Accelerator Magnets Luca Bottura CERN Division LHC, CH-1211 Geneva 23, Switzerland

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Presentation transcript:

Accelerator Magnets Luca Bottura CERN Division LHC, CH-1211 Geneva 23, Switzerland

What you will learn today  SC accelerator magnet design  Complex field representation in 2-D  Multipoles and symmetries  Elements of magnetic design  SC accelerator magnet construction  Coil winding and assembly, structures  LHC dipole  Field errors in SC accelerator magnets  Linear and non linear contributions  SC cable magnetization effects  Interaction with current distribution

Accelerators  What for ?  a microscope for nuclear physics  X-ray source (lithography, spectrography, …)  cancer therapy  isotopes transmutation  Operation modes  fixed target  collider

Evolution  Livingston plot: particle energy in laboratory frame vs. commissioning year  steady increase  main jumps happen through technology development

Why high energy ?  Shorter wavelength  Increase resolution  Higher mass  New particles  Explore early universe time, corresponding to high energy states

Linear accelerators  Sequence of  accelerating stations (cavities), and  focussing elements (quadrupoles)  E and C proportional to length accelerated beam

Circular accelerators  Sequence of  accelerating stations (cavities),  bending and focussing elements (magnets)

Energy limits  Bending radius:  Example : a 1 TeV (E=1000 GeV) proton (q=1) is bent by a 5 T field on a radius  = 667 m  Synchrotron radiation:  Example : a proton (m = 1840) with 1 TeV (E=1000 GeV) bent on  = 667 m, looses  E = keV per turn

Cost considerations  Total cost:  C 1 – civil engineering, proportional to length  C 2 – magnetic system, proportional to length and field strength  C 3 – installed power, proportional to the energy loss per turn

CERN accelerator complex

Accelerator operation energy ramp preparation and access beam dump injection phase injection pre- injection I  t 2 I  e t I  t coast

Bending Uniform field (dipole) ideal real

Focussing Gradient field (quadrupole) focussing de-focussing

FODO cell  Sequence of:  focussing (F) – bending (O) – defocussing (D) – bending (O) magnets  additional correctors (see LHC example) MB_lattice dipoleMQlattice quadrupole MSCBlattice sextupole+orbit correctorMOlattice octupole MQTtrim quadrupoleMQSskew trim quadrupole MCDOspool-piece decapole-octupole MCSspool-piece sextupole

Magnetic field  2-D field (slender magnet), with components only in x and y and no component along z  Ignore z and define the complex plane s = x + i y  Complex field function:  B is analytic in s  Cauchy-Riemann conditions:

Field expansion  B is analytic and can be expanded in Taylor series (the series converges) inside a current- free disk  Magnetic field expansion:  Multipole coefficients:

Multipole magnets B1B1 A1A1 B2B2 A2A2

Normalised coefficients  C n : absolute, complex multipoles, in R ref  c n : relative multipoles, in R ref  High-order multipoles are generally small, 100 ppm and less of the main field

Current line  Field and harmonics of a current line I located at R = x + iy  Field:  Multipoles:

Magnetic moment  Field and harmonics of a moment m = m y + m x located at R = x + iy  Field:  Multipoles:

Effect of an iron yoke - I  Current line  Image current:

Effect of an iron yoke - m  Magnetic moment  Image moment:

Magnetic design - 1  Field of a cos(p  ) distribution  Field:  Multipoles:

Magnetic design - 2  Field of intersecting circles (and ellipses)  uniform field:

Magnetic design - 3  Intersecting ellipses to generate a quadrupole  uniform gradient:

Magnetic design - 4  Approximation for the ideal dipole current distribution… Rutherford cable

Magnetic design - 5  … and for the ideal quadrupole current distribution… Rutherford cable

Magnetic design - 6  Uniform current shells dipolequadrupole

Tevatron dipole 2 current shells (layers) pole midplane

HERA dipole wedge 2 layers

LHC dipole

LHC quadrupole

Winding in blocks B B

Allowed harmonics  Technical current distribution can be considered as a series approximation: =++… B = B 1 + B 3 + …

Symmetries  Dipole symmetry:  Rotate by  and change sign to the current – the dipole is the same  Quadrupole symmetry:  Rotate by  /2 and change sign to the current – the quadrupole is the same  Symmetry for a magnet of order m:  Rotate by  /m and change sign to the current – the magnet is the same

Allowed multipoles  A magnet of order m can only contain the following multipoles (n, k, m integer) n = (2 k + 1 ) m  Dipole m=1, n={1,3,5,7,…}: dipole, sextupole, decapole …  Quadrupole m=2, n={2,6,10,…}: quadrupole, dodecapole, 20-pole …  Sextupole m=3, n={3,9,15,…}: sextupole, 18-pole …

Dipole magnet principle

Dipole magnet designs 4 T, 90 mm 4.7 T, 75 mm 6.8 T, 50 mm 3.4 T, 80 mm

LHC dipole

LHC dipole design 8.3 T, 56 mm

Superconducting coil B B

Rutherford cable superconducting cable SC strand SC filament

Collars 175 tons/m 85 tons/m F

Iron yoke flux lines gap between coil and yoke heat exchanger saturation control bus-bar

Coil ends B

Cryostated magnet

Ideal transfer function  For linear materials (  =const), no movements (R=const), no eddy currents (dB/dt=0)  Define a transfer function: … ;;

Transfer function geometric (linear) contribution T = T/kA persistent currents  T = -0.6 mT/kA (0.1 %) saturation  T = -6 mT/kA (1 %)

Saturation of the field saturated region (B > 2 T) effective iron boundary moves away from the coil: less field

Normal sextupole partial compensation of persistent currents at injection

Persistent currents BB +J c -J c M DC  Field change  B  Eddy currents J c with  =   persistent  Diamagnetic moment at each filament: M DC  J c *Dfil  J c (B,T)  M DC (  B,B,T)

Persistent currents hysteresis crossing: no overshoot possible, operation of correctors !

Persistent currents a +0.1 K temperature increase gives a units change on b3 (1.7 units/K)

Coupling currents  dB/dt resistive contact at cross-overs R c  Field ramp dB/dt  Eddy currents I eddy I eddy  dB/dt

Coupling current effects allowed and non-allowed multipoles !

Decay and Snap-back snap-back decay LHC operation cycle

Decay and snap-back Snap-back at the start of the acceleration ramp decay during injection

Decay decay during simulated 10,000 s injection exponential fit  i = 900 s

Snap-back snap-back fit:  b 3 [1-(I-I inj )/  I] 3  b3= 3.7units  I = 27A   B = 19 mT snap-back decay

Decay and SB physics  Current distribution is not uniform in the cables  joints  supercurrents  I/Ic  Current distribution changes in time, causing a variable rotating field...

Decay and SB physics … the local field change in turn affects the magnetization of the SC filaments: average M decreases (decay) net decrease of magnetization

Decay and SB physics  The magnetization state is re- established as soon as the background field is increased (snap-back)  The background field change necessary is of the same order of the internal field change in the cable   100 A change in current imbalance   10 mT average internal field change (vs. 5…20 mT measured)

A demonstration B measured computed Copper strands NbTi strand Demonstration experiment at Twente University. Courtesy of M. Haverkamp

A bit of reality…  Field quality reconstructed from measurements performed in MBP2N1  Plot of homogeneity |B(x,y)-B 1 |/B 1 inside the aperture of the magnet:  blue  OK (1  )  green  so, so (5  )  yellow  Houston, we have a problem (1  )  red  bye, bye (5  )

… the measurement

Sony Playstation III (or Tracking the LHC...) coil of MBP2N1 operating currentField homogeneity reconstructed from measurements Rref = 17 mm