on 27 January 2005 AFC module progress By Wing Lau, Oxford.
M.apollonio/j.cobbMICE UK meeting- RAL - (9/1/2007) 1 Single Particle Amplitude M. Apollonio – University of Oxford.
MICE magnetic measurements Sequence of events and MICE hall movements Alain Blondel – 10-April 2012 revision from 13 December 2012.
Emittance measurement: ID muons with time-of-flight Measure x,y and t at TOF0, TOF1 Use momentum-dependent transfer matrices iteratively to determine trace.
MICE CM30 Magnetic Shielding Update Mike Courthold 6 th July
Emittance measurement: ID muons with time-of-flight Measure x,y and t at TOF0, TOF1 Use momentum-dependent transfer matrices to map  path Assume straight.
M.apollonioCM17 -CERN- (22/2-25/2/2007)1 M. Apollonio – University of Oxford sizes for PID & shields.
MICE collaboration meeting Alain Blondel 27 – Welcome to the 10th MICE collaboration meeting. 1.Global neutrino factory situation 2.Possible.
Magnetic Shielding Issues Roy Preece STFC - RAL. Overview Issues Items in harms way – Step IV Step IV mitigation plan –Racks –Compressors Current / Future.
The status of the construction of MICE Step IV K. Long, on behalf of the MICE collaboration.
MICE CM32 8 th February 2012 Magnet Group Report Vicky Bayliss Victoria Blackmore John Cobb Mike Courthold Roy Preece Mike Zisman 1.
1 Layout and Installation MICE Collaboration Meeting, RAL, October 27-29, 2004 Elwyn Baynham, Tom Bradshaw, Paul Drumm, Matthew Hills, Yury Ivanyushenkov,
MICE magnetic measurements: AFC considerations Alain Blondel see a previous discussion for reference in CM35 (Feb 2013 slides by V. Blackmore, A. Blondel.
1 Forces Yury Ivanyushenkov RAL. 2 Goal: find maximal (static and dynamical) possible forces in MICE magnetic system. Method: calculation of axial magnetic.
1 MICE Radiation Shielding MICE Phone Conference, 28 January 2004 Yury Ivanyushenkov Engineering Department, RAL.
PID PC 7th Sept MICE MAGNETIC FIELDS & SHIELDS J. H. Cobb & H. Witte Oxford University Magnet fields for MICE (VI) calculated including magnetic.
22 October 2005MICE Meeting at RAL1 Tracker Solenoid Overview Michael A. Green Lawrence Berkeley Laboratory MICE Collaboration Meeting 22 October 2005.
Global Design Effort Magnetic and Mechanical FEA of SiD IRENG07 Bob Wands September 18, 2007.
Re-tuning MICE June 1 st 2010 Tim Carlisle. Intro At the moment MICE coil currents optimized for: central Pz = 0 RF No LH2 want to rematch M1 & M2 in.
1 Status of infrastructure MICE Collaboration Meeting, Frascati, June 26-29, 2005 Yury Ivanyushenkov Applied Science Division, Engineering and Instrumentation.
MICE CM32 25 th February 2012 Magnet Group Report Vicky Bayliss Victoria Blackmore John Cobb Mike Courthold Roy Preece Mike Zisman 1.
1 OPTICS OF MICE STEP V.0 Ulisse Bravar University of New Hampshire 26 June 2005.
26 Aug 2008PC Shield walls – extend the length of channel – will ‘pull’ field x y Coil Centred coil + 2 walls  X – Y asymmetry Off-centre coil +
1 Implementation at RAL Iouri Ivaniouchenkov on behalf of Elwyn Baynham, Tom Bradshaw, Tony Jones, Jim Rochford Engineering Department, RAL MICE Collaboration.
(one of the) Request from MPB
CM Nov 2009 DOES MICE NEED STEP III ? Somewhat hard to understand MICE Schedule… –If the gods are (un)kind it’s possible that SS1, SS2 & FC1 are.
MICE news Alain Blondel 20 – NEWS 1.CERN’s SPSC at Villars: recommandations 2.MICE step Upcoming gateway steps 4.RF from LBNL (Mike)
MICE Step IV Lattice Design Based on Genetic Algorithm Optimizations
Outcome of the Review and Response to Recommendations
Validating Magnets Using Beam
Effect of Reduced Focus Coil Current on Step IV and Step VI
Impact of Magnet Performance on the Physics Program of MICE
Presentation transcript:

1 Search for Worst-Case Forces MICE Video Conference, September 8, 2004 Yury Ivanyushenkov Applied Science Division, Engineering and Instrumentation Department, RAL

2 Aims of work Goal: find maximal (static and dynamical) possible forces in MICE magnetic system. Method: calculation of axial magnetic forces in MICE by using OPERA package (and other codes). Cases to be analyzed: - MICE stages III, IV, V and VI (see next slide): Parameters (proposal): magnetic modes - flip, semi-flip and non-flip; momentum (MeV/c) – 140, 170, 200, 240; beta (cm) – 7, 15, 25, 42; gap focus coil – match coil (mm) (was 600) ; coil currents - 0 (coil is off or quenched), nominal, max (critical current ?); magnetic shielding – with and without. - Abnormal cases: - dynamical forces during quenches; - anything else?

3 STEP I: STEP II STEP III STEP IV STEP V STEP VI By A.Blondel MICE stages

4 Model (without shielding) in OPERA Model: -18 coils; - no iron shielding

(SFOFO, 200 MeV/c, beta=42 cm, gap =600 mm) 404 Centre coils: J=64.44 A/mm 2 Focusing coils: J= A/mm 2 Coupling coils: J=96.21 A/mm 2 End #2 coils: J=67.11 A/mm Matching #2 coils: J=41.46 A/mm Matching #1 coils: J=65.06 A/mm 2 End #1 coils: J=65.22 A/mm Gap=600 MICE magnetic system geometry Note: Geometry and currents from Ulisse before Osaka meeting

6 (SFOFO, p=200 MeV/c, beta=42 cm, gap =450 mm) All forces are in tonnes ! 147 Centre coils: J=64.44 A/mm 2 Coupling coils: J=96.21 A/mm 2 End #2 coils: J=67.11 A/mm 2 Matching #2 coils: J=75.17 A/mm 2 Matching #1 coils: J=56.30 A/mm 2 End #1 coils: J=61.59 A/mm 2 Focusing coils: J= A/mm Forces in MICE magnetic system 14

(SFOFO, p=200 MeV/c, beta=42 cm, gap =600 mm) (SFOFO, p=200 MeV/c, beta=42 cm, gap =450 mm) Forces Vs. Gap for p=200 Mev/c

8 (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm) All forces are in tonnes ! 147 Centre coils: J=64.44 A/mm 2 Coupling coils: J= A/mm 2 End #2 coils: J=67.11 A/mm 2 Matching #2 coils: J=83.07 A/mm 2 Matching #1 coils: J=66.82 A/mm 2 End #1 coils: J=61.59 A/mm 2 Focusing coils: J= A/mm Forces in MICE magnetic system 21.5

9 Forces Vs. p for gap=450 mm (SFOFO, p=200 MeV/c, beta=42 cm, gap =450 mm) (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm) All forces are in tonnes !

10 (SEMI-FLIP, p=200 MeV/c, beta=42 cm, gap =600 mm) All forces are in tonnes ! 146 Centre coils: J=63.81 A/mm 2 Coupling coils: J=93.10 A/mm 2 End #2 coils: J=67.11 A/mm 2 Matching #2 coils: J=34.99 A/mm 2 Matching #1 coils: J=68.33 A/mm 2 End #1 coils: J=64.01 A/mm 2 Focusing coils: J=68.03 A/mm Forces in MICE magnetic system 46.7

11 (NON-FLIP, p=200 MeV/c, beta=42 cm, gap =600 mm) All forces are in tonnes ! 146 Centre coils: J=63.81 A/mm 2 Coupling coils: J=93.10 A/mm 2 End #2 coils: J=67.11 A/mm 2 Matching #2 coils: J=34.99 A/mm 2 Matching #1 coils: J=68.33 A/mm 2 End #1 coils: J=64.01 A/mm 2 Focusing coils: J=68.03 A/mm Forces in MICE magnetic system 15.7

12 Net Force, tonne / Case SFOFO, p=200 Mev/c, beta=42 cm SFOFO, p=240 Mev/c, beta=42 cm SEMI-FLIP, p=200 Mev/c, beta=42 cm NON-FLIP, p=200 Mev/c, beta=42 cm Gap=450 mm Gap=600 mm Gap=450 mm Gap=600 mm Central focus pair Edge focus pair7 from centre 5 towards centre 8.6 from centre 8 towards centre 13.5 towards centre 15.3 towards centre Coupling coil14 from centre 15 from centre 21.5 from centre 23 from centre 46.7 from centre 15.7 towards centre Tracker solenoid24.3 towards centre 12.5 towards centre 33.3 towards centre 17.3 towards centre 39.4 towards centre 26.3 towards centre Summary table for axial magnetic forces

13 (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm, Focus Coils quenched) All forces are in tonnes ! Centre coils: J=64.44 A/mm 2 Coupling coils: J= A/mm 2 End #2 coils: J=67.11 A/mm 2 Matching #2 coils: J=83.07 A/mm 2 Matching #1 coils: J=66.82 A/mm 2 End #1 coils: J=61.59 A/mm 2 Focusing coils: J=0 A/mm Forces in MICE magnetic system: Quenches

14 (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm, Focus Coils quenched) All forces are in tonnes ! 6.30 Forces in MICE magnetic system: Quenches (2) (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm)

15 (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm, Coupling Coils quenched) All forces are in tonnes ! Centre coils: J=64.44 A/mm 2 Coupling coils: J=0 A/mm 2 End #2 coils: J=67.11 A/mm 2 Matching #2 coils: J=83.07 A/mm 2 Matching #1 coils: J=66.82 A/mm 2 End #1 coils: J=61.59 A/mm 2 Focusing coils: J= A/mm Forces in MICE magnetic system: Quenches (3) 0

16 Forces in MICE magnetic system: Quenches (4) (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm, Coupling Coils quenched) All forces are in tonnes ! (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm)

17 (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm, Detector Magnets quenched) All forces are in tonnes ! 0 Centre coils: J=0 A/mm 2 Coupling coils: J= A/mm 2 End #2 coils: J=0 A/mm 2 Matching #2 coils: J=0 A/mm 2 Matching #1 coils: J=0 A/mm 2 End #1 coils: J=0 A/mm 2 Focusing coils: J= A/mm Forces in MICE magnetic system: Quenches (5) 31.3

18 (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm, Detector Magnets quenched) All forces are in tonnes ! Forces in MICE magnetic system: Quenches (6) (SFOFO, p=240 MeV/c, beta=42 cm, gap =450 mm)

19 Net Force, tonne / Case Normal mode Coils quenched: Focus coilsCoupling coils Detector magnets Central focus pair0000 Edge focus pair8.6 from centre from centre 31.2 towards centre Coupling coil21.5 from centre 21.1 from centre from centre Tracker solenoid33.3 towards centre 6.3 from centre 43.5 towards centre 0 Summary table for axial magnetic forces: Quench cases SFOFO, p=240 Mev/c, beta=42 cm, gap=450 mm

20 Forces in MICE magnetic system: Effect of shielding disks (SFOFO, p=200 MeV/c, beta=42 cm, gap =600 mm) Without shielding disks With shielding disks

21 Conclusions Conclusions (preliminary): so far, the highest net forces on modules are created in SEMI-FLIP mode (but the highest net force on the edge focus pair is in case of NON- FLIP mode) -> it seems there is no a single worst case for all the modules; for FLIP mode forces are the highest for 240 MeV/c; both the edge focus pair and the tracker solenoid (but not the coupling coil) are sensitive to the value of the gap; forces change when some of coils are quenched; shielding disks change forces on the detector module

22 Next steps New set of currents for various MICE stages and magnetic modes has been recently released by Ulisse Bravar. Proposal for the next steps: agree on parameter space for force cases; get from Ulisse a complete set of currents (and geometries) for all stages and magnetic modes; ask John Cobb to make a quick scan of parameter space by using his code to indicate the worst cases; check worst cases with OPERA including shielding in the model; collect recommendations from the Collaboration on abnormal cases and include these cases into the analysis; dynamical cases – ask for help from magnet experts; anything else ?