A5032241538- Astrophysics and Star Formation Studies
- Stellar, planetary, and galactic studies
- Astrophysical Phenomena and Observations
- Astro and Planetary Science
- High-pressure geophysics and materials
- Cosmology and Gravitation Theories
- Tribology and Lubrication Engineering
- Adhesion, Friction, and Surface Interactions
- Electrostatic Discharge in Electronics
- Magnetic confinement fusion research
- Pulsed Power Technology Applications
- Gyrotron and Vacuum Electronics Research
- Dust and Plasma Wave Phenomena
- Molecular Spectroscopy and Structure
- Ionosphere and magnetosphere dynamics
- Pulsars and Gravitational Waves Research
Lawrence Livermore National Laboratory
2024
Oregon State University
2019
University of Oregon
2012-2015
We have conducted 0D, 1D, 2D, and 3D simulations of an idealized coaxial impedance-matched Marx generator (IMG) []. The 0D calculations were with a four-element circuit model; the highly resolved, fully electromagnetic representations. IMG consists 30 stages distributed axially connected electrically in series. Each stage is powered by two bricks separated 180° parallel. brick comprises opposite-polarity capacitors series single switch. drive internal transmission line terminated resistive...
Views Icon Article contents Figures & tables Video Audio Supplementary Data Peer Review Share Twitter Facebook Reddit LinkedIn Tools Reprints and Permissions Cite Search Site Citation K. Z. Hadley, P. Fernandez, J. N. Imamura, E. Keever, R. Tumblin; Nonaxisymmetric instabilities in self-gravitating disks: Linear quasi-linear regimes. AIP Conference Proceedings 12 September 2012; 1480 (1): 361–363. https://doi.org/10.1063/1.4754387 Download citation file: Ris (Zotero) Reference Manager...
The development of nonaxisymmetric instabilities in polytropic disks surrounding point mass stars was modeled through the linear, quasi-linear and nonlinear regimes to study angular momentum transport that results from hydrodynamic disk instabilities. Significant redistribution occurs on characteristic orbital period disk, defined at maximum density midplane. All modes drove spreading accretion onto central star, but no fission or fragmentation occurred.