Radio frequency priming of a long-pulse relativistic magnetron
White, W.M.
Gilgenbach, R.M.
Jones, M.C.
Neculaes, V.B.
Yue Ying Lau
Pengvanich, P.
Jordan, N.M.C.
Hoff, B.W.
Edgar, R.
Spencer, T.A.
Price, D.
Sandia Nat. Labs., Albuquerque, NM;
This paper appears in: Plasma Science, IEEE Transactions on
Publication Date: June 2006
Volume: 34,
Issue: 3, Part 1
On page(s): 627-634
Location: Eindhoven, Netherlands,
ISSN: 0093-3813
INSPEC Accession Number: 8962197
Digital Object Identifier: 10.1109/TPS.2006.875829
Current Version Published: 2006-06-19
|
Rapid startup, increased pulsewidth, and mode locking of magnetrons have been explored experimentally on a relativistic magnetron by radio frequency (RF) priming. Experiments utilize a -300 kV, 2-8 kA, 300-500-ns electron beam to drive a Titan six-vane relativistic magnetron (5-100 MW output power in each of the three waveguides). The RF priming source is a 100-kW pulsed magnetron operating at 1.27-1.32 GHz. Tuning stubs are utilized in the Titan structure to adjust the frequency of the relativistic magnetron to match that of the priming source. Experiments are performed on rising sun as well as standard anode configurations. Magnetron start-oscillation time, pulsewidth, and pi-mode locking are compared with RF priming versus the unprimed case. The results show significant reductions in microwave output delay and mode competition even when Adler's Relation is not satisfied
|
Cart
