ACCELERATOR MAGNETS
Stephan RussenschuckCERN, AT-MEL-EM
1211 Geneva 23, Switzerland
Bending Field (Dipole) and Magnetic Rigidity
B vz × B
3.3356p[GeV/c] = R[m] B0[T]
Remark 1: Consider the “filling factor” in accelerators between 0.6 and 0.7.
Transverse Motion and the Normalized Gradient
ϕ ρ
Displaced particle at ρ = R + x with field Bz = B0 + ∂Bz∂x
∣∣∣x=0
x
1p0
dds
(p0
dxds
)+ (
1R2 − k)x = 0
For x R, e/p0 = −1/(B0R) and k = − 1B0R
∂Bz∂x
∣∣∣x=0
Quadrupole
B (vz × B)x (vz × B)y
Higher Order Multipole Fields: Sextupole
B (vz × B)x (vz × B)y
Multipole Field Errors and Beam Parameters
b1, a1 Closed orbit distortions
b2 β-beating
a2 Vertical dispersion, linear coupling
b3 Off-momentum β beating
a3 Chromatic coupling inducing detuning
b4 Dynamic aperture and detuning
a4 Dynamic aperture at injection
b5 Dynamic aperture and detuning
a5 Off-momentum dynamic aperture
b7 Dynamic aperture at injection
b6, a6,a7, > Dynamic aperture at injection
LHC in the LEP Tunnel (Virtual Reality)
Remark 2: Magnet systems are the most costly item in an accelerator
The 26 GeV Proton Synchrotron (PS) in its Tunnel
High Energy Ring Accelerator (HERA) at DESY
Magnet Metamorphosis
(C- Core, LEP Dipole)
0.00 0.15 -0.15 0.29 -0.29 0.44 -0.44 0.59 -0.59 0.73 -0.73 0.88 -0.88 1.03 -1.03 1.18 -1.18 1.33 -1.33 1.47 -1.47 1.62 -1.62 1.77 -1.77 1.92 -1.92 2.06 -2.06 2.21 -2.21 2.36 -2.36 2.50 -2.50 2.65 -2.65 2.8-
|Btot| (T)
N ⋅ I = 4480A B1 = 0.13T Bs = 0.042T Fill.fac. 0.27
Magnet Metamorphosis
(H-Magnet)
0.10 0.15 -0.15 0.29 -0.29 0.44 -0.44 0.59 -0.59 0.74 -0.74 0.88 -0.88 1.03 -1.03 1.18 -1.18 1.32 -1.32 1.47 -1.47 1.62 -1.62 1.77 -1.77 1.91 -1.91 2.06 -2.06 2.21 -2.21 2.35 -2.35 2.50 -2.50 2.65 -2.65 2.8-
|Btot| (T)
N ⋅ I = 24000A B1 = 0.3T Bs = 0.065T Fill.fac. 0.98
Magnet Metamorphosis(Cryogenic or Super-Ferric Magnet)
0.37 0.14 -0.14 0.29 -0.29 0.44 -0.44 0.58 -0.58 0.74 -0.74 0.88 -0.88 1.03 -1.03 1.18 -1.18 1.33 -1.33 1.47 -1.47 1.62 -1.62 1.77 -1.77 1.91 -1.91 2.06 -2.06 2.21 -2.21 2.36 -2.36 2.50 -2.50 2.65 -2.65 2.8-
|Btot| (T)
N ⋅ I = 96000A B1 = 1.18T Bs = 0.26T
Magnet Metamorphosis
(Window Frame Dipole)
0. 0.147-
0.147 0.294-
0.294 0.442-
0.442 0.589-
0.589 0.736-
0.736 0.884-
0.884 1.031-
1.031 1.178-
1.178 1.326-
1.326 1.473-
1.473 1.621-
1.621 1.768-
1.768 1.915-
1.915 2.063-
2.063 2.210-
2.210 2.357-
2.357 2.505-
2.505 2.652-
2.652 2.8-
|Btot| (T)
N ⋅ I = 360000A B1 = 2.08T Bs = 1.04T
Magnet Metamorphosis
(Tevatron Dipole)
0 21 42 63 84 105 126 147 168 189 210
0. 0.147-
0.147 0.294-
0.294 0.442-
0.442 0.589-
0.589 0.736-
0.736 0.884-
0.884 1.031-
1.031 1.178-
1.178 1.326-
1.326 1.473-
1.473 1.621-
1.621 1.768-
1.768 1.915-
1.915 2.063-
2.063 2.210-
2.210 2.357-
2.357 2.505-
2.505 2.652-
2.652 2.8-
|Btot| (T)
N ⋅ I = 471000A B1 = 4.16T Bs = 3.39T
Magnet Metamorphosis
(LHC Coil-Test Facility
0.00 0.15 -0.15 0.29 -0.29 0.44 -0.44 0.59 -0.59 0.74 -0.74 0.88 -0.88 1.03 -1.03 1.18 -1.18 1.32 -1.32 1.47 -1.47 1.62 -1.62 1.77 -1.77 1.91 -1.91 2.06 -2.06 2.21 -2.21 2.36 -2.36 2.50 -2.50 2.65 -2.65 2.8-
|Btot| (T)
N ⋅ I = 960000A B1 = 8.33T Bs = 7.77T
Magnet Metamorphosis
(LHC Main Dipole)
0. 0.147-
0.147 0.294-
0.294 0.442-
0.442 0.589-
0.589 0.736-
0.736 0.884-
0.884 1.031-
1.031 1.178-
1.178 1.326-
1.326 1.473-
1.473 1.621-
1.621 1.768-
1.768 1.915-
1.915 2.063-
2.063 2.210-
2.210 2.357-
2.357 2.505-
2.505 2.652-
2.652 2.8-
|Btot| (T)
N ⋅ I = 2x944000A B1 = 8.32T Bs = 7.44T
LHC Main Dipol Cross-Section
1. Heat exchanger, 2. Bus bar, 3. Superconducting coil, 4. Vacuum Pipe und Beam-screen, 5. Cryostat,6. Thermal shield (55- 75 K), 7. Helium-Tank, 8. Super-Insulation, 9. Collars, 10. Yoke
Overview
Maxwell’s equations in integral formOne-dimensional field calculation for conventional magnets
Maxwell’s equations in differential formThe solution of Laplace’s equation
Harmonic fieldsComplex Potentials
Ideal pole shapes of conventional magnetsFeed down
Solution of Poisson’s equationThe field of line currents
Generation of pure multipole fieldsSensitivity to manufacturing errors
Numerical field computationSaturation of the iron yoke
Superconducting filament magnetization
Maxwell’s Equations in Integral Form
∮H ⋅ ds =
∫A(J +
∂ D∂ t
) ⋅ dA∮E ⋅ ds = −
∂∂ t
∫A
B ⋅ dA∫A
B ⋅ dA = 0∫A
D ⋅ dA =∫
VρdV
Constitutive Equations
B = µ H = µ0(H + M)D = εE = ε0(E + P)J = κ E + Jimp.
1D Field Calculation for a Conventional Dipole
∮H ⋅ ds =
∫A
J ⋅ dA
Hiron siron + Hgap sgap =1
µ0µrBiron siron +
1µ0
Bgap sgap = N I
µr 1 Bgap =µ0N Isgap
Warning 1: Check that the magnetic circuit contains no flux concentrationwhich increases the magnetic flux density above 1 T, as in this case
fringe fields can no longer be neglected.
1D Field Calculation for a Conventional Quadrupole
∮H ⋅ ds =
∫1
H1 ⋅ ds +∫
2H2 ⋅ ds +
∫3
H3 ⋅ ds = N I
Bx = gy By = gx ⇒ H =gµ0
√x2 + y2 =
gµ0
r
∫ r0
0Hdr =
gµ0
∫ r0
0rdr =
gµ0
r202
= N I ⇒ g =2µ0NI
r20
LEP Dipole and Quadrupole
-0.13 0.864-
0.864 0.003-
0.003 0.005-
0.005 0.007-
0.007 0.009-
0.009 0.012-
0.012 0.014-
0.014 0.016-
0.016 0.018-
0.018 0.021-
0.021 0.023-
0.023 0.025-
0.025 0.028-
0.028 0.030-
0.030 0.032-
0.032 0.034-
0.034 0.037-
0.037 0.039-
0.039 0.041-
A (Tm)
0.664 0.110-
0.110 0.219-
0.219 0.328-
0.328 0.438-
0.438 0.547-
0.547 0.656-
0.656 0.766-
0.766 0.875-
0.875 0.984-
0.984 1.094-
1.094 1.203-
1.203 1.313-
1.313 1.422-
1.422 1.531-
1.531 1.641-
1.641 1.750-
1.750 1.859-
1.859 1.969-
1.969 2.078-
|Btot| (T)
Field Quality in the Dipole Aperture
Field Quality in the Dipole Aperture
|1 − ByBnom
y|
Definition of Field Quality in Accelerator Magnets
Fourier-series expansion of the radial component of the magnetic flux densityon a reference radius inside the aperture
Br(r0, ϕ) =∞∑
n=1
(Bn(r0) sin nϕ + An(r0) cos nϕ)
= BN(r0)∞∑
n=1
(bn(r0) sin nϕ + an(r0) cos nϕ)
An(r0) ≈1P
2P−1∑k=0
Br (r0, ϕk) cos nϕk , Bn(r0) ≈1P
2P−1∑k=0
Br (r0, ϕk) sin nϕk .
Remark 3: This definition is perfectly in line with magnetic fieldmeasurements using “harmonic coils” where the periodic flux variation
in tangential rotating coils is analyzed with a FFT.
Rotating Coil Measurement Setup at BNL (Brookhaven)
Maxwell’s Equations in Differential Form
curlH = J +∂ D∂ t
curlE = −∂B∂ t
div B = 0div D = ρ
Constitutive Equations
B = µ H = µ0(H + M)D = εE = ε0(E + P)J = κ E + Jimp.
Lemmata of Poincar e
The curl of an arbitrary vector field is source free div curlg = 0An arbitrary gradient field is curl free curl gradφ = 0
A source free field B, (div B = 0)can be expressed through a vector potential A in the form
B = curlA.
A curl free field H, (curlH = 0)can be expressed through a scalar potential φ in the form H = −gradΦm.
Remark 4: The field in the aperture of accelerator magnetsis curl and source free
Warning 2: The Lemmata of Poincare hold only for simply connected domains withconnected boundaries.
Maxwell’s “House”
Warning 3: Only for sub-domains with continuous material parameters.
Maxwell’s “Facade”
curl1µ
curlA = J1µ0
curl curlA = 0 ∇ 2A − grad div A = 0 ∇ 2Az = 0
div µgradΦm = 0 µ0 div gradΦm = 0 ∇ 2Φm = 0
r2∂2Az
∂r2 + r∂Az
∂r+
∂2Az
∂ϕ2 = 0
General Solution of the Laplace Equation
Az(r , ϕ ) =∞∑
n=1(Enrn + Fnr−n)(Gn sin nϕ + Hn cos nϕ)
Br (r , ϕ ) =1r
∂Az
∂ϕ=
∞∑n=1
nrn−1(Cn sin nϕ + Dn cos nϕ)
nrn−1Cn = Bn nrn−1Dn = An
Bϕ(r , ϕ ) = −∂Az
∂r= −
∞∑n=1
nrn−1(Dn sin nϕ − Cn cos nϕ)
Normal (Skew) Dipole (n=1)
Br = C1 cos ϕ + D1 sin ϕ Bϕ = −C1 sin ϕ + D1 cos ϕ
Bx = Br cos ϕ − Bϕ sin ϕ By = Br sin ϕ + Bϕ cos ϕ
Bx = C1 By = D1
Normal (Skew) Quadrupole (n=2)
Br = 2C2r cos 2ϕ + 2D2r sin 2ϕBϕ = −2C2r sin 2ϕ + 2D2r cos 2ϕBx = 2C2x + 2D2yBy = −2C2y + 2D2x
Remark 5: Notice that we have not yet addressed the problemof how to create such field distributions.
Normal (Skew) Sextupole (n=3)
Br = 3C3r2 cos 3ϕ + 3D3r2 sin 3ϕBϕ = −3C3r2 sin 3ϕ + 3D3r2 cos 3ϕBx = 3C3(x2 − y2) + 6D3xyBy = −6C3xy + 3D3(x2 − y2)
Remark 6: The treatment of each harmonic separately is a mathematical abstraction.In practical situations many harmonics will be present (to be minimized).
Analytical Field Computation for Superconducting Magnets
Special solution of the inhomogeneous (Poisson) differential equation
∇ 2A = J
Fundamental solution of the Laplace Operator ∇ 2 (Green’s Function)
(2D) G =1
2πln |r −r ′|
(3D) G =1
4π1
|r −r ′|
Vector potential of a line current (2D)
Az = −µ0I2π
ln(|r −r ′|
a)
The Field of Line Currents (2D)
R = |r −r ′|
r ′ = (ri , Θ)
r = (r0, ϕ)
ϕΘ
Iz
Az
y
z x
r0 < ri
Az = −µ0I2π
ln(|r −r ′|
a)
Br == −µ0I2π
∞∑n=1
(r n−10r ni
)(sin nϕ cos nΘ − cos nϕ sin nΘ)
Bn(r0) = −µ0I2π
r n−10r ni
cos nΘ An(r0) =µ0I2π
r n−10r ni
sin nΘ
The Imaging Method
Coil in non-saturated yoke Imaged coil
0 20 40 60 80 100 120 140 160
0 20 40 60 80 100 120 140 160
Field Harmonics in SC Magnet
Bn(r0) = −ns∑i=1
µ0Ii2π
rn−10rni
(1 +
µr − 1µr + 1
(ri
RYoke)2n
)cos nΘi
Scaling laws
Bn(r1) = (r1/r0)n−1Bn(r0)
Influence of the iron yoke (non-saturated)ri = 43.5mm, RYoke = 89mm: B1 - 19% , B5 - 0.07%
Remark 7: Analytical field optimization can be used for higher order harmonics, finiteelement calculations (for the estimation of saturation effects in the iron yoke) only
needed for the lower order harmonics.
Ideal (cos n θ) Current Distribution
Bn(r0) = −ns∑i=1
∫ ro
ri
∫ 2π
0
µ0J0 cos mΘ2π
r n−10r ni
(1 +
µr − 1µr + 1
(ri
RYoke)2n
)cos nΘi rdΘdr
Dipole Quadrupole
Ideal Current Distribution Approximated with Coil-Blocks
Dipole Quadrupole
B3 and B5 Contribution of Strand Current
Bn(r0) = −µ0Ii2π
r n−10r ni
(1 +
µr − 1µr + 1
(ri
RYoke)2n
)cos nΘi
-1.01 -0.90-
-0.90 -0.80-
-0.80 -0.69-
-0.69 -0.59-
-0.59 -0.48-
-0.48 -0.37-
-0.37 -0.27-
-0.27 -0.16-
-0.16 -0.60-
-0.60 0.045-
0.045 0.151-
0.151 0.257-
0.257 0.362-
0.362 0.468-
0.468 0.574-
0.574 0.680-
0.680 0.786-
0.786 0.892-
0.892 0.998-
(*E-3)
B3 CONTR. (T)
-0.35 -0.32-
-0.32 -0.28-
-0.28 -0.24-
-0.24 -0.20-
-0.20 -0.17-
-0.17 -0.13-
-0.13 -0.95-
-0.95 -0.58-
-0.58 -0.20-
-0.20 0.016-
0.016 0.054-
0.054 0.091-
0.091 0.129-
0.129 0.166-
0.166 0.204-
0.204 0.242-
0.242 0.279-
0.279 0.317-
0.317 0.354-
(*E-3)
B5 CONTR. (T)
Sensitivity to Coil Block Displacements
Bn(r0) = −µ0Ii2π
r n−10r ni
(1 +
µr − 1µr + 1
(ri
RYoke)2n
)cos nΘi
∂Bn(r0)∂Θi
= −µ0Ii2π
nrn−10r ni
(1+(
ri
RYoke)2n
)sin nΘi
∂Bn(r0)∂ri
=µ0Ii2π
nrn−10
r n+1i
(1−(
ri
RYoke)2n
)cos nΘi
Increase of the azimuthal coil size by 0.1 mm produces (in units of 10−4):
b1 = −14. b3 = 1.2 b5 = 0.03
Specified tolerances on coils: ± 0.025mm
Coil Winding
Curing Press and Curing Mold
Complex Potentials
H = −gradΦm = −∂Φm
∂xex −
∂Φm
∂yey
B = curlAz =∂Az
∂yex −
∂Az
∂xey
Cauchy-Riemann DEQ
∂Az
∂y= −µ0
∂Φm
∂x∂Az
∂x= µ0
∂Φm
∂y
W (z) = Az(x , y) + iµ0Φm(x , y) z = x + iy
−dWdz
= −∂Az
∂x− iµ0
∂Φm
∂x= By(x , y) + iBx(x , y)
Cartesian Field Components
W (z) = Az(x , y) + iµ0Φm(x , y) z = x + iy
By + iBx =∞∑
n=1
(Bn + iAn)(z0
r0)n−1 = −
µ0I2π
∞∑n=1
zn−10zn |z0| < |z|
Ideal (Iron) Pole Shapes
Feed down
∞∑n=1
cn
(zr0
)n−1
=∞∑
n=1
c′n
(z ′
r0
)n−1
= By + i Bx
z = z ′ + ∆z z = x + iy
c′n =
∞∑k=n
ck(k − 1)!
(k − n)! (n − 1)!
(∆zr0
)k−n
c′2 = c2 + 2c3
(∆zr0
)+ 3c4
(∆zr0
)2
+ …
• Measurement of magnetic axis in dipole by powering the coil as a quadrupole.
• The feed down effect can be used to center the measurements coilby minimization of the b10 which can only occur as feed down from b11.
• The dipole magnetic axis has to be well aligned with respect to the closed orbit: ± 0.1mm for both ∆x and ∆y systematic and 0.5mm for both σx and σy random (r.m.s.).
• Alignment tolerances of MCS and MCDO correctors w.r.t. MB: 0.3mm radially
Mechanical Axis Measurement for Spool Piece Alignment
Excitation Cycle of the LHC Dipoles
! " # $
" % $
" $
! & ' ( &
) )
Field Variation with Excitation
0 2000 4000 6000 8000 10000 12000
0.705
0.706
0.707
0.708
0.709
B0
I (A)
0 2000 4000 6000 8000 10000 12000
-6
-4
-2
0
2
4
6
b2
b3
b410
b510
I (A)
x 10-4
Saturation Effect in LHC Dipoles
1.002 208.2-
208.2 415.5-
415.5 622.7-
622.7 830.0-
830.0 1037.-
1037. 1244.-
1244. 1451.-
1451. 1659.-
1659. 1866.-
1866. 2073.-
2073. 2280.-
2280. 2488.-
2488. 2695.-
2695. 2902.-
2902. 3109.-
3109. 3317.-
3317. 3524.-
3524. 3731.-
3731. 3938.-
MUEr
1.002 208.2-
208.2 415.5-
415.5 622.7-
622.7 830.0-
830.0 1037.-
1037. 1244.-
1244. 1451.-
1451. 1659.-
1659. 1866.-
1866. 2073.-
2073. 2280.-
2280. 2488.-
2488. 2695.-
2695. 2902.-
2902. 3109.-
3109. 3317.-
3317. 3524.-
3524. 3731.-
3731. 3938.-
MUEr
Objectives for the ROXIE Development
Automatic generation of coil geometry
Field computation specially suited for magnet design (BEM-FEM)No meshing of the coil
No artificial boundary conditionsConfine numerical errors to the iron magnetization
Higher-order quadrilateral finite-elementsParametric mesh generator
Mathematical optimization
CAD/CAM interfaces
Field Computation with the BEM-FEM Coupling Method
IS
BS,i
Ω1
AΓ1 AΓ2
BIRONR1
BS,i
BIRONR2
BS,i
Ω2
BEM-domain
FEM-domains
Ω3
Bi
Field Quality Calculations for Collared Coils
-0.23 -0.21-
-0.21 -0.18-
-0.18 -0.16-
-0.16 -0.13-
-0.13 -0.11-
-0.11 -0.87-
-0.87 -0.62-
-0.62 -0.37-
-0.37 -0.12-
-0.12 0.012-
0.012 0.037-
0.037 0.062-
0.062 0.087-
0.087 0.111-
0.111 0.136-
0.136 0.161-
0.161 0.186-
0.186 0.211-
0.211 0.236-
A (Tm)
b2 = −0.239 b3 = 2.742 b4 = −0.012 b5 = −0.733
Preparation and Measurement of Collared Coils at BNN, Germany
Calculation of Fringe Fields in a LHC Dipole Model
y
x
z
Source field Reduced field Total field
-200 -160 -120 -80 -40 0 40 80 120 160 200
-6
-4
-2
0
2
4
6
8
Bx
By
Bz
|B|
T
mm
-200 -160 -120 -80 -40 0 40 80 120 160 200
-2
-1.5
-1
-0.5
0
0.5
1
1.5
2
Bx
By
Bz
|B|
T
mm
-200 -160 -120 -80 -40 0 40 80 120 160 200
-6
-4
-2
0
2
4
6
8
Bx
By
Bz
|B|
T
mm
Hysteresis in Superconductor Magnetization
-0.06
-0.04
-0.02
0.00
0.02
0.04
0.06
-1.6 -1.2 -0.8 -0.4 0.0 0.4 0.8 1.2 1.6Β [Τ]
µ 0 Μ
[Τ]
strand measurement
strand magnetization
filament magnetization
initial state curve
Field and Magnetization in the LHC Dipole Coil
0.024 0.100-
0.100 0.176-
0.176 0.252-
0.252 0.328-
0.328 0.403-
0.403 0.479-
0.479 0.555-
0.555 0.631-
0.631 0.707-
0.707 0.783-
0.783 0.859-
0.859 0.934-
0.934 1.010-
1.010 1.086-
1.086 1.162-
1.162 1.238-
1.238 1.314-
1.314 1.390-
1.390 1.466-
|B| (T)
-26.1 -25.0-
-25.0 -24.0-
-24.0 -22.9-
-22.9 -21.9-
-21.9 -20.8-
-20.8 -19.7-
-19.7 -18.7-
-18.7 -17.6-
-17.6 -16.5-
-16.5 -15.5-
-15.5 -14.4-
-14.4 -13.3-
-13.3 -12.3-
-12.3 -11.2-
-11.2 -10.1-
-10.1 -9.12-
-9.12 -8.05-
-8.05 -6.99-
-6.99 -5.93-
(*E3)
M (A/m)
Generated B3 Field Errors
Bn(r0) = −µ0Ii2π
r n−10r ni
cos nΘ
Bn(r0) =µ0
2πr n−10
r n+1i
n(mr ′ sin nθ + mθ cos nθ)
-0.20 -0.18-
-0.18 -0.16-
-0.16 -0.14-
-0.14 -0.12-
-0.12 -0.99-
-0.99 -0.77-
-0.77 -0.55-
-0.55 -0.34-
-0.34 -0.12-
-0.12 0.009-
0.009 0.030-
0.030 0.052-
0.052 0.074-
0.074 0.095-
0.095 0.117-
0.117 0.139-
0.139 0.161-
0.161 0.182-
0.182 0.204-
(*E-3)
B3 Contr. of Istrand (T)
-0.83 -0.75-
-0.75 -0.67-
-0.67 -0.59-
-0.59 -0.51-
-0.51 -0.43-
-0.43 -0.35-
-0.35 -0.28-
-0.28 -0.20-
-0.20 -0.12-
-0.12 -0.43-
-0.43 0.003-
0.003 0.011-
0.011 0.019-
0.019 0.027-
0.027 0.035-
0.035 0.043-
0.043 0.050-
0.050 0.058-
0.058 0.066-
(*E-3)
B3 Contr. of Mstrand (T)
Macro-Photography of Cable and Strand
Inner (outer) layer LHC dipole coil:Filament diameter 7 (6) µm, Strand diameter 1.065 (0.825) mm
Warning 4:
Scaling Laws for Multipoles are Wrong in 3 Dimensions
Bn(r1) = (r1
r0)n−1Bn(r0) bn(r1) = (
r1
r0)n−Nbn(r0)
0 20 40 60 80 100 120 140 160 180 200
-80
-60
-40
-20
0
20
40
60
80
b3
b3 (scaled, wrong)
Scaling Laws Hold for Integrated Multipoles
∇ 2Φm(x , y , z) =∂2Φm(x , y , z)
∂x2 +∂2Φm(x , y , z)
∂y2 +∂2Φm(x , y , z)
∂z2 = 0
Φm(x , y) =∫ z0
−z0
Φm(x , y , z)dz
∇ 2Φm(x , y) =∂2Φm(x , y)
∂x2 +∂2Φm(x , y)
∂y2 = 0
Sufficient condition: Integration path is extended far enough away from (into) themagnet so that the axial component of the field has dropped to zero.
∂2Φm
∂x2 +∂2Φm
∂y2 =∫ z0
−z0
(∂2Φm
∂x2 +∂2Φm
∂y2
)dz =
∫ z0
−z0
(−
∂2Φm
∂z2
)dz = −
∂Φm
∂z
∣∣∣∣z0
−z0
= Hz|−z0 − Hz|z0
References
[1] M. Aleksa, S. Russenschuck and C. Vollinger Magnetic Field Calculations Including the Impact of Persistent Currents inSuperconducting Filaments IEEE Trans. on Magn., vol. 38, no. 2, 2002.
[2] Bossavit, A.: Computational Electromagnetism, Academic Press, 1998
[3] Beth, R. A.: An Integral Formula for Two-dimensional Fields, Journal of Applied Physics, Vol. 38, Nr. 12, 1967
[4] Binns, K.J., Lawrenson, P.J., Trowbridge, C.W.: The analytical and numerical solution of electric and magnetic fields,John Wiley & Sons, 1992
[5] Bryant P.J.: Basic theory of magnetic measurements, CAS, CERN Accelerator School on Magnetic Measurement andAlignment, CERN 92-05, Geneva, 1992
[6] CAS, CERN Accelerator School on Superconductivity in Particle Accelerators, Haus Rissen, Hamburg, Germany, 1995,Proceedings, CERN-96-03
[7] Kurz, S., Russenschuck, S.: The application of the BEM-FEM coupling method for the accurate calculation of fields insuperconducting magnets, Electrical Engineering, 1999
[8] Mess, K.H., Schmuser, P., Wolff S.: Superconducting Accelerator Magnets, World Scientific, 1996
[9] M. Pekeler et al., Coupled Persistent-Current Effects in the Hera Dipoles and Beam Pipe Correction Coils, Desy Reportno. 92-06, Hamburg, 1992
[10] Russenschuck, S.: ROXIE: Routine for the Optimization of magnet X-sections, Inverse field calculation and coil Enddesign, Proceedings of the First International ROXIE users meeting and workshop, CERN 99-01, ISBN 92-9083-140-5.
[11] Wilson, M.N.: Superconducting Magnets, Oxford Science Publications, 1983