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Simulation, measurement, and mitigation of beam instability caused by the kicker impedance in the 3-GeV rapid cycling synchrotron at the Japan Proton Accelerator Research Complex

机译:在日本质子加速器研究中心的3-GeV快速循环同步加速器中,由突跳阻抗引起的光束不稳定性的仿真,测量和缓解

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The transverse impedance of eight extraction pulsed kicker magnets is a strong beam instability source in the 3-GeV rapid cycling synchrotron (RCS) at the Japan Proton Accelerator Research Complex. Significant beam instability occurs even at half of the designed 1 MW beam power when the chromaticity ($ensuremath{xi}$) is fully corrected for the entire acceleration cycle by using ac sextupole (SX) fields. However, if $ensuremath{xi}$ is fully corrected only at the injection energy by using dc SX fields, the beam is stable. In order to study realistic beam instability scenarios, including the effect of space charge and to determine practical measures to accomplish 1 MW beam power, we enhance the orbit particle tracking code to incorporate all realistic time-dependent machine parameters, including the time dependence of the impedance itself. The beam stability properties beyond 0.5 MW beam power are found to be very sensitive to a number of parameters in both simulations and measurements. In order to stabilize a beam at 1 MW beam power, two practical measures based on detailed and systematic simulation studies are determined, namely, (i) proper manipulation of the betatron tunes during acceleration and (ii) reduction of the dc SX field to reduce the $ensuremath{xi}$ correction even at injection. The simulation results are well reproduced by measurements, and, as a consequence, an acceleration to 1 MW beam power is successfully demonstrated. In this paper, details of the orbit simulation and the corresponding experimental results up to 1 MW of beam power are presented. To further increase the RCS beam power, beam stability issues and possible measures beyond 1 MW beam power are also considered.
机译:在日本质子加速器研究中心的3-GeV快速循环同步加速器(RCS)中,八个抽出脉冲的喷射器磁铁的横向阻抗是强烈的光束不稳定源。当通过使用交流六极(SX)场在整个加速周期中完全校正了色度($ ensuremath { xi} $)时,即使在设计的1 MW光束功率的一半处,也会出现明显的光束不稳定性。但是,如果仅通过使用dc SX场在注入能量处对$ ensuremath { xi} $进行完全校正,则光束是稳定的。为了研究现实的光束不稳定情况,包括空间电荷的影响并确定实现1 MW光束功率的实际措施,我们增强了轨道粒子跟踪代码,以纳入所有与时间相关的真实机器参数,包括与时间有关的机器参数。阻抗本身。在模拟和测量中,发现束功率超过0.5 MW的束稳定性对许多参数非常敏感。为了将光束稳定在1 MW的光束功率下,基于详细和系统的模拟研究,确定了两种可行的措施,即(i)在加速过程中适当控制电子加速器调谐,以及(ii)减小直流SX场以减小$ ensuremath { xi} $更正,即使在注射时也是如此。通过测量可以很好地再现模拟结果,因此,成功证明了向1 MW光束功率的加速。本文介绍了高达1 MW束功率的轨道模拟的细节以及相应的实验结果。为了进一步增加RCS束功率,还考虑了束稳定性问题和超过1 MW束功率的可能措施。

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