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Mauricio Lopes – FNAL
Introduction to superconducting magnets*
US Particle Accelerator School – Grand Rapids, MI – June 2012
* From: “Superconducting Accelerator Magnets” by Paolo Ferracin, Ezio Todesco, Soren O. Prestemon and Helene Felice, January 2012
A Brief History of the Superconductivity
US Particle Accelerator School – Grand Rapids, MI – June 2012 2
Heike Kamerlingh Onne
1908 – Successfully liquified helium (4.2 K) 1911 – Discovered the superconductivity while measuring the conductivity of Mercury as function of temperature 1913 – Nobel prize
US Particle Accelerator School – Grand Rapids, MI – June 2012 3
1933 – Walther Meissner and Robert Ochsenfeld discover perfect diamagnetic property of supeconductors. 1935 – First theoretical works on SC by Heinz and Fritz London 1950 – Ginzburg and Landau proposed a macroscopic theory for SC.
Meissner effect
A Brief History of the Superconductivity
Why using SC magnets?
US Particle Accelerator School – Grand Rapids, MI – June 2012 4
𝐵𝑟 =𝑃
𝑞=
𝐾2 + 2𝐾𝐸𝑜
𝑞𝑐
Example: Lets calculate the magnetic rigidity for a 1 TeV proton:
𝐵𝑟 ≈1 𝑇𝑒𝑉
𝑐≈ 3333 𝑇. 𝑚
Let us assume a maximum field of 1.5 T; the circumference of such machine will be:
𝑟 = 2222 𝑚 𝐶 = 2𝜋𝑟 ≈ 14 𝑘𝑚
The Tevatron was the first machine to use large scale superconductor magnets with a 4.2 T in a 6.3 km circumference!
Critical surface
US Particle Accelerator School – Grand Rapids, MI – June 2012 5
Critical surface for different SC materials
US Particle Accelerator School – Grand Rapids, MI – June 2012 6
10
100
1,000
10,000
100,000
1,000,000
0 5 10 15 20 25 30 35
Applied Field, T
S
up
erc
on
du
cto
r C
riti
cal C
urr
en
t D
en
sit
y,
A/m
m²
YBCO: Tape, || Tape-plane, SuperPower (Usedin NHMFL tested Insert Coil 2007)
YBCO: Tape, |_ Tape Plane, SuperPower (Usedin NHMFL tested Insert Coil 2007)
Bi-2212: non-Ag Jc, 427 fil. round wire, Ag/SC=3(Hasegawa ASC-2000/MT17-2001)
Nb-Ti: Max @1.9 K for whole LHC NbTi strandproduction (CERN, Boutboul '07)
Nb-Ti: Nb-47wt%Ti, 1.8 K, Lee, Naus andLarbalestier UW-ASC'96
Nb3Sn: Non-Cu Jc Internal Sn OI-ST RRP 1.3mm, ASC'02/ICMC'03
Nb3Sn: Bronze route int. stab. -VAC-HP, non-(Cu+Ta) Jc, Thoener et al., Erice '96.
Nb3Sn: 1.8 K Non-Cu Jc Internal Sn OI-ST RRP1.3 mm, ASC'02/ICMC'03
Nb3Al: RQHT+2 At.% Cu, 0.4m/s (Iijima et al2002)
Bi 2223: Rolled 85 Fil. Tape (AmSC) B||, UW'6/96
Bi 2223: Rolled 85 Fil. Tape (AmSC) B|_, UW'6/96
MgB2: 4.2 K "high oxygen" film 2, Eom et al.(UW) Nature 31 May '02
MgB2: Tape - Columbus (Grasso) MEM'06
2212 round wire
2223 tape B|_
At 4.2 K Unless Otherwise Stated
Nb3Sn Internal Sn
Nb3Sn 1.8 K
2223 tape B||
Nb3Sn ITER
MgB2 film
MgB2
tape
Nb3Al: RQHT
1.9 K LHC
Nb-Ti
YBCO B||c
YBCO B||ab
NbTi Parameterization
US Particle Accelerator School – Grand Rapids, MI – June 2012 7
7.1
0
0 1C
CCT
TBTB
where BC0 is the critical field at zero temperature (BC0 ~14.5 T)
7.1
0_
11),(
cccrefc
c
T
T
B
B
B
B
B
C
J
TBJ
where JC_ref is the critical current density at 4.2 K and 5 T (JC_ref ~ 3000 A/mm2); C, , and are fitting parameters:
C ~ 31.4 T ~ 0.63 ~ 1.0 ~ 2.3
(Lubell’s formula)
(Bottura’s formula)
Nb3Sn Parameterization
US Particle Accelerator School – Grand Rapids, MI – June 2012 8
22
0
2
)(1
),(1
)(),,(
cc
cT
T
TB
B
B
CTBJ
)(77.11
)(31.01
)(1
),(
0
2
0
2
00
cccc
c
T
TLn
T
T
T
T
B
TB
where:
2/17.1
_0 1)( mCC
7.1
_0 1),( mcc BTB
3/17.1
_00 1)( mcc TT
and:
= 900 = -0.003 Tc0_m = 18K C0_m = 48500 AT1/2/mm2 (for Jc = 3000 A/mm2 @ 4.2 K and 12 T)
(Summer’s formula)
Strand Fabrication
US Particle Accelerator School – Grand Rapids, MI – June 2012 9
Superconducting cables
• Most of the superconducting coils for particle accelerators are wound from a multi-strand cable.
• The advantages of a multi-strand cable are: – reduction of the strand piece length; – reduction of number of turns
• easy winding; • smaller coil inductance
– less voltage required for power supply during ramp-up; – after a quench, faster current discharge and less coil voltage.
– current redistribution in case of a defect or a quench in one strand.
• The strands are twisted to – reduce interstrand coupling currents (see interfilament coupling currents)
• Losses and field distortions
– provide more mechanical stability
• The most commonly used multi-strand cables are the Rutherford cable and the cable-in-conduit.
US Particle Accelerator School – Grand Rapids, MI – June 2012 10
Superconducting cables • Rutherford cables are fabricated by a cabling machine.
– Strands are wound on spools mounted on a rotating drum.
– Strands are twisted around a conical mandrel into an assembly of rolls (Turk’s head). The rolls compact the cable and provide the final shape.
US Particle Accelerator School – Grand Rapids, MI – June 2012 11
Superconducting cables
• The final shape of a Rutherford cable can be rectangular or trapezoidal. • The cable design parameters are:
– Number of wires Nwire
– Wire diameter dwire
– Cable mid-thickness tcable
– Cable width wcable
– Pitch length pcable
– Pitch angle cable (tan cable = 2 wcable / pcable) – Cable compaction (or packing factor) kcable
– i.e the ratio of the sum of the cross-sectional area of the strands (in the
direction parallel to the cable axis) to the cross-sectional area of the cable.
• Typical cable compaction: from 88% (Tevatron) to 92.3% (HERA).
cablecablecable
wirewirecable
tw
dNk
cos4
2
US Particle Accelerator School – Grand Rapids, MI – June 2012 12
US Particle Accelerator School – Grand Rapids, MI – June 2012 13
Cable insulation
• The cable insulation must feature – Good electrical properties to withstand
high turn-to-turn voltage after a quench.
– Good mechanical properties to withstand high pressure conditions
– Porosity to allow penetration of helium (or epoxy)
– Radiation hardness
• In NbTi magnets the most common insulation is a series of overlapped layers of polyimide (kapton).
• In the LHC case: – two polyimide layers 50.8 µm thick
wrapped around the cable with a 50% overlap, with another adhesive polyimide tape 68.6 µm thick wrapped with a spacing of 2 mm.
US Particle Accelerator School – Grand Rapids, MI – June 2012 14
Superconducting Magnets Design Perfect dipole
-60
0
60
-40 0 40
+
+-
-
-60
0
60
-40 0 40
+
+-
-
A wall-dipole, cross-section A practical winding with flat cables
1 - Wall dipole (similar to the window frame magnet)
US Particle Accelerator School – Grand Rapids, MI – June 2012 15
Superconducting Magnets Design Perfect dipole
2 - Intersecting ellipsis
-60
0
60
-40 0 40
+
+-
-
-60
0
60
-40 0 40
+
+-
-
Intersecting ellipses A practical (?) winding with flat cables
US Particle Accelerator School – Grand Rapids, MI – June 2012 16
Intersecting Cylinders
US Particle Accelerator School – Grand Rapids, MI – June 2012 17
within a cylinder carrying uniform current j0, the field is perpendicular to the radial direction and proportional to the distance to the center r: Combining the effect of the two cylinders Similar proof for intersecting ellipses
2
00 rjB
0sinsin2
2211
00
rrrj
Bx
sj
rrrj
By2
coscos2
00
2211
00
Superconducting Magnets Design Perfect dipole 3 – Cos() current distribution
-60
0
60
-40 0 40
+
+-
-j = j0 cos
US Particle Accelerator School – Grand Rapids, MI – June 2012 18
Superconducting Magnets Design Perfect quadrupole
US Particle Accelerator School – Grand Rapids, MI – June 2012 19
-60
0
60
-40 0 40
+
+
- - j = j 0 cos 2
- -
+
+
Quadrupole as an ideal cos2
-60
0
60
-40 0 40
+
+
- -
- -
+
+
Quadrupole as two intersecting ellipses
Dipole design using sector coils
US Particle Accelerator School – Grand Rapids, MI – June 2012 20
-60
0
60
-40 0 40
+
+-
-j = j0 cos
+
+
-
-
w
r
1
1
)(n
n
ref
nR
zCzB
n
ref
ref
nz
R
R
IC
0
0
2
0
0
0
01
cos
2
1Re
2 z
I
z
IB
ddjI
sin2cos
22 00
1 wj
ddj
B
wr
r
Multipoles of a dipole sector coil
US Particle Accelerator School – Grand Rapids, MI – June 2012 21
wr
r
n
n
refwr
r
n
n
ref
n ddinRj
ddinRj
C 1
1
0
1
0)exp(
)exp(
22
r
wRjB
ref1log)2sin(
0
2
n
rwr
n
nRjB
nnn
ref
n
2
)()sin(2 221
0
for n = 2
for n > 2
wrr
jRB
ref 11
3
)3sin(2
0
3
33
4
0
5
11
5
)5sin(
wrr
jRB
ref
for =/5 (36°) or for =2/5 (72°) B5=0 for =/3 (60°) B3=0
Multi-sector dipole coil
US Particle Accelerator School – Grand Rapids, MI – June 2012 22
0.0
5.0
10.0
15.0
20.0
25.0
30.0
35.0
40.0
45.0
50.0
1
23
wrr
jRB
ref 11
3
3sin3sin3sin 123
2
0
3
33
123
4
0
5)(
11
5
5sin5sin5sin
wrr
jRB
ref
0)5sin()5sin()5sin(
0)3sin()3sin()3sin(
123
123
(48°,60°,72°) or (36°,44°,64°) are some of the possible solutions
[0°-43.2°, 52.2°-67.3°] sets also B7 = 0 !
Multi-sector dipole coil
US Particle Accelerator School – Grand Rapids, MI – June 2012 23
0)3sin()3sin()3sin()3sin()3sin( 12345
0)5sin()5sin()5sin()5sin()5sin( 12345
0)7sin()7sin()7sin()7sin()7sin( 12345
0)9sin()9sin()9sin()9sin()9sin( 12345
0)11sin()11sin()11sin()11sin()11sin( 12345 (B3, B5 and B7) = 0
[0°-33.3°, 37.1°- 53.1°, 63.4°- 71.8°] sets (B3, B5, B7 , B9 and B11) = 0!
Examples
US Particle Accelerator School – Grand Rapids, MI – June 2012 24
0
20
40
60
0 20 40 60x (mm)
y (
mm
)RHIC main dipole - 1995 Tevatron main dipole - 1980
0
20
40
60
0 20 40 60x (mm)
y (
mm
)
Two layer design
US Particle Accelerator School – Grand Rapids, MI – June 2012 25
0
50
0 50
1
2
r
w
wrwrwrrB
2
11)3sin(
11)3sin( 213
3323315)2(
1
)(
1)5sin(
)(
11)5sin(
wrwrwrrB
0
20
40
60
80
0 20 40 60 80x (mm)
y (
mm
)
72o
37o
0
15
30
45
60
75
90
0.0 0.1 0.2 0.3 0.4 0.5 0.6
w/r (adim)
Angle
(deg
rees)
a1 - first branch a2 - first branch
a1 - second branch a2 - second branch
1 2
21
Tevatron main dipole
Quadrupole design using sector coils
US Particle Accelerator School – Grand Rapids, MI – June 2012 26
-50
0
50
-50 0 50
+
+
+
+
--
- -
r w
1
1
)(n
n
ref
nR
zCzB
n
ref
ref
nz
R
R
IC
0
0
2
2
0
0
2
0
0
2
2cos
2
1Re
2 z
RI
z
RIB
refref
ddjI
r
wRjdd
RjB
refwr
r
ref1ln2sin
42cos
28
0
0
2
0
2
Multipoles of a quadrupole sector coil
US Particle Accelerator School – Grand Rapids, MI – June 2012 27
44
5
0
6
11
6
)6sin(
wrr
jRB
ref
88
8
0
10
11
10
)10sin(
wrr
jRB
ref
for =/6 (30°) one has B6 = 0
for =/10 (18°) or =/5 (36°) one sets B10 = 0
It follows the same philosophy of the Dipole design!
Examples
US Particle Accelerator School – Grand Rapids, MI – June 2012 28
Tevatron main quadrupole
0
20
40
0 20 40 60 80x (mm)
y (
mm
)
RHIC main quadrupole
0
20
40
0 20 40 60 80x (mm)
y (
mm
)
~[0°-12°, 18°-30°] ~[0°-18°, 22°-32°]
0
20
40
0 20 40 60 80x (mm)
y (
mm
)
LHC main quadrupole
~[0°-24°, 30°-36°]
Peak field and bore field ratio (l)
US Particle Accelerator School – Grand Rapids, MI – June 2012 29
0
20
40
60
80
0 20 40 60 80x (mm)
y (
mm
)
LHC main dipole – location of the peak field
0
20
40
60
80
0 20 40 60 80x (mm)
y (
mm
)
RHIC main dipole – location of the peak field
0
20
40
60
80
0 20 40 60 80x (mm)
y (
mm
)
Tevatron main dipole – location of the peak field
Peak field and bore field ratio (l)
US Particle Accelerator School – Grand Rapids, MI – June 2012 30
1.0
1.1
1.2
1.3
1.4
1.5
1.6
0 20 40 60 80width (mm)
l (
adim
)
1 layer 60
1 layer 48-60-72
1 layer 42.8-51.6-67
1 layer three blocks
1.0
1.1
1.2
1.3
1.4
1.5
1.6
0 20 40 60 80width (mm)
l (
adim
)
1 layer 60
1 layer 48-60-72
1 layer 42.8-51.6-67
1 layer three blocks
Fit
w
arrw 1~),(l a ~ 0.045
Examples
US Particle Accelerator School – Grand Rapids, MI – June 2012 31
1.0
1.1
1.2
1.3
0.0 0.5 1.0 1.5 2.0equivalent width w/r
l [
adim
]
TEV MB HERA MB
SSC MB RHIC MB
LHC MB Fresca
MSUT D20
HFDA NED
Operational Margin
US Particle Accelerator School – Grand Rapids, MI – June 2012 32
24 %
Lorentz Forces
US Particle Accelerator School – Grand Rapids, MI – June 2012 33
• A superconducting accelerator magnet has a large magnetic stored energy
• A quench produces a resistive zone
• Current is flowing through the magnet
• The challenge of the protection is to provide a safe conversion of the magnetic energy to heat in order to minimize – Peak temperature (“hot spot”) and temperature gradients in the magnet
– Peak voltages
• The final goal being to avoid any magnet degradation – High temperature => damage to the insulation or stabilizer
– Large temperature gradient => damage to the conductor due to differential thermal expansion of materials
Joule Heating Voltages (R and L)
Quench protection
US Particle Accelerator School – Grand Rapids, MI – June 2012 34
US Particle Accelerator School – Grand Rapids, MI – June 2012 35
Quench
Normal zone growth
Detection
Power supply
switched off Protection
heaters Extraction Quenchback
Trigger protection options
Current decay in the magnet
I
t
Magnetic energy
Converted to heat by Joule heating
General quench protection diagram
The faster this chain happens the safer is the magnet
Training
US Particle Accelerator School – Grand Rapids, MI – June 2012 36
Magnetization
US Particle Accelerator School – Grand Rapids, MI – June 2012 37
Magnetization
US Particle Accelerator School – Grand Rapids, MI – June 2012 38
Magnetization
US Particle Accelerator School – Grand Rapids, MI – June 2012 39
Summary
US Particle Accelerator School – Grand Rapids, MI – June 2012 40
• Design and Fabrication of Superconducting Magnets belong to a different Universe
• Although the mathematical formulation for the field generation is shared, the design of superconducting magnets involves many other aspects:
o Thermal considerations o Mechanical Analysis o Fabrication techniques o Quench Protection o Material Science
• If one is interested to learn more about superconducting magnet, one should
attend to the Superconducting Accelerator Magnets USPAS course. The material for that course can be found at:
http://etodesco.web.cern.ch/etodesco/uspas/uspas.html
Next…
US Particle Accelerator School – Grand Rapids, MI – June 2012 41
Unusual design examples