Multipole magnet

Multipole magnets are magnets built from multiple individual magnets, typically used to control beams of charged particles. Each type of magnet serves a particular purpose.

  • Dipole magnets are used to bend the trajectory of particles
  • Quadrupole magnets are used to focus particle beams
  • Sextupole magnets are used to correct for chromaticity introduced by quadrupole magnets[1]

Magnetic field equations

The magnetic field of an ideal multipole magnet in an accelerator is typically modeled as having no (or a constant) component parallel to the nominal beam direction ( z {\displaystyle z} direction) and the transverse components can be written as complex numbers:[2]

B x + i B y = C n ( x i y ) n 1 {\displaystyle B_{x}+iB_{y}=C_{n}\cdot (x-iy)^{n-1}}

where x {\displaystyle x} and y {\displaystyle y} are the coordinates in the plane transverse to the nominal beam direction. C n {\displaystyle C_{n}} is a complex number specifying the orientation and strength of the magnetic field. B x {\displaystyle B_{x}} and B y {\displaystyle B_{y}} are the components of the magnetic field in the corresponding directions. Fields with a real C n {\displaystyle C_{n}} are called 'normal' while fields with C n {\displaystyle C_{n}} purely imaginary are called 'skewed'.

First few multipole fields
n name magnetic field lines example device
1 dipole
2 quadrupole
3 sextupole

Stored energy equation

For an electromagnet with a cylindrical bore, producing a pure multipole field of order n {\displaystyle n} , the stored magnetic energy is:

U n = n ! 2 2 n π μ 0 N 2 I 2 . {\displaystyle U_{n}={\frac {n!^{2}}{2n}}\pi \mu _{0}\ell N^{2}I^{2}.}

Here, μ 0 {\displaystyle \mu _{0}} is the permeability of free space, {\displaystyle \ell } is the effective length of the magnet (the length of the magnet, including the fringing fields), N {\displaystyle N} is the number of turns in one of the coils (such that the entire device has 2 n N {\displaystyle 2nN} turns), and I {\displaystyle I} is the current flowing in the coils. Formulating the energy in terms of N I {\displaystyle NI} can be useful, since the magnitude of the field and the bore radius do not need to be measured.

Note that for a non-electromagnet, this equation still holds if the magnetic excitation can be expressed in Amperes.

Derivation

The equation for stored energy in an arbitrary magnetic field is:[3]

U = 1 2 ( B 2 μ 0 ) d τ . {\displaystyle U={\frac {1}{2}}\int \left({\frac {B^{2}}{\mu _{0}}}\right)\,d\tau .}

Here, μ 0 {\displaystyle \mu _{0}} is the permeability of free space, B {\displaystyle B} is the magnitude of the field, and d τ {\displaystyle d\tau } is an infinitesimal element of volume. Now for an electromagnet with a cylindrical bore of radius R {\displaystyle R} , producing a pure multipole field of order n {\displaystyle n} , this integral becomes:

U n = 1 2 μ 0 0 R 0 2 π B 2 d τ . {\displaystyle U_{n}={\frac {1}{2\mu _{0}}}\int ^{\ell }\int _{0}^{R}\int _{0}^{2\pi }B^{2}\,d\tau .}


Ampere's Law for multipole electromagnets gives the field within the bore as:[4]

B ( r ) = n ! μ 0 N I R n r n 1 . {\displaystyle B(r)={\frac {n!\mu _{0}NI}{R^{n}}}r^{n-1}.}

Here, r {\displaystyle r} is the radial coordinate. It can be seen that along r {\displaystyle r} the field of a dipole is constant, the field of a quadrupole magnet is linearly increasing (i.e. has a constant gradient), and the field of a sextupole magnet is parabolically increasing (i.e. has a constant second derivative). Substituting this equation into the previous equation for U n {\displaystyle U_{n}} gives:

U n = 1 2 μ 0 0 R 0 2 π ( n ! μ 0 N I R n r n 1 ) 2 d τ , {\displaystyle U_{n}={\frac {1}{2\mu _{0}}}\int ^{\ell }\int _{0}^{R}\int _{0}^{2\pi }\left({\frac {n!\mu _{0}NI}{R^{n}}}r^{n-1}\right)^{2}\,d\tau ,}

U n = 1 2 μ 0 0 R ( n ! μ 0 N I R n r n 1 ) 2 ( 2 π r d r ) , {\displaystyle U_{n}={\frac {1}{2\mu _{0}}}\int _{0}^{R}\left({\frac {n!\mu _{0}NI}{R^{n}}}r^{n-1}\right)^{2}(2\pi \ell r\,dr),}

U n = π μ 0 n ! 2 N 2 I 2 R 2 n 0 R r 2 n 1 d r , {\displaystyle U_{n}={\frac {\pi \mu _{0}\ell n!^{2}N^{2}I^{2}}{R^{2n}}}\int _{0}^{R}r^{2n-1}\,dr,}

U n = π μ 0 n ! 2 N 2 I 2 R 2 n ( R 2 n 2 n ) , {\displaystyle U_{n}={\frac {\pi \mu _{0}\ell n!^{2}N^{2}I^{2}}{R^{2n}}}\left({\frac {R^{2n}}{2n}}\right),}

U n = n ! 2 2 n π μ 0 N 2 I 2 . {\displaystyle U_{n}={\frac {n!^{2}}{2n}}\pi \mu _{0}\ell N^{2}I^{2}.}

References

  1. ^ "Varna 2010 | the CERN Accelerator School" (PDF). Archived from the original (PDF) on 2017-05-13.
  2. ^ "Wolski, Maxwell's Equations for Magnets – CERN Accelerator School 2009".
  3. ^ Griffiths, David (2013). Introduction to Electromagnetism (4th ed.). Illinois: Pearson. p. 329.
  4. ^ Tanabe, Jack (2005). Iron Dominated Electromagnets - Design, Fabrication, Assembly and Measurements (4th ed.). Singapore: World Scientific.