PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The characteristics of beam mod ulation in the relativistic klystron amplifier at 1.3 and 3.3 GHz are analyzed. Good agreement is found between our simulation results and the 1.3-GHz RK A experiment by Friedman and Serlin. The unstable window modes for a 3.3-GHz RKA configurat ion are identified, and met hods for suppressing the window modes are discussed.
Chiping Chen,Palmyra Catravas, andGeorge Bekefi
"Design studies of a 3.3-GHz relativistic klystron amplifier", Proc. SPIE 1629, Intense Microwave and Particle Beams III, (1 April 1992); https://doi.org/10.1117/12.137151
ACCESS THE FULL ARTICLE
INSTITUTIONAL Select your institution to access the SPIE Digital Library.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The alert did not successfully save. Please try again later.
Chiping Chen, Palmyra Catravas, George Bekefi, "Design studies of a 3.3-GHz relativistic klystron amplifier," Proc. SPIE 1629, Intense Microwave and Particle Beams III, (1 April 1992); https://doi.org/10.1117/12.137151