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Efficient, 100-160 MW, X- and Ku-band gyroklystron amplifier designs for linear colliders

Summary form only given. Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirem...

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Main Authors: Saraph, G.P., Lawson, W., Anderson, J.P., Castle, M., Granatstein, V.L.
Format: Conference Proceeding
Language:English
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Lawson, W.
Anderson, J.P.
Castle, M.
Granatstein, V.L.
description Summary form only given. Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirements. Simulations are carried out using the existing set of codes which includes a scattering matrix code for cold-cavity fields, a linear start-oscillation code for stability, and a nonlinear gyroklystron code for optimizing parameters to get maximum efficiency and gain. The cavities are designed to have high mode purity, good inter-cavity isolation, and stability to the excitation of the spurious modes. The quality factors of the cavities, the lengths of the drift sections, and the magnetic field profile are optimized for each design. During this study, the effect of velocity spread in the beam on the efficiency of the device is taken into account. In addition, HFSS code is used to study the effect of dielectric loading and power losses in the cavity.
doi_str_mv 10.1109/PLASMA.1996.551515
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Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirements. Simulations are carried out using the existing set of codes which includes a scattering matrix code for cold-cavity fields, a linear start-oscillation code for stability, and a nonlinear gyroklystron code for optimizing parameters to get maximum efficiency and gain. The cavities are designed to have high mode purity, good inter-cavity isolation, and stability to the excitation of the spurious modes. The quality factors of the cavities, the lengths of the drift sections, and the magnetic field profile are optimized for each design. During this study, the effect of velocity spread in the beam on the efficiency of the device is taken into account. 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Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirements. Simulations are carried out using the existing set of codes which includes a scattering matrix code for cold-cavity fields, a linear start-oscillation code for stability, and a nonlinear gyroklystron code for optimizing parameters to get maximum efficiency and gain. The cavities are designed to have high mode purity, good inter-cavity isolation, and stability to the excitation of the spurious modes. The quality factors of the cavities, the lengths of the drift sections, and the magnetic field profile are optimized for each design. During this study, the effect of velocity spread in the beam on the efficiency of the device is taken into account. 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Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirements. Simulations are carried out using the existing set of codes which includes a scattering matrix code for cold-cavity fields, a linear start-oscillation code for stability, and a nonlinear gyroklystron code for optimizing parameters to get maximum efficiency and gain. The cavities are designed to have high mode purity, good inter-cavity isolation, and stability to the excitation of the spurious modes. The quality factors of the cavities, the lengths of the drift sections, and the magnetic field profile are optimized for each design. During this study, the effect of velocity spread in the beam on the efficiency of the device is taken into account. In addition, HFSS code is used to study the effect of dielectric loading and power losses in the cavity.</abstract><cop>United States</cop><pub>IEEE</pub><doi>10.1109/PLASMA.1996.551515</doi></addata></record>
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identifier ISSN: 0730-9244
ispartof IEEE Conference Record - Abstracts. 1996 IEEE International Conference on Plasma Science, 1996, p.265
issn 0730-9244
2576-7208
language eng
recordid cdi_ieee_primary_551515
source IEEE Electronic Library (IEL) Conference Proceedings
subjects CAVITY RESONATORS
COMPUTERIZED SIMULATION
Cyclotrons
DESIGN
Dielectric losses
Klystrons
LINEAR COLLIDERS
Magnetic fields
MICROWAVE AMPLIFIERS
PARTICLE ACCELERATORS
Plasma simulation
Plasma sources
POWER RANGE 100-1000 MW
Pulse amplifiers
Q factor
Scattering parameters
Stability
title Efficient, 100-160 MW, X- and Ku-band gyroklystron amplifier designs for linear colliders
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