Sep 26, 2006S. Kahn -- 50 T HTS Solenoid1 A Proposal for a 50 T HTS Solenoid Steve Kahn Muons Inc. September 26, 2006.

Slides:



Advertisements
Similar presentations
Energy In a Magnetic Field
Advertisements

Superconducting Magnet Program S. Gourlay CERN March 11-12, Lawrence Berkeley National Laboratory IR Quad R&D Program LHC IR Upgrade Stephen A.
Chapter 30. Induction and Inductance
Q1 for JLAB’s 12 Gev/c Super High Momentum Spectrometer S.R. Lassiter, P.B. Brindza, M. J. Fowler, S.R. Milward, P. Penfold, R. Locke Q1 SHMS HMS Q2 Q3.
Sources of the Magnetic Field
Zian Zhu Superconducting Solenoid Magnet BESIII Workshop Zian Zhu Beijing, Oct.13,2001.
Aug 10, 2006S. Kahn T HTS Solenoid1 A Proposal for a 50 T HTS Solenoid Steve Kahn Muons Inc. August 10, 2006.
MUTAC Review, 9 April MuCOOL and MICE Coupling Magnet Status Michael A. Green Lawrence Berkeley Laboratory Berkeley CA
Preliminary Analysis of the Target System Magnets 1.Version with a 6-T copper magnet insert 2.Version with a 6-T high-temperature superconductor insert.
1 Chapter 27 Current and Resistance. 2 Electric Current Electric current is the rate of flow of charge through some region of space The SI unit of current.
1 The Genoa Tracker Solenoids and their Contribution toward a New Design Michael A. Green Lawrence Berkeley National Laboratory and Pasquale Fabbricatore.
Stellarator magnets L. Bromberg J.H. Schultz MIT Plasma Science and Fusion Center ARIES meeting March 8-9, 2004.
CM-18 June Magnet Conductor Parameters and How They affect Conductor Selection for MICE Magnets Michael Green Lawrence Berkeley Laboratory Berkeley.
Twin Solenoid Twin Solenoid - conceptual design for FCC-hh detector magnet - Matthias GT Mentink Alexey Dudarev Helder Pais Da Silva Leonardo Erik Gerritse.
Aug 29, 2006S. Kahn T HTS Solenoid1 A Proposal for a 50 T HTS Solenoid Steve Kahn Muons Inc. August 29, 2006.
Alexander Barnaveli GEORGIA №1. Electromagnetic cannon A solenoid can be used to fire a small ball. A capacitor is used to energize the solenoid coil.
Superconducting Large Bore Sextupole for ILC
MCTF Alexander Zlobin MUTAC Meeting 8-10 April MCTF Magnet and HTS Conductor R&D.
Induction and Inductance Chapter 30 Magnetic Flux.
3 Nov 2006S. Kahn -- Quench Protection1 Quench Protection of the 50 T HTS Solenoid Steve Kahn Muons Inc. 3 November 2006.
Nov PHYS , Dr. Andrew Brandt PHYS 1444 – Section 003 Lecture #20, Review Part 2 Tues. November Dr. Andrew Brandt HW28 solution.
Possible HTS wire implementation Amalia Ballarino Care HHH Working Meeting LHC beam-beam effects and beam-beam interaction CERN, 28 th August 2008.
Feb 15, 2008S. Kahn -- RF in HCC Channel1 Examination of How to Put RF into the HCC Steve Kahn Katsuya Yonehara NFMCC Meeting Feb 15, 2008 Muons, Inc.
Magnetism 1. 2 Magnetic fields can be caused in three different ways 1. A moving electrical charge such as a wire with current flowing in it 2. By electrons.
Status of CEPC Detector magnet
Mar 19, 2008 S. Kahn -- RF in HCC Channel 1 Examination of How to Put RF into the HCC Steve Kahn NFMCC Meeting Mar 19, 2008.
Magnets for muon collider ring and interaction regions V.V. Kashikhin, FNAL December 03, 2009.
Superconducting R&D – Now Strand and Cable R&D FERMILAB Magnet Systems Department – Now SC Materials Department (TD) HTS Insert Coil Test in External Solenoid.
Aug 9, 2008S. Kahn -- HCC Magnet Plans1 HCC Magnet Future Plans Steve Kahn Aug 9, 2008 NFMCC Friday Meeting.
Magnetic Field Chapter 28 opener. A long coil of wire with many closely spaced loops is called a solenoid. When a long solenoid carries an electric current,
MAGNETIC INDUCTION MAGNETUIC FLUX: FARADAY’S LAW, INDUCED EMF:
Inductance and AC Circuits. Mutual Inductance Self-Inductance Energy Stored in a Magnetic Field LR Circuits LC Circuits and Electromagnetic Oscillations.
Magnets and Supports Bob Wands October 20, 2006 PPD/MD/Engineering Analysis Group Fermilab 4 th Concept Detector at Fermilab October, 2006.
1 Feb 2007S. Kahn -- Quench Protection1 Quench Protection for Very High Field Magnets using HTS Conductors Stephen Kahn Muons Inc. NFMCC UCLA Meeting 1.
Magnet for ARIES-CS Magnet protection Cooling of magnet structure L. Bromberg J.H. Schultz MIT Plasma Science and Fusion Center ARIES meeting UCSD January.
Subscale quadrupole (SQ) series Paolo Ferracin LARP DoE Review FNAL June 12-14, 2006.
PHYSICS 222 EXAM 2 REVIEW SI LEADER: ROSALIE DUBBERKE.
Harold G. Kirk Brookhaven National Laboratory High-Field Solenoids for a MC Final Cooling System AAC 2012 Austin, Texas June 11-15, 2012.
SI leader: Rosalie Dubberke
Monday, Apr. 16, 2012PHYS , Spring 2012 Dr. Jaehoon Yu 1 PHYS 1444 – Section 004 Lecture #20 Monday, April 16, 2012 Dr. Jaehoon Yu Today’s homework.
BNL High Field and HTS Magnet Program Ramesh Gupta BNL, NY USA H T.
Nov 9, 2005S. Kahn -- Solenoid Proposal1 High Field Solenoid Discussions at BNL Steve Kahn Muons Inc. Nov 9, 2005.
Monday, April 23, PHYS , Spring 2007 Dr. Andrew Brandt PHYS 1444 – Section 004 Lecture #19 Monday, April 23, 2007 Dr. Andrew Brandt Inductance.
CERN Accelerator School Superconductivity for Accelerators Case study 3 Paolo Ferracin ( ) European Organization for Nuclear Research.
2 July 2002Realistic Fields for a Ring Cooler Magnet System -- S.Kahn Page 1 Realistic Fields for a Ring Cooler Steve Kahn 2 July 2002 NuFact’02 Meeting.
Helical Solenoid Development
Muons, Inc. 14 Jan 2010 S. Kahn--IR Quads 1 IR Quadrupoles with Exotic Materials Steve Kahn, Muons Inc. Bob Palmer, BNL Don Summers, Ole Miss.
Study of the HTS Insert Quench Protection M. Sorbi and A. Stenvall 1 HFM-EuCARD, ESAC meeting, WP 7.4.1CEA Saclay 28 feb. 2013,
Magnet R&D for Large Volume Magnetization A.V. Zlobin Fermilab Fifth IDS-NF Plenary Meeting 8-10 April 2010 at Fermilab.
J. Polinski, B. Baudouy -The NED heat transfer program at CEA CEA Saclay, January 11th NED heat transfer program at CEA NED heat transfer program.
Thermal screen of the cryostat Presented by Evgeny Koshurnikov, GSI, Darmstadt September 8, 2015 Joint Institute for Nuclear Research (Dubna)
Chapter 28 Sources of Magnetic Field Ampère’s Law Example 28-6: Field inside and outside a wire. A long straight cylindrical wire conductor of radius.
FNAL Workshop, July 19, 2007 ILC Main Linac Superconducting Quadrupole V.Kashikhin 1 ILC Main Linac Superconducting Quadrupole (ILC HGQ1) V. Kashikhin.
CHATS-AS 2011clam1 Integrated analysis of quench propagation in a system of magnetically coupled solenoids CHATS-AS 2011 Claudio Marinucci, Luca Bottura,
Jim Kerby Fermilab With many thanks to Vladimir Kashikhin, the FNAL, KEK, and Toshiba teams. SCRF BTR Split Quadrupole ILC ML & SCRF Baseline Technical.
Magnetics.
Generic technology development - High field magnet R&D
Fundamentals of Applied Electromagnetics
Quench estimations of the CBM magnet
M. Migliorati, C. Vaccarezza INFN - LNF
Mechanical Modelling of the PSI CD1 Dipole
Electromagnetic Theory
HTS Magnet R&D at BNL Ramesh Gupta November 17, 2017.
Yingshun Zhu Accelerator Center, Magnet Group
PHYS 1444 – Section 003 Lecture #21
Design and Optimization of Force-Reduced Superconducting Magnets
The superconducting solenoids for the Super Charm-Tau Factory detector
Quench calculations of the CBM magnet
Chapter 28 Sources of Magnetic Field
Budker Institute of Nuclear Physics,
Presentation transcript:

Sep 26, 2006S. Kahn T HTS Solenoid1 A Proposal for a 50 T HTS Solenoid Steve Kahn Muons Inc. September 26, 2006

Sep 26, 2006S. Kahn T HTS Solenoid2 Alternating Solenoid Lattice for Cooling We plan to use high field solenoid magnets in the near final stages of cooling. The need for a high field can be seen by examining the formula for equilibrium emittance: The figure on the right shows a lattice for a 15 T alternating solenoid scheme previously studied.

Sep 26, 2006S. Kahn T HTS Solenoid3 From R. Palmer

Sep 26, 2006S. Kahn T HTS Solenoid4

Sep 26, 2006S. Kahn T HTS Solenoid5 A Proposal for a High Field Solenoid Magnet R&D The availability of commercial high temperature superconductor tape (HTS) should allow significantly higher field that can produce smaller emittance muon beams. HTS tape can carry significant current in the presence of high fields where Nb 3 Sn or NbTi conductors cannot. We would like to see what we can design with this commercially available HTS tape.

Sep 26, 2006S. Kahn T HTS Solenoid6 Comparison of J E for HTS Conductors We have chosen to use Bi2223 since it is available as a reinforced tape from AMSC The conductor can carry significant current at very high fields. NbTi and Nb 3 Sn can not.

Sep 26, 2006S. Kahn T HTS Solenoid7 Properties of American Superconductor’s High Temperature Superconductor Wire 6% more current per turn 10 % more turns per radial space New and Improved High Strength Plus Tape High Strength Tape used for calculations

Sep 26, 2006S. Kahn T HTS Solenoid8 Cross Sections of AMSC HTS Tape High Strength Tape High Compression Tape High Current Tape React and Wind

Sep 26, 2006S. Kahn T HTS Solenoid9 Some Mechanical Properties of Oxford BSSCO-2212 Young’s Modulus E~51-63 GPa Ultimate Strength~130 MPa Strain Degradation at 0.4% Wind and React

Sep 26, 2006S. Kahn T HTS Solenoid10 Why Do We Want to Go to Liquid Helium ? The parallel field orientation is the most relevant for a solenoid magnet. Previous calculations had used the perpendicular field. (We can view this not as a mistake, but as a contingency).

Sep 26, 2006S. Kahn T HTS Solenoid11 Current Carrying Capacity for HTS Tape in a Magnetic Field Scale Factor is relative to 77ºK with self field

Sep 26, 2006S. Kahn T HTS Solenoid12 Fit to High Field to Extrapolate Beyond 27 T We are using BSSCO 2223 which has been measured only to 27 T in the perpendicular configuration. We are using it in the parallel configuration. –We have to extrapolate to high field. We know that BSSCO 2212 has been tested to 45 T, so we think that the AMSC tape will work. –The high field measurements of BSSCO 2212 has a different falloff from BSSCO We certainly will need measurements of the AMSC tape at high field FieldQuadraticLinear

Sep 26, 2006S. Kahn T HTS Solenoid13 A Vision of a Very High Field Solenoid Design for 50 Tesla. Inner Aperture Radius: 2.5 cm. Axial Length chosen: 1 meter Use stainless steel ribbon between layers of HTS tape. –We will vary the thickness of the SS ribbon. –The SS ribbon provides additional tensile strength HTS tape has 300 MPa max tensile strength. SS-316 ribbon: choose 660 MPa (Goodfellow range for strength is MPa) Composite strength =  SS  SS + (1-  SS )  HTS (adds like parallel springs). We use the J eff associated to 50 Tesla. –We operate at 85% of the critical current. All parameters used come from American Superconductor’s Spec Sheets.

Sep 26, 2006S. Kahn T HTS Solenoid14 Constraining Each Layer With A Stainless Steel Strip Instead of constraining the forces as a single outer shell where the radial forces build up to the compressive strain limit, we can put a mini-shell with each layer. Suggested by R. Palmer, but actually implemented previously by BNL’s Magnet Division for RIA magnet. (See photo)

Sep 26, 2006S. Kahn T HTS Solenoid15 A Slightly More Aggressive Approach We can vary the amount of stainless steel interleafing as a function of radius to achieve 0.4% strain. –At small radius where we have smaller stress, we could use a smaller fraction of stainless steel. (See previous slide) –In the middle radial region we would use more stainless where the tensile strength is largest. Following this approach we can build a 50 Tesla solenoid. Case 3: 50 Tesla solenoid with SS interleaving varied to achieve 0.4% strain throughout. A 60 Tesla solenoid may be achieved by increasing the current as the field falls off with radius by using independent power supplies for different radial regions.

Sep 26, 2006S. Kahn T HTS Solenoid16 Varying SS Interleaving to Achieve Maximum Strain The thickness of the stainless steel interleaving is varied as a function of radius so as to reach the maximum allowable strain through out the magnet. –This minimizes the outer solenoid radius (and consequently the conductor costs). –This also brings the center of current closer to the axis and reduces the stored energy. –This is likely to increase the mechanical problems.

Sep 26, 2006S. Kahn T HTS Solenoid17 Case Comparisons The tables on the left summarize the parameters and results of the three cases presented. –The analysis assumes the solenoid length is 70 cm (We are now using a 1 m length.) –The top table shows the dimensional parameters: Inner/outer radius Conductor length and amp-turns. –The bottom table shows the results from the magnetic properties: Stored energy Radial and Axial Forces

Sep 26, 2006S. Kahn T HTS Solenoid18 Comments on Stored Energy The 70 cm length was chosen to be consistent with the range of ~100 MeV muon. It is also the minimum solenoid length where there is some “non-fringing” central field. The stored energy of the 50 Tesla magnet (case 3) is 20 Mega- Joules (for 70 cm). –This can be compared to 7 Mega-Joules for the 10 m long LHC 2-in-one dipole. The LHC quench protection system actually handles a string of dipoles in a sextant (?). There are differences between HTS and NbTi that need to be considered for quench protection. –HTS goes resistive at a slower rate than NbTi. –A quench propagates at a slower velocity in HTS than for NbTi. –We will have to perform computer simulations of quench protection for the HTS system to determine how to protect the magnet in case of an incident.

Sep 26, 2006S. Kahn T HTS Solenoid19 What about Axial Forces? There is a significant contribution to the axial forces from the fringing radial fields at the ends. –In the 50 Tesla solenoid shown we will see a fringing field of 9 Tesla –We have seen that there is a total axial compressive force at the center of ~30 Mega-Newtons.

Sep 26, 2006S. Kahn T HTS Solenoid20 More on Compressive Forces The top figure shows the Lorentz force density at the end of the solenoid as a function of radius for the three cases. –The axial pressure on the end is P=J  B r  t where t is the tape width. This peaks at 10 MPa. The lower figure shows the Lorentz force density along the length for the peak radial position. –It is largest at the end and falls to zero at center as expected. These stresses are not large. Do we have to worry about compressive strain along the axial direction? –The maximum allowable compressive strain for the tape is 0.15%.

Sep 26, 2006S. Kahn T HTS Solenoid21 Formulate R&D Plan Initial measurements of material properties. –J C measurements under tensile and compressive strain. –Modulus measurements of conductor. –Thermal cycling to 4  K. Formulate and prepare inserts for high field tests. –Design insert for test in 30 Tesla magnet. This magnet has a reasonable size aperture. –At 30 Tesla, some part of the insert should be at the strain limit. –Program for conductor tests at 45 Tesla. 45 Tesla magnet has limited aperture (3.1 cm). It has a warm aperture. There is a 38 Tesla facility in Japan that could be used if the 45 Tesla facility is not available.

Sep 26, 2006S. Kahn T HTS Solenoid22 Preliminary Calculations for Quench Protection I am presenting some preliminary calculations using the quench calculation program QUENCH. –This program was written by Martin Wilson at Rutherford Lab in the 1970’s. The current version of the program is marketed by B. Hassenzahl of Advanced Energy Analysis. BNL has a license to use it. There are other codes available: –QUENCHPRO at FNAL Technical Division. –SPQR from CERN. –Vector Fields is developing a quench propagation code ??

Sep 26, 2006S. Kahn T HTS Solenoid23 Conductor and Insulator Description The conductor is BSCCO 2223 which is 30% HTS filaments and 70% Ag matrix and Ag-Mg sheath (for strength). We assume the matrix/sheath is all Ag for the calculation. The insulator is assumed to be the Stainless Steel interleaving. A minimum thickness (0.07 mm) is used since we are describing the inner layers. –In practice we will likely add a ceramic coating or kapton wrap as insulator. This will inhibit the transverse quench propagation. ComponentAreaFraction HTS conductor mm Ag matrix/sheath mm SS Insulator0.301 mm

Sep 26, 2006S. Kahn T HTS Solenoid24 Conductor Material Properties Necessary for Quench Protection We need the material properties of all the components of the conductor and insulation. The important properties are –Heat capacitance (Specific Heat) –Resistivity –Thermal conductance Obtained from resistivity with Wiedemann-Frantz law. C V and  are parameterized as in up to four temperature ranges:

Sep 26, 2006S. Kahn T HTS Solenoid25 Critical Current Measurements Measurements of critical current as a function of B and temperature are from EHTS (another provider of BSSCO 2223). The measured data is used to determine parameters of the following equation: Used only high field part of data to determine B c20

Sep 26, 2006S. Kahn T HTS Solenoid26 Quench Propagation Velocity Quench protection calculations depend on the quench propagation velocity. The quench propagation velocity can be calculated from the formula below. –This is what I did. –Experience for NbTi shows that the formula does not reproduce the measurements. Typically the experimentally determined value is used. –We need to measure this for HTS. –One of the weaknesses of the velocity calculation is that the specific heat (  C V ) varies as T 3 and is rapidly varying at the quench front. TsTs T0T0 T1T1 Lorentz Number

Sep 26, 2006S. Kahn T HTS Solenoid27 Circuit for Quench Energy Extraction Quench circuit components: –Solenoid represented by inductance L. Also there is an internal resistance (not shown) which is about 10 ohm. –R PR represents the energy extraction resistance. This will take the large share of quench energy. –Switch will be activated by quench detection system. Could even be a diode system. –R EXT represents the resistance associated to leads, power supply, etc. R EXT LR PR R SW Power Supply Solenoid Magnet

Sep 26, 2006S. Kahn T HTS Solenoid28 Circuit Parameters QUENCH treats the whole magnet. It does not provide for segmenting the magnet into separate coupled systems. –The total inductance can be calculated from the stored energy: U=½LI 2 where U=20 Mega-Joules and I is the total amp- turns(=2.97  10 7 ). There are 444 layers  175 turns/layer = turns. This gives 280 henrys (big!) –The resistance associated with 61 km of Ag is 8 ohms. We certainly will need to trigger an external resistance into the circuit with a quench is detected.

Sep 26, 2006S. Kahn T HTS Solenoid29 Quench Parameters as a Function of External Resistance The figures show the following parameters as a function of an external resistance for energy extraction. Maximum temperature on conductor Time constant for decay External voltage on external resistance Note that as one increases the external resistance one decreases temperature, but increases the external voltage.

Sep 26, 2006S. Kahn T HTS Solenoid30 A Better Approach It may be a better approach to divide the magnet radial into separate thermally and electrically isolated systems on separate power supplies. These systems would be coupled through mutual inductance. –Each system would contain less stored energy and could have different time constants and different start times. –Different sub-systems would have different critical currents since they are at different magnetic fields. Some may not quench at all. QUNECH can not simply handle this complex system. –Do the other codes handle this or do we have to write our own? –Fermilab people may have thought about this.

Sep 26, 2006S. Kahn T HTS Solenoid31 What Do We Need to Measure? It is clear from this initial calculation that some parameters are not well known. We should try to measure them. –Electrical resistivity and heat capacity of HTS conductor as a function of temperature. This should be done above critical current. –Same measurements of Silver as a control. –Determine I c (B) at high field. Verify that the critical current relation that we used (which was developed for NbTi, Nb 3 Sn) works for HTS. –Measure the quench propagation velocity. This is important.