DocumentCode :
2744867
Title :
Progress in pulsed high power microwave source research at the University of Strathclyde
Author :
Cross, A.W. ; Phelps, A.D.R.
Author_Institution :
Dept. of Phys. & Appl. Phys., Strathclyde Univ., Glasgow, UK
fYear :
2000
fDate :
12-15 Sept. 2000
Firstpage :
379
Lastpage :
380
Abstract :
In general the coherent gain in high power microwave sources arises from the collective interaction of a beam of electrons with the electromagnetic fields of a cavity. In the case of pulsed microwave sources the electron beam itself is pulsed and is supplied from pulsed power supplies. The term "microwave" is taken here as applying to the electromagnetic wave spectrum in the range 1-300 GHz. Microwave sources can be continuous (CW) or pulsed and "high power" in this context typically means CW sources with average powers of 10\´s of kWs to MWs and pulsed sources capable of peak powers from MWs to GWs and beyond.
Keywords :
cavity resonators; electron beams; gyrotrons; microwave generation; microwave tubes; millimetre wave generation; millimetre wave tubes; pulsed power supplies; 1 to 300 GHz; CW microwave source; CW sources; University of Strathclyde; average powers; cavity; coherent gain; collective interaction; continuous wave microwave source; electromagnetic fields; electromagnetic wave spectrum; electron beam; high power microwave source; high power microwave source research; high power microwave sources; microwave; microwave sources; peak powers; pulsed electron beam; pulsed high power microwave source research; pulsed microwave sources; pulsed power supplies; pulsed sources; Cathodes; Current density; Electron beams; Microwave devices; Physics; Plasma density; Plasma waves; Pulsed power supplies; Space charge; Voltage;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Infrared and Millimeter Waves, 2000. Conference Digest. 2000 25th International Conference on
Conference_Location :
Beijing, China
Print_ISBN :
0-7803-6513-5
Type :
conf
DOI :
10.1109/ICIMW.2000.893069
Filename :
893069
Link To Document :
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