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Kornilov, V.

Paper Title Page
TUPD004 Linear Coupling with Space Charge in SIS18 1922
 
  • W.M. Daqa
    IAP, Frankfurt am Main
  • O. Boine-Frankenheim, I. Hofmann, V. Kornilov, J. Struckmeier
    GSI, Darmstadt
 
 

For high current synchrotrons and for the SIS18 operation as booster of the projected SIS100 it is important to improve the multi-turn injection efficiency. This can be achieved by coupling the transverse planes with skew quadrupoles, which can move the particles away from the septum. Linear betatron coupling by skew quadrupole components in SIS18 including space charge effect was studied in an experiment using different diagnostic methods during the crossing of the difference coupling resonance. The beam loss was measured using a fast current transformer, the transverse emittance exchange was observed using a residual gas monitor and the coupled tunes were obtained from the Schottky noise spectrum. We compared the experimental results with simulation using PARMTRA which is a code developed at GSI.

 
TUPD029 Coherent Instability Thresholds and Dynamic Aperture with Octupoles and Nonlinear Space-Charge in the SIS100 Synchrotron 1988
 
  • V. Kornilov, O. Boine-Frankenheim
    GSI, Darmstadt
  • V.V. Kapin
    ITEP, Moscow
 
 

Octupole magnets can be used as a passive cure against transverse collective instabilities. The octupole field creates a betatron frequency spread due to amplitude-dependent tune shift and thus enhances Landau damping. The drawback is the reduction of the dynamic aperture (DA). Ultimately, a balance between collective damping and DA must be found. Here we analyse the transverse coherent instability thresholds in SIS100 with octupoles and nonlinear space-charge taken into account. As the major impedance sources at low frequencies, the resistive wall and the kickers are considered. A coasting beam is assumed, which results in a conservative stability estimation. On the other hand, we simulate the DA of the SIS100 lattice using the MADX code, with systematic multipole errors, random multipole errors, and closed-orbit errors taken into account.