Parallel simulations of hall-Mhd plasmas
Plasma processes such as magnetic reconnection, turbulent regimes or dynamo-generated magnetic fields, are well studied within the framework of one-fluid magnetohydrodynamics (MHD). However, there are processes such as the Hall current, which are not covered by the MHD description. The Hall effect i...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
2006
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 04957caa a22007697a 4500 | ||
|---|---|---|---|
| 001 | PAPER-21873 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250430104600.0 | ||
| 008 | 190411s2006 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-33749005655 | |
| 030 | |a SPSRA | ||
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Gómez, Daniel Osvaldo | |
| 245 | 1 | 0 | |a Parallel simulations of hall-Mhd plasmas |
| 260 | |c 2006 | ||
| 270 | 1 | 0 | |m Gómez, D.; Instituto de Astronomí A y Física Del Espacio (IAFE), Buenos Aires, Argentina; email: dgomez@df.uba.ar |
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| 504 | |a Craig, I.J.D., Watson, P.G., (2003) Solar Phys., 214, p. 130 | ||
| 504 | |a Dorelli, J.C., (2003) Phys. Plasmas, 10, p. 3310 | ||
| 504 | |a Dorelli, J.C., Birn, J., (2003) J. Geophys. Res., 108, p. 1133 | ||
| 504 | |a Ma, Z., Bhattacharjee, A., (2001) J. Geophys. Res., 106, p. 3773 | ||
| 504 | |a Mininni, P.D., Gómez, D.O., Mahajan, S.M., (2002) Astrophys. J. Lett., p. 81 | ||
| 504 | |a Mininni, P.D., Gómez, D.O., Mahajan, S.M., (2003) Astrophys. J., 587, p. 472 | ||
| 504 | |a Mozer, F., Bale, S., Phan, T.D., (2002) Phys. Rev. Lett., 89, p. 015002 | ||
| 504 | |a Priest, E.R., (1984) Magnetic Reconnection in Space and Laboratory Plasmas, Geophys. Monogr. Ser., 30, p. 63. , Hones, E. W. (ed.) | ||
| 504 | |a Sano, T., Stone, J.M., (2002) Astrophys. J., 570, p. 314 | ||
| 504 | |a Smith, D., Ghosh, S., Dmitruk, P., Matthaeus, W.H., (2004) Geophys. Res. Lett., 31, pp. L02805 | ||
| 504 | |a Sonnerup, B.U.O., (1981) J. Geophys. Res., 86, p. 10049 | ||
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| 504 | |a Yakovlev, D.G., Urpin, V.A., (1980) Astr. Zh., 57, p. 526 | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a Plasma processes such as magnetic reconnection, turbulent regimes or dynamo-generated magnetic fields, are well studied within the framework of one-fluid magnetohydrodynamics (MHD). However, there are processes such as the Hall current, which are not covered by the MHD description. The Hall effect is known to be relevant for the dynamics of several astrophysical plasmas, such as the interstellar medium, the early universe, or the solar wind at 1 AU. While the relevance of Hall currents in magnetic reconnection is intensively being studied (specially in connection with reconnection events at the Earth's magnetopause and magnetotail), their role on turbulent regimes or on dynamo mechanisms is mostly unknown. We report results from parallel simulations of the incompressible Hall-MHD equations in 21÷2 and three dimensions to quantitatively investigate the role of Hall currents in different problems, such as magnetic reconnection in 21÷2 dimensions, the dynamo generation of magnetic fields in three-dimensional simulations, or the relaxation to stationary turbulent regimes. © Springer 2006. |l eng | |
| 593 | |a Instituto de Astronomí A y Física Del Espacio (IAFE), Buenos Aires, Argentina | ||
| 593 | |a Department of Physics, University of Buenos Aires, Buenos Aires, Argentina | ||
| 690 | 1 | 0 | |a MAGNETIC RECONNECTION |
| 690 | 1 | 0 | |a MHD |
| 690 | 1 | 0 | |a MHD DYNAMO |
| 690 | 1 | 0 | |a TURBULENCE |
| 690 | 1 | 0 | |a ELECTRIC CURRENTS |
| 690 | 1 | 0 | |a HALL EFFECT |
| 690 | 1 | 0 | |a MAGNETIC FIELDS |
| 690 | 1 | 0 | |a MAGNETIC PROPERTIES |
| 690 | 1 | 0 | |a PLASMAS |
| 690 | 1 | 0 | |a COMPUTER SIMULATION |
| 690 | 1 | 0 | |a EARTH (PLANET) |
| 690 | 1 | 0 | |a MAGNETOHYDRODYNAMICS |
| 690 | 1 | 0 | |a SOLAR WIND |
| 690 | 1 | 0 | |a TURBULENCE |
| 690 | 1 | 0 | |a MAGNETIC RECONNECTION |
| 690 | 1 | 0 | |a MAGNETOHYDRODYNAMIC DYNAMO |
| 690 | 1 | 0 | |a STATIONARY TURBULENT REGIMES |
| 690 | 1 | 0 | |a DYNAMO MECHANISMS |
| 690 | 1 | 0 | |a HALL CURRENT |
| 690 | 1 | 0 | |a MAGNETOHYDRODYNAMICS |
| 690 | 1 | 0 | |a PLASMA FLOW |
| 773 | 0 | |d 2006 |g v. 122 |h pp. 231-238 |k n. 1-4 |p Space Sci Rev |x 00386308 |w (AR-BaUEN)CENRE-6897 |t Space Science Reviews | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-33749005655&doi=10.1007%2fs11214-006-7287-y&partnerID=40&md5=c4e45e05587e11199669a80afe9c8212 |y Registro en Scopus |
| 856 | 4 | 0 | |u https://doi.org/10.1007/s11214-006-7287-y |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_00386308_v122_n1-4_p231_Gomez |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00386308_v122_n1-4_p231_Gomez |y Registro en la Biblioteca Digital |
| 961 | |a paper_00386308_v122_n1-4_p231_Gomez |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/article |a info:ar-repo/semantics/artículo |b info:eu-repo/semantics/publishedVersion | ||
| 999 | |c 82826 | ||