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High Order Image Terms and Harmonic Closed Orbits at the ISIS Synchrotron Ben Pine With thanks to Dr Chris Warsop, ISIS Synchrotron Group and Operations Team ISIS, Rutherford Appleton Laboratory, UK Science and Technology Facilities Council


  1. High Order Image Terms and Harmonic Closed Orbits at the ISIS Synchrotron Ben Pine With thanks to Dr Chris Warsop, ISIS Synchrotron Group and Operations Team ISIS, Rutherford Appleton Laboratory, UK Science and Technology Facilities Council Space Charge Workshop, October 5, 2017

  2. Origin of the idea At ISIS, 3 rd , 4 th and 5 th harmonics of the closed orbit are corrected at highest intensities Rees and Prior 1 suggested this due to higher order image terms driven by the closed orbit Term they looked at quadrupole term proportional to square of closed orbit Suggested vertical closed orbit could excite horizontal resonance 1 GH Rees and CR Prior, Image Effects on Crossing an Integer Resonance, Particle Accelerators 1995, Vol 48. Ben Pine Space Charge Workshop Oct 5, 2017 2 / 29

  3. Origin of the idea (2) Idea examined again by Baartman 2 Expanded Laslett’s image term calculation to include more terms Suggested term Rees and Prior had looked at was an envelope resonance 2 R Baartman, Betatron Resonances with Space Charge, Proc. Workshop on High Intensity Hadron Rings, 1998 Ben Pine Space Charge Workshop Oct 5, 2017 3 / 29

  4. Overview ISIS facility Image terms from pencil beams in parallel plate geometry Numerical results from round beams in rectangular geometry Resonance theory for high order image terms Simulation results for beams with harmonic closed orbits Ben Pine Space Charge Workshop Oct 5, 2017 4 / 29

  5. ISIS ISIS is the spallation neutron source at RAL 50 Hz 800 MeV RCS H - injection at 70 MeV over ∼ 200 turns High intensity, up to 3 × 10 13 ppp accelerated Beam loss is the main limit to intensity Beam loss is controlled at low energy on collimators Ben Pine Space Charge Workshop Oct 5, 2017 5 / 29

  6. Beam loss Beam loss takes many forms e.g. longitudinal/transverse, injection/extraction My work focuses on losses resulting from transverse space charge In particular from image forces ISIS has a unique conformal vacuum vessel, which follows the profile of the design beam envelopes Limits the range over which the tunes can be changed Makes image forces much more complicated 100 80 80 Width � mm � Width � mm � 60 60 40 40 Horizontal Aperture Vertical Aperture 20 20 Horizontal Envelope Vertical Envelope 0 0 0 5 10 15 0 5 10 15 Length � m � Length � m � Ben Pine Space Charge Workshop Oct 5, 2017 6 / 29

  7. Image terms: Laslett and Baartman Solution for a potential of pencil beam between parallel plate boundary � � λ sin( π y / 2 h ) − sin( π ¯ y / 2 h ) � � U = − ln � . � � 2 πε 0 1 + cos( π ( y + ¯ y ) / 2 h )) � This leads to the usual Laslett coefficients of ǫ 1 = π 2 48 , and ξ 1 = π 2 16 λ E y ≃ − πε 0 h 2 ( ǫ 1 ˆ y + ξ 1 ¯ y ) . But if you expand the answer to obtain more terms: y 3 y 2 y 2 ¯ y 3 E yimage 1 � ˆ ¯ ¯ y ¯ ˆ ˆ ˆ � y y y = ǫ 1 h 2 + ξ 1 h 2 + κ 30 h 4 + κ 21 h 4 + κ 12 h 4 + κ 03 h 4 + ... 4 λ 4 πε 0 This expression was taken as starting point for numerical work on two dimensional round beams in rectangular apertures. Ben Pine Space Charge Workshop Oct 5, 2017 7 / 29

  8. 20 mm 40 mm Numerical results - off-centred beams Subset Whole beam results Section of beam results Ben Pine Space Charge Workshop Oct 5, 2017 8 / 29

  9. 20 mm 40 mm Numerical results - off-centred beams Subset Whole beam results Section of beam results Ben Pine Space Charge Workshop Oct 5, 2017 9 / 29

  10. Closed orbits at low and high intensity Starting with the equation for transverse betatron motion d 2 y dt 2 + ( Q Ω) 2 y = F y . γ m 0 Changing to the longitudinal coordinate from time and expressing F y as � ¯ v × ¯ � the Lorentz Force Law, F y = e E + ¯ B y , � Q � 2 d 2 y � ¯ 1 v × ¯ � ds 2 + y = E + ¯ y . B ρ 0 B 0 ρ 0 v s At low intensity the E term is zero. Considering just dipole errors, with a single kick ∆ B � Q � 2 d 2 y y = ∆ B ds 2 + . ρ 0 B 0 ρ 0 This equation is solved by the particular integral � β s ∆ B � y = cos Q θ 2 | sin π Q | B 0 ρ 0 Ben Pine Space Charge Workshop Oct 5, 2017 10 / 29

  11. Closed orbits at low and high intensity Simulations were with a single angular kick at the beginning of the second superperiod. Simulations were with a distributed angular kick to produce a 13 th harmonic closed orbit. Ben Pine Space Charge Workshop Oct 5, 2017 11 / 29

  12. Image driving terms The equation of motion with respect to the established closed orbit is y ′′ + ky = F D + F I The one dimensional single particle Hamiltonian can be written H ( y , P y , s ) = 1 y + 1 2 ky 2 + V D + V I 2 P 2 Writing the indirect space charge forces in Baartman’s general form y 2 y 3 � 1 λ y ¯ y y ¯ V I = ǫ 1 2 h 2 + ξ 1 h 2 + κ 30 h 4 + γ m 0 β 2 c 2 πε 0 y 2 ¯ y 2 y 3 ¯ y 4 � y κ 21 2 h 4 + κ 12 3 h 4 + κ 03 4 h 4 + . . . Ben Pine Space Charge Workshop Oct 5, 2017 12 / 29

  13. Hamiltonian including κ 12 κ 12 image term inserted into Hamiltonian as T 12 y 3 ¯ y where T 12 is constant absorbing κ 12 and other constant terms. Changing y to action-angle variables and substituting for ¯ y : � 3 � 2 J 2 sin 3 φ a n cos n θ + V 0 ( J ) H = ω J + T 12 ω V 0 ( J ) is non-linear term in J due to direct space charge and other image terms. � 3 � 2 J 2 � 3 H = ω J + a n T 12 8 (sin( φ − n θ ) + sin( φ + n θ )) ω − 1 � 8 (sin(3 φ − n θ ) + sin(3 φ + n θ )) + V 0 ( J ) κ 12 term has resonances at Q = n and 3 Q = n . Ben Pine Space Charge Workshop Oct 5, 2017 13 / 29

  14. Hamiltonian including κ 21 y 2 where T 21 is constant absorbing κ 21 κ 21 image term inserted as T 21 y ¯ and other constant terms. Changing y to action-angle variables and substituting for ¯ y : 2 J ω sin 2 φ a 2 n cos 2 n θ + V 0 ( J ) H = ω J + T 21 J H = ω J + T 21 a 2 2 ω (1 + cos 2 n θ − cos 2 φ − cos 2 φ cos 2 n θ ) + V 0 ( J ) n Of terms in bracket, 1 st is tune shift and 2 nd and 3 rd average to zero. Last term is dominant. cos 2 φ cos 2 n θ = 1 2 (cos(2 φ − 2 n θ ) + cos(2 φ + 2 n θ )) Resonance due to κ 21 term at 2 Q = 2 n . Ben Pine Space Charge Workshop Oct 5, 2017 14 / 29

  15. Coherent response of the beam Single particle analysis incomplete Beam responds coherently to excitation Resonant frequencies are modified Behaviour can be described with an altered resonance formula ω = nQ H + mQ V + ∆ ω = N In simulations to follow resonances were located by scanning intensity and so shifting the coherent frequencies Ben Pine Space Charge Workshop Oct 5, 2017 15 / 29

  16. Selected simulation results Overview Self-consistent PIC simulations Smooth focusing or alternating gradient Simulations run for 100 turns RMS orbit and envelope matched beam distributions Coherent moments, single particle tunes, phase space distributions and losses recorded Dipole driving terms applied singly or harmonically Ben Pine Space Charge Workshop Oct 5, 2017 16 / 29

  17. Selected simulation results Overview For each higher order term that was investigated the same procedure was followed 1 Start with a zero intensity beam 2 Move the tune of the lattice to a suitable point 3 Kick the beam to create the required closed orbit harmonic 4 Match the new closed orbit 5 Increase the beam intensity until the coherent beam frequency interacted with the image driving term 6 With each step in intensity, re-match the RMS orbit and envelope Ben Pine Space Charge Workshop Oct 5, 2017 17 / 29

  18. Selected simulation results KV beam, smooth focusing lattice, κ 12 image term, driven with 13 th harmonic closed orbit Quadrupole moment spectra with closed orbit excited by single kick driving κ 21 image term at 9 th harmonic, at intensities of 0, 3 and 5 . 5 × 10 13 ppp. Blue: horizontal, yellow: vertical. Ben Pine Space Charge Workshop Oct 5, 2017 18 / 29

  19. Selected simulation results KV beam, smooth focusing lattice, κ 12 image term, driven with 13 th harmonic closed orbit Horizontal phase space on turns 50, 60 and 70 for beam excited by single kick driving κ 21 image term at 9 th harmonic, at intensity of 5 . 5 × 10 13 ppp. Ben Pine Space Charge Workshop Oct 5, 2017 19 / 29

  20. Selected simulation results WB beam, smooth focusing lattice, investigation of effects of 4 th harmonic closed orbit at ISIS nominal tunes Quadrupole moment spectra with 4 th harmonic closed orbit driving κ 21 image term at 8 th harmonic, at intensities of 0, 5 and 6 × 10 13 ppp. Blue: horizontal, yellow: vertical. Ben Pine Space Charge Workshop Oct 5, 2017 20 / 29

  21. Selected simulation results WB beam, smooth focusing lattice, investigation of effects of 4 th harmonic closed orbit at ISIS nominal tunes Sextupole moment spectra with 4 th harmonic closed orbit driving κ 30 image term at 12 th harmonic, at intensities of 0, 5 and 6 × 10 13 ppp. Blue: horizontal, yellow: vertical. Ben Pine Space Charge Workshop Oct 5, 2017 21 / 29

  22. Selected simulation results WB beam, smooth focusing lattice, investigation of effects of 4 th harmonic closed orbit at ISIS nominal tunes Horizontal phase space showing integer resonance for waterbag beam driven with 4 th harmonic closed orbit at intensity of 6 × 10 13 ppp, on turns 10, 20 and 30. Ben Pine Space Charge Workshop Oct 5, 2017 22 / 29

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