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)
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
Zsolt SZOKE (TE/ABT/SE)
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“gap”: the middle of the aperture “fringe”: 5mm from the septum
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10 20 30 40 Current [kA] Time [ms] 1 2 3 4 5 6
2 4 6 8 10 12 14 x 10
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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50 Current [kA] Time [ms] 1 2 3 4 5 6
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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10 20 30 40 Current [kA] Time [ms] 1 2 3 4 5 6
2 4 6 8 10 12 14 x 10
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 0.03 Magnetic flux density [T]
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50 Current [kA] Time [ms] 1 2 3 4 5 6
20 Field integral [Tmm] 1 2 3 4 5 6
20 40 Current [kA] Time [ms] 1 2 3 4 5 6
10 20 30 Field integral [Tmm]
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10 20 30 40 Current [kA] Time [ms] 1 2 3 4 5 6
2 4 6 8 10 12 14 x 10
Magnetic flux density [T] 5 10 15 20 25
20 40 Current [kA] Time [ms] 5 10 15 20 25
0.02 0.04 0.06 Magnetic flux density [T]
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50 Current [kA] Time [ms] 1 2 3 4 5 6
20 Field integral [Tmm] 5 10 15 20 25
20 40 Current [kA] Time [ms] 5 10 15 20 25
20 40 60 Field integral [Tmm]
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Direct fringe field cancellation very effective
The thicker the septum, the lower the fringe field
The shorter the pulse, the lower the fringe field
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Optimization
25 June 2009, edited by D. Brandt, CERN-2010-004, pp. 167-184
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