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| Content Provider | IEEE Xplore Digital Library |
|---|---|
| Author | Deeney, C. Douglas, M.R. Coverdale, C.A. Spielman, R.B. Peterson, D.L. Roderick, N. Haines, M.G. Nash, T.J. Derzon, M. McGurn, J. Jobe, D. Gilliland, T. Breeze, S. Torres, J. Seamen, J.F. |
| Copyright Year | 1999 |
| Description | Author affiliation: Sandia Nat. Labs., Albuquerque, NM, USA (Deeney, C.) |
| Abstract | Summary form only given, as follows. The quest to reduce the complexity, cost and risk of higher current accelerators drives the need for implosion times that are longer than the canonical 100 ns of present waterline generators. Experiments have been performed at 100 to 200 ns implosion times on the 10-MA Saturn and the 20 MA Z accelerators. These experiments have shown that 7 to 10 ns FWHM pulses can be produced even at the longest implosion times. The experimental data will be presented along with calculations which indicate that stability, uniformity and plasma opacity are critical to determining the radiation efficiency of these implosions. |
| File Size | 92108 |
| File Format | |
| ISBN | 0780352246 |
| ISSN | 07309244 |
| DOI | 10.1109/PLASMA.1999.829545 |
| Language | English |
| Publisher | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Publisher Date | 1999-06-24 |
| Publisher Place | USA |
| Access Restriction | Subscribed |
| Rights Holder | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Subject Keyword | Wire Saturn Acceleration Laboratories Plasma accelerators Plasma stability Costs US Department of Energy |
| Content Type | Text |
| Resource Type | Article |
| Subject | Atomic and Molecular Physics, and Optics Condensed Matter Physics Electrical and Electronic Engineering |
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