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ESS Workshop


        How Well Do Our Numerical
       Simulations Predict the Beam
    Performance in the Linacs We Build?
                  J. Stovall




                 April, 2009
                  Bilbao

ESS2009 Bilbao                    CERN/TERA
Are Accurate Simulations Important?
•We rely on them initially to validate/certify the machine
design
   •Linac
       •Verify the design details
       •Bracket allowable errors
       •Identify expected sources of beam loss
       •Developing commissioning strategies
   •Beam properties on target
       •Energy, emittance & halo at full current
   •The codes themselves must be “certified” at some level


ESS2009 Bilbao                                    CERN/TERA
Codes Do a Very Good Job Qualitatively
                    25
                                                           DTL-CCL Transition               CCL-SCL Transition
                             1 0 L in a c s , a ll e r r o r s
                                                                                                           Predicted beam loss in
                    20       + m is m a tc h

                                                                                                           SNS warm linac with
    Beam Loss (W)




                                          P m in
                                                                                                           errors
                    15                    Pave
                                          Pm ax

                    10


                     5


                     0
                         0      20        40        60           80     100     120   140   160   180   200
                                                                      W (M e V )

                                                                                                         Measured activation in
                                                                                                         the SNS CCL
Measured Residual
activation @ 1ft after ~ 48h
1 W gives ~ 100 mRem/hr
at 1 ft after ~ 12 hrs

                                                                                                        Galambos, SNS


  ESS2009 Bilbao                                                                                                        CERN/TERA
Simulation Codes Agree at Few % Level
                                                                                              UNILAC RMS Beam Size
                          SNS DTL-1 99% Emittance
                                                                                                 Profiles 4 Codes
                              Profiles 5 Codes
                0.40
                0.38
                0.36
                                                                    3% εt
                0.34
εn,99% (πcm-mrad)




                0.32
                0.30
                0.28
                0.26
                0.24
                0.22
                0.20
                   0.06   0.07   0.08   0.09   0.10   0.11   0.12   0.13    0.14
                                               β




                                                                                   Groening, GSI

           ESS2009 Bilbao                                                                                  CERN/TERA
Codes Differ in the Details
                             Radial Distribution at Tank 1 Exit
                 6.0
              10   8
                   5
                   4
                   3
                                                          1M particle
                   2
                   2
                 5.0
              10   8
                   5
                                                            ParTrans
                   4
                   3
                   2
                   2
                                                            IMPACT
              104.0
                 8
                                                            LINAC
                   5
                   4
                   3
                   2
                   2
                                                            PARMELA
   I (nAmp)




              103.0
                 8
                                                            PARMILA
                   5
                   4
                   3
                   2
                   2
              102.0
                 8
                   5
                   4
                   3
                   2
                   2
              101.0
                 8
                   5
                   4
                   3
                   2
                   2
              100.0
                 7
                                                   11%
                   5
                   4
                   3
                   2
                   2
              10-1.0
                       0     1     2     3     4      5       6        7     8
                                   Normalized Beam Radius (σ)
ESS2009 Bilbao                                                             CERN/TERA
Is This the Right Question?
•Some put far too much emphasis on how well our codes
predict beam behave
•Machines are never built exactly like our computer models
say they should be
    •There are always unknown errors introduced during
    fabrication & assembly
•We never know the exact initial conditions
    •Beam or linac parameters
•We can come close, and the codes will give a good
indication of what the beam will look like
•Equally important, however, is to to show how the beam will
change with various machine parameters
•Simulations can predict much more than the diagnostics can
appreciate
ESS2009 Bilbao                                    CERN/TERA
The Codes
   •Beam Optics codes like Trace3D
       •Transform envelope with analytical space charge
       •Do a very 1st order good job
       •Used as basis for most tuning algorithms
   •PIC Dynamics codes
       •Parmila, Tracewin, Linac, Dynamion
       •106 particles with 3-D space charge
       •Matrix based
       •Do a good job on core simulations
       •Agree at few% level
   •Integrating dynamics Codes
       •Impact, Track, Tstep (Parmela)
       •Can now integrate ~109 particles through field
       maps
ESS2009 Bilbao                                    CERN/TERA
Code Limitations
•The real problem is
   •An accurate 6-D description of the initial beam particle
   distribution
   •An accurate description of the fields
       •Magnets and their alignment can be accurately
       mapped
       •The axial rf field distribution in RFQ’s is not
       measurable
       •The rf field distribution in DTLs & CCLs are probably
       reasonably well known from cavity calculations and
       bead pulls
       •The rf field distribution in SC cavities at operating
       temperature is anyone’s guess
       •Rf phase & amplitude errors are transient
ESS2009 Bilbao                                      CERN/TERA
Simulations Can Predict More than
             the Diagnostics Can Appreciate
    = 35       = 60       = 90
o          o          o




                                 Experiment
                                                             Int / Int_max [%]
                                                                   0–5
                                                                  5 – 10
                                                                 10 – 20




                                 DYNAMION
                                                                 20 – 40
                                                                 40 -100




                                 PARMILA
                                                    UNILAC, Final
                                              Distributions (Horizontal)

                                              • core: good agreement (ex. 35°)
                                 TraceWin




                                              • 90°: quot;wingsquot; seen in exp. & sims
                                              • deviations at lowest densities
                                 LORASR




                                                                           Groening, GSI

ESS2009 Bilbao                                                               CERN/TERA
One-to-One RFQ Simulation:~1 B Particles
  • Benefits of simulating a large number of particles: actual number if
    possible
     - Suppress noise from the PIC method: enough particles/cell
     - More detailed simulation: better characterization of the beam halo
       10                      10                       10
        8 1M                    8 10M                    8 100M
        6                       6                        6
        4                       4                        4
∆W/W (%)




                           ∆W/W (%)




                                                    ∆W/W (%)
        2                       2                        2
        0                       0                        0
       -2                      -2                       -2
       -4                      -4                       -4
       -6                      -6                       -6
       -8                      -8                       -8
      -10                     -10                      -10
        -100      0       100   -100       0       100   -100        0       100
               ∆φ (deg)                 ∆φ (deg)                  ∆φ (deg)


                                                                                   Phase space plots
                                                                                   for 865 M protons
                                                                                   after 30 cells in the
                                                                                   RFQ.
                                                                                         Mustapha, ANL


ESS2009 Bilbao                                                                             CERN/TERA
Even 1B Particles Yield a Poor Representation
                     of the Details




                 TRACK, 1B particle    SNS measurement in
                Simulation of an RFQ        MEBT Jeon, SNS
Mustapha, ANL


  ESS2009 Bilbao                                    CERN/TERA
SNS MEBT “Round Beam” Study




                  Jeon, SNS

ESS2009 Bilbao                CERN/TERA
The Roll of Codes in Machine Tuning
•Steering strategies, model-based vs. empirical
• Matching strategies, model-based vs. empirical
• Combined with beam measurements
   •profiles & halo
   •emittance
   •beam loss
   •longitudinal measurements
•Code limitations
•Diagnostics limitations
•SNS has the most relevant experience


ESS2009 Bilbao                                     CERN/TERA
Model-Based Tuning at SNS
•The simulations do a good job on the core, but
   •The particles we are concerned with are in the halo; one
   part in 1E6
   •We are unable to measure beam properties at that level
   •We are lacking input distributions for simulations
   anywhere near that level
•We have pretty good results for model-based tuning, but of
course that is exercising only the core
•Particles destined to get lost don'care what the core is
                                   t
doing



ESS2009 Bilbao                                     CERN/TERA
SNS Warm-Linac Tuning
•In practice we set the warm linac quads up to the design
values
    •PMQs in the DTL
    •EMQs in the CCL
    •With these values, the measured Twiss parameters of
    the beam core are within ~ 10% of expected
    •This is about as good as any matching can do
    •Or as good as we believe the measurements
•Then at high beam intensity we adjust quad strengths
manually to reduce beam loss down the linac.
    •These adjustments are typically < 1% “tweaks”



ESS2009 Bilbao                                    CERN/TERA
SC Linac & HEBT Tuning
•In the superconducting linac we set up the quads to the
design values
    • The laser profile measurements show that the beam is
    poorly matched but
    • They are too slow to be used in iteratively with quad
    adjustments
•In the HEBT we typically see a large mismatch
    •It is easily corrected using a model based technique
    •But the resulting losses at ring injection are higher after
    matching
    •Since we inevitably run out of time we roll back to the
    unmatched setup
•Beam loss is minimized manually – monkey tuning.

ESS2009 Bilbao                                         CERN/TERA
Beam Tracking vs. Beam Dynamics Codes
           Beam optics codes                       Beam dynamics codes
        (example: Trace-3D)                      (example: TRACK, IMPACT)
   Matrix based, usually first order           Particle tracking, all orders included
   Hard-edge field approximation               3D fields including realistic fringe fields
   Space charge forces approximated            Solving Poisson equation at every step
                                               Actual particles distribution: core, halo …
   Beam envelopes and emittances
                                               Slower, Good for detailed studies
   Fast, Good for preliminary studies
                                               including errors and beam loss
   Simplex optimization: Limited number
                                               Larger scale optimization possible
   of fit parameters


   It is more appropriate to use beam dynamics codes for
   optimization:
– More realistic representation of the beam especially for high-intensity and multiple
  charge state beams (3D external fields and accurate SC calculation).
– Include quantities not available from beam optics codes: minimize beam halo formation
  and beam loss.
– Now possible with faster PC’s and parallel computer clusters …
                                                                          Mustapha, ANL


ESS2009 Bilbao                                                              CERN/TERA

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ESS-Bilbao Initiative Workshop. Beam dynamics: Simulations of high power linacs

  • 1. ESS Workshop How Well Do Our Numerical Simulations Predict the Beam Performance in the Linacs We Build? J. Stovall April, 2009 Bilbao ESS2009 Bilbao CERN/TERA
  • 2. Are Accurate Simulations Important? •We rely on them initially to validate/certify the machine design •Linac •Verify the design details •Bracket allowable errors •Identify expected sources of beam loss •Developing commissioning strategies •Beam properties on target •Energy, emittance & halo at full current •The codes themselves must be “certified” at some level ESS2009 Bilbao CERN/TERA
  • 3. Codes Do a Very Good Job Qualitatively 25 DTL-CCL Transition CCL-SCL Transition 1 0 L in a c s , a ll e r r o r s Predicted beam loss in 20 + m is m a tc h SNS warm linac with Beam Loss (W) P m in errors 15 Pave Pm ax 10 5 0 0 20 40 60 80 100 120 140 160 180 200 W (M e V ) Measured activation in the SNS CCL Measured Residual activation @ 1ft after ~ 48h 1 W gives ~ 100 mRem/hr at 1 ft after ~ 12 hrs Galambos, SNS ESS2009 Bilbao CERN/TERA
  • 4. Simulation Codes Agree at Few % Level UNILAC RMS Beam Size SNS DTL-1 99% Emittance Profiles 4 Codes Profiles 5 Codes 0.40 0.38 0.36 3% εt 0.34 εn,99% (πcm-mrad) 0.32 0.30 0.28 0.26 0.24 0.22 0.20 0.06 0.07 0.08 0.09 0.10 0.11 0.12 0.13 0.14 β Groening, GSI ESS2009 Bilbao CERN/TERA
  • 5. Codes Differ in the Details Radial Distribution at Tank 1 Exit 6.0 10 8 5 4 3 1M particle 2 2 5.0 10 8 5 ParTrans 4 3 2 2 IMPACT 104.0 8 LINAC 5 4 3 2 2 PARMELA I (nAmp) 103.0 8 PARMILA 5 4 3 2 2 102.0 8 5 4 3 2 2 101.0 8 5 4 3 2 2 100.0 7 11% 5 4 3 2 2 10-1.0 0 1 2 3 4 5 6 7 8 Normalized Beam Radius (σ) ESS2009 Bilbao CERN/TERA
  • 6. Is This the Right Question? •Some put far too much emphasis on how well our codes predict beam behave •Machines are never built exactly like our computer models say they should be •There are always unknown errors introduced during fabrication & assembly •We never know the exact initial conditions •Beam or linac parameters •We can come close, and the codes will give a good indication of what the beam will look like •Equally important, however, is to to show how the beam will change with various machine parameters •Simulations can predict much more than the diagnostics can appreciate ESS2009 Bilbao CERN/TERA
  • 7. The Codes •Beam Optics codes like Trace3D •Transform envelope with analytical space charge •Do a very 1st order good job •Used as basis for most tuning algorithms •PIC Dynamics codes •Parmila, Tracewin, Linac, Dynamion •106 particles with 3-D space charge •Matrix based •Do a good job on core simulations •Agree at few% level •Integrating dynamics Codes •Impact, Track, Tstep (Parmela) •Can now integrate ~109 particles through field maps ESS2009 Bilbao CERN/TERA
  • 8. Code Limitations •The real problem is •An accurate 6-D description of the initial beam particle distribution •An accurate description of the fields •Magnets and their alignment can be accurately mapped •The axial rf field distribution in RFQ’s is not measurable •The rf field distribution in DTLs & CCLs are probably reasonably well known from cavity calculations and bead pulls •The rf field distribution in SC cavities at operating temperature is anyone’s guess •Rf phase & amplitude errors are transient ESS2009 Bilbao CERN/TERA
  • 9. Simulations Can Predict More than the Diagnostics Can Appreciate = 35 = 60 = 90 o o o Experiment Int / Int_max [%] 0–5 5 – 10 10 – 20 DYNAMION 20 – 40 40 -100 PARMILA UNILAC, Final Distributions (Horizontal) • core: good agreement (ex. 35°) TraceWin • 90°: quot;wingsquot; seen in exp. & sims • deviations at lowest densities LORASR Groening, GSI ESS2009 Bilbao CERN/TERA
  • 10. One-to-One RFQ Simulation:~1 B Particles • Benefits of simulating a large number of particles: actual number if possible - Suppress noise from the PIC method: enough particles/cell - More detailed simulation: better characterization of the beam halo 10 10 10 8 1M 8 10M 8 100M 6 6 6 4 4 4 ∆W/W (%) ∆W/W (%) ∆W/W (%) 2 2 2 0 0 0 -2 -2 -2 -4 -4 -4 -6 -6 -6 -8 -8 -8 -10 -10 -10 -100 0 100 -100 0 100 -100 0 100 ∆φ (deg) ∆φ (deg) ∆φ (deg) Phase space plots for 865 M protons after 30 cells in the RFQ. Mustapha, ANL ESS2009 Bilbao CERN/TERA
  • 11. Even 1B Particles Yield a Poor Representation of the Details TRACK, 1B particle SNS measurement in Simulation of an RFQ MEBT Jeon, SNS Mustapha, ANL ESS2009 Bilbao CERN/TERA
  • 12. SNS MEBT “Round Beam” Study Jeon, SNS ESS2009 Bilbao CERN/TERA
  • 13. The Roll of Codes in Machine Tuning •Steering strategies, model-based vs. empirical • Matching strategies, model-based vs. empirical • Combined with beam measurements •profiles & halo •emittance •beam loss •longitudinal measurements •Code limitations •Diagnostics limitations •SNS has the most relevant experience ESS2009 Bilbao CERN/TERA
  • 14. Model-Based Tuning at SNS •The simulations do a good job on the core, but •The particles we are concerned with are in the halo; one part in 1E6 •We are unable to measure beam properties at that level •We are lacking input distributions for simulations anywhere near that level •We have pretty good results for model-based tuning, but of course that is exercising only the core •Particles destined to get lost don'care what the core is t doing ESS2009 Bilbao CERN/TERA
  • 15. SNS Warm-Linac Tuning •In practice we set the warm linac quads up to the design values •PMQs in the DTL •EMQs in the CCL •With these values, the measured Twiss parameters of the beam core are within ~ 10% of expected •This is about as good as any matching can do •Or as good as we believe the measurements •Then at high beam intensity we adjust quad strengths manually to reduce beam loss down the linac. •These adjustments are typically < 1% “tweaks” ESS2009 Bilbao CERN/TERA
  • 16. SC Linac & HEBT Tuning •In the superconducting linac we set up the quads to the design values • The laser profile measurements show that the beam is poorly matched but • They are too slow to be used in iteratively with quad adjustments •In the HEBT we typically see a large mismatch •It is easily corrected using a model based technique •But the resulting losses at ring injection are higher after matching •Since we inevitably run out of time we roll back to the unmatched setup •Beam loss is minimized manually – monkey tuning. ESS2009 Bilbao CERN/TERA
  • 17. Beam Tracking vs. Beam Dynamics Codes Beam optics codes Beam dynamics codes (example: Trace-3D) (example: TRACK, IMPACT) Matrix based, usually first order Particle tracking, all orders included Hard-edge field approximation 3D fields including realistic fringe fields Space charge forces approximated Solving Poisson equation at every step Actual particles distribution: core, halo … Beam envelopes and emittances Slower, Good for detailed studies Fast, Good for preliminary studies including errors and beam loss Simplex optimization: Limited number Larger scale optimization possible of fit parameters It is more appropriate to use beam dynamics codes for optimization: – More realistic representation of the beam especially for high-intensity and multiple charge state beams (3D external fields and accurate SC calculation). – Include quantities not available from beam optics codes: minimize beam halo formation and beam loss. – Now possible with faster PC’s and parallel computer clusters … Mustapha, ANL ESS2009 Bilbao CERN/TERA