The DOI matches its Crossref record; 11 of the 11 references it cites were found in a registry or an index.
MHD simulations of the magnetorotational instability in a shearing box with zero net flux: II. The effect of transport coefficients
Open accessAbstract
Aims.We study the influence of the choice of transport coefficients (viscosity and resistivity) on MHD turbulence driven by the magnetorotational instability (MRI) in accretion disks.
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Citations
Cites
Instability, turbulence, and enhanced transport in accretion disks
Balbus, S. A., & Hawley, J. F. (1998) · Reviews of Modern Physics · doi:10.1103/revmodphys.70.1 · Cited by 2,624
Local Three-dimensional Magnetohydrodynamic Simulations of Accretion Disks
Hawley, J. F., Gammie, C. F., & Balbus, S. A. (1995) · The Astrophysical Journal · doi:10.1086/175311 · Cited by 1,238
II. Spiral Arms as Sheared Gravitational Instabilities
Goldreich, P., & Lynden-Bell, D. (1965) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/130.2.125 · Cited by 945
Simulations of the Small‐Scale Turbulent Dynamo
Schekochihin, A. A., Cowley, S. C., Taylor, S. F., Maron, J. L., & McWilliams, J. C. (2004) · The Astrophysical Journal · doi:10.1086/422547 · Cited by 502
Local Three-dimensional Simulations of an Accretion Disk Hydromagnetic Dynamo
Hawley, J. F., Gammie, C. F., & Balbus, S. A. (1996) · The Astrophysical Journal · doi:10.1086/177356 · Cited by 412
Lesur, G., & Longaretti, P.-Y. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11888.x · Cited by 254
Self-citationFromang, S., & Papaloizou, J. (2007) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20077942 · Cited by 246
Self-citationOn the relevance of subcritical hydrodynamic turbulence to accretion disk transport
Lesur, G., & Longaretti, P.-Y. (2005) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20053683 · Cited by 159
Self-citationTeyssier, R., Fromang, S., & Dormy, E. (2006) · Journal of Computational Physics · doi:10.1016/j.jcp.2006.01.042 · Cited by 138
Self-citationHydrodynamic stability of rotationally supported flows: Linear and nonlinear 2D shearing box results
Umurhan, O. M., & Regev, O. (2004) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20040573 · Cited by 119
Cited by
Hot Accretion Flows Around Black Holes
Yuan, F., & Narayan, R. (2014) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082812-141003 · Cited by 1,529
Protoplanetary disk structures in Ophiuchus
Andrews, S. M., Wilner, D. J., Hughes, A. M., Qi, C., & Dullemond, C. P. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/700/2/1502 · Cited by 709
Dynamics of Protoplanetary Disks
Armitage, P. J. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081710-102521 · Cited by 517
ZONAL FLOWS AND LONG-LIVED AXISYMMETRIC PRESSURE BUMPS IN MAGNETOROTATIONAL TURBULENCE
Johansen, A., Youdin, A., & Klahr, H. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/697/2/1269 · Cited by 386
Metadata
- Authors
- Fromang, S., Papaloizou, J., Lesur, G., & Heinemann, T.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2007-10-02
- Volume
- 476
- Issue
- 3
- Pages
- 1123-1132
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W171251996
- Cited by
- 257
- References
- 11
- FWCI
- 17.31
- Type
- journal article
- Language
- en
- Open access
- green
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- Fromang, S., Papaloizou, J., Lesur, G., & Heinemann, T. (2007). MHD simulations of the magnetorotational instability in a shearing box with zero net flux: II. The effect of transport coefficients. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20077943
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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