Paper
8 September 1995 Power electron beam front shortening for intense-microwave pulse generation
Eugene A. Galstjan, Lev N. Kazanskiy
Author Affiliations +
Abstract
The starting point for this investigation is a suggestion that it is possible to get a clearly defined shock electromagnetic wave in a quite short modified magnetically insulated transmittion line (MITL). The line modification resides in an inner coaxial dielectric insert. One may consider the insert as a distributed matched spark-gap. The parameters of the high voltage pulse supplying at the line input are as follows: 1.5 MV, 20-30 kA, 90 ns, front duration--30 ns. A current pulse with a front duration less than 1 ns has been observed at the line output. The output current has ranged up to about 10--12 kA. Efficiency of the sharp front formation grows owing to its dependence on the speed of the flashover front propagation. So, an estimation of this dependence is a step of great importance is solution of the problem. The flashover front speed has been estimated on physical grounds which can be derived from experimental data for the early phases of dielectric surface flashover in vacuum.
© (1995) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Eugene A. Galstjan and Lev N. Kazanskiy "Power electron beam front shortening for intense-microwave pulse generation", Proc. SPIE 2557, Intense Microwave Pulses III, (8 September 1995); https://doi.org/10.1117/12.218566
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Dielectrics

Electron beams

Electromagnetism

Radio propagation

Diodes

Electromagnetic radiation

Wave propagation

RELATED CONTENT

Negative energy cyclotron resonance maser
Proceedings of SPIE (December 01 1990)
Terahertz sources
Proceedings of SPIE (June 02 1994)
Study of electromagnetic shock wave in modified MITL
Proceedings of SPIE (October 28 1996)

Back to Top