Eddy Current Septum Magnet Optimization Powering Options of SMH42 - - PowerPoint PPT Presentation

eddy current septum magnet optimization
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Eddy Current Septum Magnet Optimization Powering Options of SMH42 - - PowerPoint PPT Presentation

Eddy Current Septum Magnet Optimization Powering Options of SMH42 and the Influence of the Septum Thickness on the Fringe Field Zsolt SZOKE (TE/ABT/SE) Outline Eddy Current Septa Magnets Our Goal Baseline Design Performance


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SLIDE 1

Eddy Current Septum Magnet Optimization

Powering Options of SMH42 and the Influence of the Septum Thickness on the Fringe Field

Zsolt SZOKE (TE/ABT/SE)

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SLIDE 2

Outline

  • Eddy Current Septa Magnets
  • Our Goal
  • Baseline Design Performance
  • Analysis in Time Domain
  • Comparing Full Sine and Half Sine Excitation
  • Comparing 5mm and 3mm Septum Blades
  • Comparing 2ms and 7ms Wavelength

19/08/2014 LIU-PS Meeting 2

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SLIDE 3

Eddy Current Septa Magnets

  • Different types of septa:

– direct drive (DC, pulsed) – eddy current (only pulsed)

  • Eddy current type - advantages:

– coil dimensions are not critical – the pulsed coil has such a magnetic field which induces eddy currents in the septum counteracting the fringe field – septum can be very thin

19/08/2014 LIU-PS Meeting 3

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SLIDE 4

Our Goal

  • Optimize different eddy current septum

magnet parameters.

  • 3 comparisons made with the baseline design.
  • Baseline: 2ms, full sine, 5mm septum.
  • Examination of the fringe field: By and ∫Bydl.

19/08/2014 LIU-PS Meeting 4

7ms half sine 3mm septum

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SLIDE 5

Baseline Design Performance

  • ʃBy,gapdlmax = 502.67Tmm
  • By,gap,max = 542mT
  • ʃBy,fringedlmax = -1.37Tmm (after the current pulse)
  • By,fringe,max = -1.4mT (after the current pulse)
  • Idriving,max = 30251A
  • Gap fringe

field shape:

19/08/2014 LIU-PS Meeting 5

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SLIDE 6

Analysis in Time Domain (1/2)

  • Opera finite element simulation, spanning 3×

the excitation time

  • Discrete moments  interpolation in MATLAB
  • 2 types of interpolation:

– PCHIP: for plotting – SPLINE: for peak determination

19/08/2014 LIU-PS Meeting 6

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SLIDE 7

Analysis in Time Domain (2/2)

  • 6 values for each simulated moment:

– t [ms] – I [kA] – By (gap) – ∫Bydl (gap) – By (fringe) – ∫Bydl (fringe)

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“gap”: the middle of the aperture “fringe”: 5mm from the septum

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SLIDE 8

Comparing By of Full Sine and Half Sine

  • Fringe field extents

after excitation.

  • Full sine:

By = -1.4mT

  • Half sine:

By = 15mT

19/08/2014 LIU-PS Meeting 8

1 2 3 4 5 6

  • 40
  • 30
  • 20
  • 10

10 20 30 40 Current [kA] Time [ms] 1 2 3 4 5 6

  • 2

2 4 6 8 10 12 14 x 10

  • 3

Magnetic flux density [T] 1 2 3 4 5 6 20 40 Current [kA] Time [ms] 1 2 3 4 5 6 0.01 0.02 Magnetic flux density [T]

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SLIDE 9

Comparing ʃBydl of Full Sine and Half Sine

  • Integrated fringe

field extents after excitation.

  • Full sine:

∫Bydl = -1.37Tmm

  • Half sine:

∫Bydl = 14.28Tmm

19/08/2014 LIU-PS Meeting 9

1 2 3 4 5 6

  • 50

50 Current [kA] Time [ms] 1 2 3 4 5 6

  • 20

20 Field integral [Tmm] 1 2 3 4 5 6 20 40 Current [kA] Time [ms] 1 2 3 4 5 6 10 20 Field integral [Tmm]

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SLIDE 10

Comparing Full Sine and Half Sine

  • Huge time constants in both cases:

– 1 or 2ms excitation time (half or full sine) – time constant: >4ms

  • Fringe field peak values are 10.4-10.7 times

lower using full sine wave instead of half sine.

  • Using ‘direct damping’ of the fringe field (full

sine excitation) proves to be very effective.

19/08/2014 LIU-PS Meeting 10

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SLIDE 11

Comparing By of 5mm and 3mm Septa

  • Fringe field extents

after excitation.

  • 5mm septum blade:

By = -1.4mT

  • 3mm septum blade:

By = -3.6mT

19/08/2014 LIU-PS Meeting 11

1 2 3 4 5 6

  • 40
  • 30
  • 20
  • 10

10 20 30 40 Current [kA] Time [ms] 1 2 3 4 5 6

  • 2

2 4 6 8 10 12 14 x 10

  • 3

Magnetic flux density [T] 1 2 3 4 5 6

  • 40
  • 20

20 40 Current [kA] Time [ms] 1 2 3 4 5 6

  • 0.01

0.01 0.02 0.03 Magnetic flux density [T]

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SLIDE 12

Comparing ʃBydl of 5mm and 3mm Septa

  • Integrated fringe

field extents after excitation.

  • 5mm septum blade :

∫Bydl = -1.37Tmm

  • 3mm septum blade :

∫Bydl = -3.51Tmm

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1 2 3 4 5 6

  • 50

50 Current [kA] Time [ms] 1 2 3 4 5 6

  • 20

20 Field integral [Tmm] 1 2 3 4 5 6

  • 40
  • 20

20 40 Current [kA] Time [ms] 1 2 3 4 5 6

  • 10

10 20 30 Field integral [Tmm]

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SLIDE 13

Comparing 5mm and 3mm Septa

  • A thinner septum blade is advantageous for the

beam: lower continuous losses.

  • 3 mm septum blade has higher current density.
  • Fringe field peak values are 1.7-2.6 times lower

using 5mm septum instead of 3mm.

19/08/2014 LIU-PS Meeting 13

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SLIDE 14

Comparing By of 2ms and 7ms Wavelength

  • Fringe field extents

after excitation.

  • 2ms wavelength:

By = -1.4mT

  • 7ms wavelength:

By = -15.6mT

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1 2 3 4 5 6

  • 40
  • 30
  • 20
  • 10

10 20 30 40 Current [kA] Time [ms] 1 2 3 4 5 6

  • 2

2 4 6 8 10 12 14 x 10

  • 3

Magnetic flux density [T] 5 10 15 20 25

  • 40
  • 20

20 40 Current [kA] Time [ms] 5 10 15 20 25

  • 0.02

0.02 0.04 0.06 Magnetic flux density [T]

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SLIDE 15

Comparing ʃBydl of 2ms and 7ms Wavelength

  • Integrated fringe

field extents after excitation.

  • 2ms wavelength :

∫Bydl = -1.37Tmm

  • 7ms wavelength :

∫Bydl = -15.14Tmm

19/08/2014 LIU-PS Meeting 15

1 2 3 4 5 6

  • 50

50 Current [kA] Time [ms] 1 2 3 4 5 6

  • 20

20 Field integral [Tmm] 5 10 15 20 25

  • 40
  • 20

20 40 Current [kA] Time [ms] 5 10 15 20 25

  • 20

20 40 60 Field integral [Tmm]

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SLIDE 16

Comparing 2ms Wavelength and 7ms

  • 3.5 ms pulse half sine shape would be a pulse

length similar to present SMH42.

  • Shorter pulse length (w.r.t. baseline design)

wasn’t investigated, since it will be very difficult to build a compatible magnet.

  • Fringe field peak values are 3.2-11.1 times

lower using 2ms full sine wave instead of 7ms.

19/08/2014 LIU-PS Meeting 16

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SLIDE 17

Final Conclusion

Full sine vs. Half sine

Direct fringe field cancellation very effective

5mm septum vs. 3mm septum

The thicker the septum, the lower the fringe field

2ms wavelength vs. 7ms wavelength

The shorter the pulse, the lower the fringe field

The base line design appears a good compromise. Next: the BMP42 septum bumper analysis.

19/08/2014 LIU-PS Meeting 17

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SLIDE 18

References

  • Full documentation: Z. Szoke: Eddy Current Septa Magnet

Optimization

  • M. J. Barnes, J. Borburgh, B. Goddard, M. Hourican, in Proceedings
  • f the CAS-CERN Accelerator School: Magnets, Bruges, Belgium, 16-

25 June 2009, edited by D. Brandt, CERN-2010-004, pp. 167-184

  • Finite element simulations: Cobham Opera 16
  • Data processing: MATLAB R2013b

19/08/2014 LIU-PS Meeting 18

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SLIDE 19

Thank You for Your Attention! Q&A

19/08/2014 LIU-PS Meeting 19