Magnetic Multipoles, Magnet Design Alex Bogacz, Geoff Krafft and Timofey Zolkin

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Magnetic Multipoles,
Magnet Design
Alex Bogacz, Geoff Krafft and Timofey Zolkin
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 1
Maxwell’s Equations for Magnets - Outline
Solutions to Maxwell’s equations for magnetostatic fields:
in two dimensions (multipole fields)
in three dimensions (fringe fields, end effects, insertion devices...)
How to construct multipole fields in two dimensions, using
electric currents and magnetic materials, considering
idealized situations.
A. Wolski, University of Liverpool and the Cockcroft Institute, CAS
Specialised Course on Magnets, 2009,
http://cas.web.cern.ch/cas/Belgium-2009/Lectures/PDFs/Wolski-1.pdf
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Basis
Vector calculus in Cartesian and polar coordinate systems;
Stokes’ and Gauss’ theorems
Maxwell’s equations and their physical significance
Types of magnets commonly used in accelerators.
following notation used in: A. Chao and M. Tigner, “Handbook of
Accelerator Physics and Engineering,” World Scientific (1999).
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
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3
Maxwell’s equations
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 4
Maxwell’s equations
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 5
Physical interpretation of
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 6
Physical interpretation of
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
7
Linearity and superposition
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 8
Multipole fields
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
9
Multipole fields
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 10
Multipole fields
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 11
Multipole fields
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 12
Multipole fields
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 13
Multipole fields
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013 14
Generating multipole fields from a current
distribution
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
15
Multipole fields from a current distribution
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
16
Multipole fields from a current distribution
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
17
Multipole fields from a current distribution
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
18
Multipole fields from a current distribution
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
19
Multipole fields from a current distribution
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields from a current distribution
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields from a current distribution
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields from a current distribution
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields from a current distribution
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields from a current distribution
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Lecture 5 - Magnetic Multipoles
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Superconducting quadrupole - collider final focus
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Multipole fields in an iron-core magnet
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Multipole fields in an iron-core magnet
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields in an iron-core magnet
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
29
Multipole fields in an iron-core magnet
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields in an iron-core magnet
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields in an iron-core magnet
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields in an iron-core magnet
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields in an iron-core magnet
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields in an iron-core magnet
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields in an iron-core magnet
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic MultipolesUSPAS, Fort Collins, CO, June 10-21, 2013
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Multipole fields in an iron-core magnet
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
37
Generating multipole fields in an iron-core magnet
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
38
Generating multipole fields in an iron-core magnet
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
39
Generating multipole fields in an iron-core magnet
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
40
Generating multipole fields in an iron-core magnet
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
41
Maxwell’s Equations for Magnets - Summary
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Lecture 5 - Magnetic Multipoles USPAS, Fort Collins, CO, June 10-21, 2013
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Multipoles in Magnets - Outline
Deduce that the symmetry of a magnet imposes constraints
on the possible multipole field components, even if we relax
the constraints on the material properties and other
geometrical properties;
Consider different techniques for deriving the multipole field
components from measurements of the fields within a
magnet;
Discuss the solutions to Maxwell’s equations that may be
used for describing fields in three dimensions.
Thomas Jefferson National Accelerator Facility
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Previous lecture re-cap
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
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Previous lecture re-cap
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Lecture 5 - Magnetic Multipoles
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Allowed and forbidden harmonics
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Lecture 5 - Magnetic Multipoles
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Allowed and forbidden harmonics
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Lecture 5 - Magnetic Multipoles
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Allowed and forbidden harmonics
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Lecture 5 - Magnetic Multipoles
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Allowed and forbidden harmonics
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Lecture 5 - Magnetic Multipoles
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49
Allowed and forbidden harmonics
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
50
Allowed and forbidden harmonics
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Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
51
Measuring multipoles
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Measuring multipoles in Cartesian basis
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Measuring multipoles in Cartesian basis
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Measuring multipoles in Polar basis
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Measuring multipoles in Polar basis
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Measuring multipoles in Polar basis
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Advantages of mode decompositions
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Three-dimensional fields
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Lecture 5 - Magnetic Multipoles USPAS, Fort Collins, CO, June 10-21, 2013
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Three-dimensional fields
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Lecture 5 - Magnetic Multipoles
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Three-dimensional fields
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Lecture 5 - Magnetic Multipoles
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Three-dimensional fields
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Lecture 5 - Magnetic Multipoles
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Three-dimensional fields
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Lecture 5 - Magnetic Multipoles
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Summary – Part II
Symmetries in multipole magnets restrict the multipole components that can be
present in the field.
It is useful to be able to find the multipole components in a given field from
numerical field data: but this must be done carefully, if the results are to be
accurate.
Usually, it is advisable to calculate multipole components using field data on a
surface enclosing the region of interest: any errors or residuals will decrease
exponentially within that region, away from the boundary. Outside the
boundary, residuals will increase exponentially.
Techniques for finding multipole components in two dimensional fields can be
generalized to three dimensions, allowing analysis of fringe fields and insertion
devices.
In two or three dimensions, it is possible to use a Cartesian basis for the field
modes; but a polar basis is sometimes more convenient.
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Appendix A - Field Error Tolerances
Focusing ‘point’ error perturbs the betatron motion leading to the Courant-Snyder invariant
change:
Beam envelope and beta-function oscillate at double the betatron frequency
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Appendix A - Field Error Tolerances
Single point mismatch as measured by the Courant-Snyder invariant change:
    (   ) 2  2 (   ) x   x 2
   2     x     2
x   sin ,  
,

sin   cos  -  sin  

Each source of field error (magnet) contributes the following Courant-Snyder
variation
  2  cos   
2
B
  
,
grad
dl
B
  m x m ,wherem    kmdl
m 1
here, m =1 quadrupole, m =2 sextupole, m=3 octupole, etc
  2  
m 1



m

m cos sin     
 m1
m



m
2

m sin   ,

m
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Appendix A - Field Error Tolerances
multipole expansion coefficients of the azimuthal magnetic field, B - Fourier series
representation in polar coordinates at a given point along the trajectory):
r
B  r ,      
m  2  r0 
m -1
 Bm cos m  Am sin m 
multipole gradient and integrated geometric gradient:
Gm =
1
r0
m
Bm 1  kGauss cm - m 
kn 
Gn
cm- ( n 1) 
B
n
G dl


n
B
cm- n 
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Appendix A - Field Error Tolerances
Cumulative mismatch along the lattice (N sources):

 N    1  2 

m 1
n 1 
N



m -1
m cos sin m 

  2  
 m1



m -1

m sin m  

2

 ,


Standard deviation of the Courant-Snyder invariant is given by:



 2 -  2

2

   2i 
i 1 
m 1

N

i

m -1
m  cos sin 
m

 i   
 m1
2

i

m -1

m sin  

2
m



Assuming weakly focusing lattice (uniform beta modulation) the following averaging
(over the betatron phase) can by applied:
2
... 
1
2

d ...
0
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Appendix A - Field Error Tolerances
Some useful integrals …. :
cos sin m   0 ,
m -1
sin m  
sin m - 2  
m
0m odd
 m - 1!!m even
m !!
will reduce the coherent contribution to the C-S variance as follows:




 2i 

i 1 
m 1

N

i

m -1
m  cos sin 
m

 i   
 m1
2

i

m -1

m sin  

2
m



Including the first five multipoles yields:



 
N
i 1
2
i





2
12 sin 2   i 2 2  213 sin 4   i  32  215  224 sin 6   ...


1
2
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2 4
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2 4 6
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Appendix A - Field Error Tolerances
Beam radius at a given magnet is :
ai 
1
 i
2
One can define a ‘good fileld radius’ for a given type of magnet as: a  Max(ai )
Assuming the same multipole content for all magnets in the class one gets:



N
1
2
i 1
2
i




3
5
 12  a 2 2 2  213  a 4 32  215  224  ...
2
2
The first factor purely depends on the beamline optics (focusing), while the second one
describes field tolerance (nonlinearities) of the magnets:




3
5
  12  a 2 2 2  213  a 4 32  215  224  ...
2
2
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Appendix B - The vector potential
A scalar potential description of the magnetic field has been very useful to
derive the shape for the pole face of a multipole magnet.
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Appendix B - The vector potential
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Appendix B - The vector potential
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Appendix B - The vector potential
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Appendix B - The vector potential
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Appendix B - The vector potential
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Appendix B - The vector potential
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Appendix B - The vector potential
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Appendix B - The vector potential
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Appendix B - The vector potential
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
80
Appendix B - The vector potential
Thomas Jefferson National Accelerator Facility
Operated by JSA for the U.S. Department of Energy
Lecture 5 - Magnetic Multipoles
USPAS, Fort Collins, CO, June 10-21, 2013
81
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