Zobrazeno 1 - 10
of 234
pro vyhledávání: '"D. Winske"'
Publikováno v:
Annales Geophysicae, Vol 14, Pp 1-10 (1996)
The electromagnetic proton cyclotron anisotropy instability is excited if the hot proton temperature anisotropy, T⊥h/T\mid\mid h, is sufficiently large compared to unity, where the subscript h denotes the hot protons and the perpendicular and pa
Externí odkaz:
https://doaj.org/article/2692ae9b39734f31b0c51c1cbbc3e689
Autor:
R. S. Dorst, D. B. Schaeffer, A. Le, J. J. Pilgram, C. G. Constantin, S. Vincena, S. K. P. Tripathi, D. Winske, D. Larson, M. Cowee, C. Niemann
Publikováno v:
Physics of Plasmas. 29:082113
The laminar coupling of energy between a laser-produced plasma and a background magnetized plasma was investigated via planar laser induced fluorescence diagnostic and magnetic flux probes. Experiments performed on the Large Plasma Device at the Univ
Autor:
Richard J.H. Smith, J.C. Boguski, Jason Sears, D. Winske, H. Swan, L. Chapdelaine, Thomas Weber, Tom Intrator, J.P. Dunn, K. Gao, T.M. Hutchinson
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3ae3e57ab7bd74feda1077e9994f26e4
https://doi.org/10.2172/1154987
https://doi.org/10.2172/1154987
Akademický článek
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Autor:
D. Winske, J. D. Huba
Publikováno v:
Physics of Plasmas. 5:2305-2316
The evolution of the Rayleigh–Taylor instability in a low β, two-dimensional plasma is studied using a hybrid code and a nonideal magnetohydrodynamic (MHD) code. The Rayleigh–Taylor instability was chosen as a test case because it is an importan
Autor:
K. Lagattuta, D. Winske
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer. 58:703-708
Autor:
D. Winske
Publikováno v:
Physics of Plasmas. 4:2454-2463
Hybrid simulations with kinetic ions and massless fluid electrons are used to investigate the linear and nonlinear behavior of the Rayleigh-Taylor instability in a collisionless, magnetized plasma in slab geometry with the plasma subject to a time va
Publikováno v:
Cometary Plasma Processes
In this paper, recent kinetic simulation studies of cometary bow shocks are reviewed. Cometary shocks are formed due to solar wind mass loading by water group cometary ions. This process is kinetic in nature and varies as a function of the angle betw
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d7eaa8504d72044bc2950ce24523fa5d
https://doi.org/10.1029/gm061p0037
https://doi.org/10.1029/gm061p0037
Autor:
D. Winske
Publikováno v:
Physics of Plasmas. 3:3966-3974
Hybrid simulations with kinetic ions and massless fluid electrons are used to investigate the linear and nonlinear behavior of the magnetized Rayleigh–Taylor instability in slab geometry with the plasma subject to a constant gravity. Three regimes