Zobrazeno 1 - 10
of 45
pro vyhledávání: '"Vyacheslav S. Lukin"'
Solar prominences are formed by partially ionized plasma with inter-particle collision frequencies, which generally warrant magnetohydrodynamic treatment. In this work, we explore the dynamical impacts and observable signatures of two-fluid effects i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6290e79592f2d58a59935fc4d5f1d1d4
Publikováno v:
Astronomy & Astrophysics. 650:A181
Solar prominences are formed by partially ionized plasma with inter-particle collision frequencies generally warranting magnetohydrodynamic treatment. In this work we explore the dynamical impacts and observable signatures of two-fluid effects in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c933292cd27f0345bcbf4c38a5cd2fc
https://doi.org/10.1051/0004-6361/202140425
https://doi.org/10.1051/0004-6361/202140425
Solar chromosphere consists of a partially ionized plasma, which makes modeling the solar chromosphere a particularly challenging numerical task. Here we numerically model chromospheric waves using a two-fluid approach with a newly developed numerica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b41dc47767671fb9952df1560fddf76
http://arxiv.org/abs/1905.03559
http://arxiv.org/abs/1905.03559
Autor:
Vyacheslav S. Lukin, Lei Ni
We numerically study magnetic reconnection on different spatial scales and at different heights in the weakly ionized plasma of the low solar atmosphere (around $300-800$~km above the solar surface) within a reactive 2.5 D multi-fluid plasma-neutral
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c22b9732bdd3d688b8300dcce87846c1
http://arxiv.org/abs/1810.09874
http://arxiv.org/abs/1810.09874
Publikováno v:
Astrophys J
Magnetic reconnection in the solar corona is thought to be unstable to the formation of multiple interacting plasmoids, and previous studies have shown that plasmoid dynamics can trigger MHD waves of different modes propagating outward from the recon
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ce493a8f70a8a8064416a4fe7b34aca9
http://arxiv.org/abs/1803.11212
http://arxiv.org/abs/1803.11212
Magnetic reconnection in strongly magnetized regions around the temperature minimum region of the low solar atmosphere is studied by employing MHD-based simulations of a partially ionized plasma within a reactive 2.5D multi-fluid model. It is shown t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5bf29083305bf6f31870292fdad1593d
http://arxiv.org/abs/1712.00582
http://arxiv.org/abs/1712.00582
Publikováno v:
Astronomy & Astrophysics. 630:A79
Waves and shocks traveling through the solar chromospheric plasma are influenced by its partial ionization and weak collisional coupling, and may become susceptible to multi-fluid effects, similar to interstellar shock waves. In this study, we consid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f864e6f450d88730e5c5a264e7243923
https://doi.org/10.1051/0004-6361/201935844
https://doi.org/10.1051/0004-6361/201935844
Autor:
A. Kirk, J. Horacek, C. D. Challis, I. Klimek, W. A. Peebles, K. Imada, W. A. Gracias, H. R. Wilson, A. W. Morris, L. Piron, K Tani, M. Wischmeier, Sean Conroy, D. A. Ryan, M. O’Brien, F. Arese Lucini, Fabio Riva, Ryota Imazawa, Sandra C. Chapman, Anders Nielsen, P. Cahyna, Nick Walkden, Michael Barnes, I. Fitzgerald, C. Gurl, G. Fishpool, A. Patel, Takuma Yamada, M. Cecconello, M. Turnyanskiy, Ben F. McMillan, A. R. Field, G. Cunningham, Y. Liu, T.R. Barrett, F. J. Casson, Michael F. J. Fox, M. Cox, G. Naylor, A.J. Thornton, Matthew Carr, Nicolas Fedorczak, R. Scannell, L. Pangione, L. Garzotti, N. C. Hawkes, Hiroshi Tanabe, T. Farley, Yasushi Ono, M. Evans, Gen Motojima, Daniel Dunai, T. O'Gorman, S. Saarelma, William Dorland, H. F. Meyer, G. McArdle, B. Huang, E. Havlickova, T. Watanabe, Michiaki Inomoto, R. O. Dendy, Paolo Ricci, Edmund Highcock, F. van Wyk, H. Leggate, Matthias Komm, Jens Madsen, Alexander Schekochihin, S. A. Silburn, I. T. Chapman, S.M. Kaye, Hajime Tanaka, Jeppe Olsen, F. Militello, S. D. Pinches, R. V. Perez, D. Harting, K. G. McClements, Jarrod Leddy, C. M. Roach, Roddy G. L. Vann, Luke Easy, Walter Guttenfelder, Patrick Tamain, Benjamin Daniel Dudson, M. G. O'Mullane, John Omotani, W. A. Cooper, B. Lloyd, Felix I. Parra, K. J. Gibson, EUROfusion Mst Team, S. Cardnell, N. J. Conway, O. M. Jones, W. Lai, J. Young, S. S. Henderson, Brendan M. Crowley, Romualdo Martín, Neal Crocker, A. Meakins, A. V. Danilov, Ray M. Sharples, D. L. Keeling, M. Gorelenkova, J. Simpson, J. Hollocombe, J. Adamek, Bogdan Hnat, N. Ben Ayed, L Kogan, Matthew Reinke, M. Valovic, J. R. Harrison, Bruce Lipschultz, Vladimir Shevchenko, Clive Michael, J. Storrs, M. Romanelli, M. Price, S. E. Sharapov, John Howard, J. Mailloux, N. Thomas-Davies, D. Muir, Stanislas Pamela, David Dickinson, James W. Bradley, M. Kocan, J. Chorley, Philippa Browning, H. P. Summers, Yuichi Takase, Vyacheslav S. Lukin, G. P. Maddison, J. Milnes, Keii Gi, L. Appel, Adam Stanier, Daniel Thomas, S. Allan, Ivan Lupelli, Young-chul Ghim, D. F. Howell, J. C. Hillesheim, S.W. Lisgo, A. N. Saveliev, David Taylor, W. Boeglin, Kazutake Kadowaki, J. Brunner, C. Ham, R. J. Akers, D. S. Darrow, B. Lomanowski, T. C. Hender, S. Elmore, Mast Team, Simon Freethy, S. Zoletnik, Kouji Shinohara
Publikováno v:
NUCLEAR FUSION
Nuclear Fusion
Nuclear fusion, 2016, Vol.57(10), pp.102007 [Peer Reviewed Journal]
Nuclear Fusion
Nuclear fusion, 2016, Vol.57(10), pp.102007 [Peer Reviewed Journal]
New results from MAST are presented that focus on validating models in order to extrapolate to future devices. Measurements during start-up experiments have shown how the bulk ion temperature rise scales with the square of the reconnecting field. Dur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d4cbc811b670e3be0e5a928793f091b
http://arxiv.org/abs/1611.06047
http://arxiv.org/abs/1611.06047
Kinetic simulations have demonstrated that three-dimensional reconnection in collisionless regimes proceeds through the formation and interaction of magnetic flux ropes, which are generated due to the growth of tearing instabilities at multiple reson
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2befcf55e59badb6330ee1fb4eb0d18c
http://arxiv.org/abs/1601.07220
http://arxiv.org/abs/1601.07220
Publikováno v:
Journal of Computational Physics. 231:2963-2976
The truncation of large physical domains to concentrate computational resources is necessary or desirable in simulating many natural and man-made plasma phenomena. Three open boundary condition (BC) methods for such domain truncation of dissipative m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::736f13e13dab4467ccb5d991ffb3bb1b
https://doi.org/10.1016/j.jcp.2012.01.003
https://doi.org/10.1016/j.jcp.2012.01.003