30 November 2017 Design of a 100 MW, 17 GHz second harmonic gyroklystron experiment
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Proceedings Volume 2104, 18th International Conference on Infrared and Millimeter Waves; 21047D (2017) https://doi.org/10.1117/12.2298697
Event: 18th International Conference on Infrared and Millimeter Waves, 1993, Colchester, United Kingdom
Abstract
In an effort to expand the frontiers of high-energy physics, electron-positron colliders withcenter-of-mass energies approaching 1 TeV (and beyond) are being planned.1 These machines willrequire efficient, reliable, pulsed microwave amplifiers with peak power levels exceeding the state- of-the-art. The current linear collider standard is the 100 GeV Stanford Linear Collider,2 for whicha 1 ,us, 150 MW, S-Band klystron was developed.3 It is anticipated that comparable power levelswill be required in 10-20 GHz devices. Because klystron peak power scales (optimistically) withthe output wavelength squared, considerable enhancement is required.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
P. E. Latham, "Design of a 100 MW, 17 GHz second harmonic gyroklystron experiment", Proc. SPIE 2104, 18th International Conference on Infrared and Millimeter Waves, 21047D (30 November 2017); doi: 10.1117/12.2298697; https://doi.org/10.1117/12.2298697
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