Mode control in a high gain relativistic klystron amplifier with 3 GW output power

被引:5
|
作者
Wu Yang [1 ,2 ]
Xie Hong-Quan [3 ]
XU Zhou [1 ]
机构
[1] China Acad Engn Phys, Inst Appl Elect, Mianyang 621900, Peoples R China
[2] Sci & Technol High Power Microwave Lab, Mianyang 621900, Peoples R China
[3] Southwestern Univ Sci & Technol, Coll Sci, Mianyang 621010, Peoples R China
基金
中国国家自然科学基金;
关键词
high power microwave; relativistic klystron amplifier; high gain; mode control;
D O I
10.1088/1674-1137/38/1/017001
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
Higher mode excitation is very serious in the relativistic klystron amplifier, especially for the high gain relativistic amplifier working at tens of kilo-amperes. The mechanism of higher mode excitation is explored in the PIC simulation and it is shown that insufficient separation of adjacent cavities is the main cause of higher mode excitation. So RF lossy material mounted on the drift tube wall is adopted to suppress higher mode excitation. A high gain S-band relativistic klystron amplifier is designed for the beam current of 13 kA and the voltage of 1 MV. PIC simulation shows that the output power is 3.2 GW when the input power is only 2.8 kW.
引用
收藏
页数:4
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