Experimental studies of bandwidth and power production in a three-cavity, 35 GHz gyroklystron amplifier

被引:41
作者
Calame, JP [1 ]
Garven, M
Choi, JJ
Nguyen, K
Wood, F
Blank, M
Danly, BG
Levush, B
机构
[1] USN, Res Lab, Washington, DC 20375 USA
[2] Univ Maryland, College Pk, MD 20742 USA
[3] Kwangwoon Univ, Dept Radio Engn, Seoul, South Korea
[4] KN Res, Rockville, MD 20850 USA
[5] Dyncorp, Rockville, MD 20850 USA
关键词
D O I
10.1063/1.873283
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The operating characteristics of a three-cavity, Ka-Band gyroklystron employing a large amount of stagger-tuning are reported. Particular attention is given to examining how the frequency response (peak power, bandwidth, and overall shape) is altered by changes in operating parameters. A peak power of 225 kW at 34.90 GHz, with a 2 mu s pulse length, 32% efficiency, 30.3 dB saturated gain, and a 3 dB bandwidth of 0.82% (286 MHz) was obtained with a 70.2 kV, 10.0 A beam at a magnetic field of 13.07 kG. This operating point represents a compromise between the output power and the bandwidth. The operating magnetic field was found to have a dramatic influence on the power-bandwidth tradeoff; a lower field of 12.91 kG produced 245 kW with 0.63% bandwidth, while a higher field of 13.39 kG increased the bandwidth to 0.94% at a lower power of 200 kW. The results are in excellent agreement with large signal simulations. (C) 1999 American Institute of Physics. [S1070-664X(99)02001-7].
引用
收藏
页码:285 / 297
页数:13
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