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High power microwave emission and diagnostics of microsecond electron beams

Abstract

Experiments were performed to generate high power, long-pulse microwaves by the gyrotron mechanism in rectangular cross-section interaction cavities. Long-pulse electron beams are generated by MELBA (Michigan Electron Long Beam Accelerator), which operates with parameters: -0.8 MV, 1-10 kA, and 0.5-1 microsecond pulse length. Microwave power levels are in the megawatt range. Polarization control is being studied by adjustment of the solenoidal magnetic field. Initial results show polarization power ratios up to a factor of 15. Electron beam dynamics (V{sub perp}/V{sub par}) are being measured by radiation darkening on glass plates. Computer modeling utilizes the MAGIC Code for electromagnetic waves and a single electron orbit code that includes a distribution of angles. (author). 4 figs., 4 refs.
Authors:
Gilgenbach, R; Hochman, J M; Jayness, R; Rintamaki, J I; Lau, Y Y; Luginsland, J; Lash, J S; [1]  Spencer, T A [2] 
  1. Univ. of Michigan, Ann Arbor, MI (United States). Intense Electron Beam Interaction Lab.
  2. Air Force Phillips Lab., Kirtland AFB, NM (United States)
Publication Date:
Dec 31, 1996
Product Type:
Conference
Report Number:
INIS-CZ-0002; CONF-960610-
Reference Number:
SCA: 661220; PA: AIX-28:055632; EDB-97:113960; SN: 97001834637
Resource Relation:
Conference: BEAMS `96: 11. international conference on high-power particle beams, Prague (Czech Republic), 10-14 Jun 1996; Other Information: PBD: 1996; Related Information: Is Part Of Beams `96. Proceedings of the 11th international conference on high power particle beams. Vol. I; Jungwirth, K.; Ullschmied, J. [eds.]; PB: [684] p.
Subject:
66 PHYSICS; ELECTRON BEAMS; MICROWAVE RADIATION; MICROWAVE AMPLIFIERS; COMPUTERIZED SIMULATION; BEAM DYNAMICS; CAVITY RESONATORS; ELECTRONS; KILO AMP BEAM CURRENTS; MAGNETIC FIELDS; POLARIZATION; POWER RANGE 01-10 MW; RELATIVISTIC RANGE; TRAJECTORIES
OSTI ID:
511045
Research Organizations:
Ceskoslovenska Akademie Ved, Prague (Czech Republic). Ustav Fyziky Plazmatu
Country of Origin:
Czech Republic
Language:
English
Other Identifying Numbers:
Other: ON: DE97637662; ISBN 80-902250-3-9; TRN: CZ9726739055632
Availability:
INIS; OSTI as DE97637662
Submitting Site:
INIS
Size:
pp. 347-350
Announcement Date:
Sep 04, 1997

Citation Formats

Gilgenbach, R, Hochman, J M, Jayness, R, Rintamaki, J I, Lau, Y Y, Luginsland, J, Lash, J S, and Spencer, T A. High power microwave emission and diagnostics of microsecond electron beams. Czech Republic: N. p., 1996. Web.
Gilgenbach, R, Hochman, J M, Jayness, R, Rintamaki, J I, Lau, Y Y, Luginsland, J, Lash, J S, & Spencer, T A. High power microwave emission and diagnostics of microsecond electron beams. Czech Republic.
Gilgenbach, R, Hochman, J M, Jayness, R, Rintamaki, J I, Lau, Y Y, Luginsland, J, Lash, J S, and Spencer, T A. 1996. "High power microwave emission and diagnostics of microsecond electron beams." Czech Republic.
@misc{etde_511045,
title = {High power microwave emission and diagnostics of microsecond electron beams}
author = {Gilgenbach, R, Hochman, J M, Jayness, R, Rintamaki, J I, Lau, Y Y, Luginsland, J, Lash, J S, and Spencer, T A}
abstractNote = {Experiments were performed to generate high power, long-pulse microwaves by the gyrotron mechanism in rectangular cross-section interaction cavities. Long-pulse electron beams are generated by MELBA (Michigan Electron Long Beam Accelerator), which operates with parameters: -0.8 MV, 1-10 kA, and 0.5-1 microsecond pulse length. Microwave power levels are in the megawatt range. Polarization control is being studied by adjustment of the solenoidal magnetic field. Initial results show polarization power ratios up to a factor of 15. Electron beam dynamics (V{sub perp}/V{sub par}) are being measured by radiation darkening on glass plates. Computer modeling utilizes the MAGIC Code for electromagnetic waves and a single electron orbit code that includes a distribution of angles. (author). 4 figs., 4 refs.}
place = {Czech Republic}
year = {1996}
month = {Dec}
}