45 th ICFA Beam Dynamic Workshop June 8–12, 2009, Cornell University, Ithaca New York Modelling Cyclotron Resonances in ECLOUD 1) Comparison with CesrTA.

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Presentation transcript:

45 th ICFA Beam Dynamic Workshop June 8–12, 2009, Cornell University, Ithaca New York Modelling Cyclotron Resonances in ECLOUD 1) Comparison with CesrTA and PEP-II Measurements 2) Exploration of SEY parameter space 3) Next Steps Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education Electron Cloud Simulations Meeting 22 July 2009

Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 2/13 June 2009 CesrTA Measurements See talk by Joe Calvey, CTA09 4 ns, 2 GeV TiN Collector 1TiN Collector 9 Alu Collector 1Al Collector 9

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 3/13 ECLOUD Model for CesrTA Aluminum  (0)=1.0  max =2.0 E peak = 300 eV Resonant enhancement for uncoated Al chamber. Collector number defined by azimuthal impact position on wall. RFA area and transparency used to calculate currents. Summed over 90 bunches, 45 filled, 0.9 mA. with 4 ns spacing. No modelling of kinematic acceptance or cloud/RFA interaction

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 4/13 ECLOUD Model for CesrTA Aluminum  (0)=1.0  max =2.0 E peak = 300 eV No saturation for CesrTA conditions. Off resonance / n=1.45 B=129 GOn resonance / n=1.0 B=89 G

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 5/13 ECLOUD Model for CesrTA Aluminum  (0)=1.0  max =2.0 E peak = 300 eV The SEY curve for Al results in a higher yield region being populated by the resonant energy and grazing angle enhancement. Off resonance / n=1.45 B=129 GOn resonance / n=1.0 B=89 G

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 6/13 ECLOUD Model for CesrTA Aluminum  (0)=1.0  max = 0.4 E peak = 500 eV Resonant enhancement for TiN-coated chamber. To get resonant suppression, need  max < 0.6. Direct SEY measurements gave a value of 0.95 (Pivi, et al). Collector number defined by azimuthal impact position on wall. RFA area and transparency used to calculate currents. Summed over 90 bunches, 45 filled, 0.9 mA. with 4 ns spacing. No modelling of kinematic acceptance or cloud/RFA interaction

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 7/13 ECLOUD Model for CesrTA TiN  (0)=1.0  max =0.4 E peak = 500 eV TiN coating provides saturation, even on resonance. Off resonance / n=1.43 B=127 GOn resonance / n=1.0 B=89 G

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 8/13 ECLOUD Model for CesrTA TiN  (0)=1.0  max =0.4 E peak = 500 eV Resonant suppression results from competing effects. Off resonance / n=1.43 B=127 GOn resonance / n=1.0 B=89 G

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 9/13 AluminumTiN-Coating SLAC-PUB Observation of Magnetic Resonances in Electron Clouds In A Positron Storage Ring, M.T.F. Pivi, et al, SLAC-PUB PEP-II e + beam mA bunches 4.2 ns spacing

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 10/13 ECLOUD Model for PEP-II Al  (0)=1.0  max =2.0 E peak = 310 eV ECLOUD finds saturation in PEP-II conditions, consistent with measurements. Off resonance / n=4.4 B=364 GOn resonance / n=4.0 B=341 G

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 11/13 ECLOUD Model for PEP-II Al  (0)=1.0  max =2.0 E peak = 310 eV Collector number defined by azimuthal impact position on wall. RFA area and transparency used to calculate currents. Summed over mA bunches with 4.2 ns spacing. No modelling of kinematic acceptance or cloud/RFA interaction ECLOUD fails to model the resonant suppression for the PEP-II Al chamber with the expected SEY parameters. It does model the dips in the low-n resonances, in agreement with POSINST.

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 12/13 ECLOUD Model for PEP-II Al  (0)=1.0  max =0.5 E peak = 500 eV Collector number defined by azimuthal impact position on wall. RFA area and transparency used to calculate currents. Summed over mA bunches with 4.2 ns spacing. No modelling of kinematic acceptance or cloud/RFA interaction ECLOUD can model resonant suppression --> enhancement in the same chicane scan, but the comparison with the PEP-II measurements is not satisfactory.

22 July 2009 Modelling Cyclotron Resonances with ECLOUD / J.A.Crittenden 13/13 Present Status and Plans ECLOUD can model both resonant suppression and enhancement if the secondary yield curve has a minimum between low energy and the peak energy. At present we have studied primarily  (0) = 1.0. We have mapped out the resonant behavior as a function of the SEY parameters  max and E peak for PEP-II and CesrTA conditions. Attempts to model the PEP-II measurements of SLAC-PUB appear to require lower yields than we expect, and the level of agreement is unsatisfactory. Highest priority is now placed on modelling RFA acceptance and secondary yield, as coded by Joe Calvey. We can hope/expect that iterative feedback between modelling and measurements during upcoming data-taking period will provide additional understanding of the physics of electron cloud development.