DocumentCode
1209763
Title
Experimental studies of stability and amplification in a two-cavity second harmonic gyroklystron
Author
Matthews, H.W. ; Lawson, W. ; Calame, J.P. ; Flaherty, M.K.E. ; Hogan, B. ; Cheng, J. ; Latham, P.E.
Author_Institution
Lab. for Plasma Res., Maryland Univ., College Park, MD, USA
Volume
22
Issue
5
fYear
1994
fDate
10/1/1994 12:00:00 AM
Firstpage
825
Lastpage
833
Abstract
We report the operating characteristics of a sequence of two-cavity second harmonic gyroklystrons which are derived in part from a previous fundamental tube and utilize output cavities which resonate at twice the drive frequency. We present results from the design simulations as well as details of the stable range of operating parameters. While the harmonic tube is somewhat more susceptible to spurious oscillations and more sensitive to parameter variations than the fundamental device, there is still considerable parameter space available for amplifier operation. Peak powers above 30 MW are obtained with efficiencies greater than 28% and large signal gains of 27 dB. These results depend critically on the magnetic field profile which has a slight up-taper at the optimum operating point. The nominal beam parameters include a pulse length of 1 μs, a voltage near 450 kV, a current in the range 235-245 A, and a perpendicular to parallel velocity ratio (α=v⊥/vz) near one
Keywords
cavity resonators; gyrotrons; harmonics; klystrons; microwave power amplifiers; plasma instability; 1 mus; 235 to 245 A; 27 dB; 28 percent; 30 MW; 450 kV; amplifier operation; design simulations; magnetic field profile; nominal beam parameters; operating characteristics; output cavities; parameter space; pulse length; spurious oscillations; stability; two-cavity second harmonic gyroklystron; velocity ratio; Cyclotrons; Frequency; Gyrotrons; Klystrons; Magnetic fields; Magnetic resonance; Particle beams; Pulse amplifiers; Stability; Voltage;
fLanguage
English
Journal_Title
Plasma Science, IEEE Transactions on
Publisher
ieee
ISSN
0093-3813
Type
jour
DOI
10.1109/27.338298
Filename
338298
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