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pro vyhledávání: '"Nathaniel D. Hamlin"'
Publikováno v:
IEEE Transactions on Plasma Science. 50:3036-3056
Autor:
Nathaniel D. Hamlin, Charles Seyler
Publikováno v:
IEEE Transactions on Plasma Science. 47:2064-2073
Extended-MHD simulations of power flow along a pulsed-power transmission line are performed in a 2-D axisymmetric geometry, in particular looking at the influence of Hall physics for a transmission line coupled to the liner used in a magnetized liner
Autor:
Nathaniel D. Hamlin, Charles E. Seyler
Publikováno v:
2017 IEEE International Conference on Plasma Science (ICOPS).
Autor:
Nathaniel D. Hamlin, Charles E. Seyler
Publikováno v:
2014 IEEE 41st International Conference on Plasma Sciences (ICOPS) held with 2014 IEEE International Conference on High-Power Particle Beams (BEAMS).
Autor:
William I. Newman, Nathaniel D. Hamlin
Publikováno v:
Newman, WI; & Hamlin, ND. (2014). PRIMITIVE VARIABLE DETERMINATION IN CONSERVATIVE RELATIVISTIC MAGNETOHYDRODYNAMIC SIMULATIONS. SIAM JOURNAL ON SCIENTIFIC COMPUTING, 36(4), B661-B683. doi: 10.1137/140956749. UCLA: Retrieved from: http://www.escholarship.org/uc/item/0s53f84b
In nonrelativistic hydrodynamics and magnetohydrodynamics, conservative integration schemes for the fluid equations of motion are generally employed. The computed quantities, namely, the mass density, (vector) momentum density, and energy density, ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::913fecee19025bc57fe74e5950bf062d
http://www.escholarship.org/uc/item/0s53f84b
http://www.escholarship.org/uc/item/0s53f84b
Autor:
William I. Newman, Nathaniel D. Hamlin
Publikováno v:
Hamlin, ND; & Newman, WI. (2013). Role of the Kelvin-Helmholtz instability in the evolution of magnetized relativistic sheared plasma flows. Physical Review E-Statistical, Nonlinear, and Soft Matter Physics, 87(4). doi: 10.1103/PhysRevE.87.043101. UCLA: Retrieved from: http://www.escholarship.org/uc/item/5r77x3v6
We explore, via analytical and numerical methods, the Kelvin-Helmholtz (KH) instability in relativistic magnetized plasmas, with applications to astrophysical jets. We solve the single-fluid relativistic magnetohydrodynamic (RMHD) equations in conser