Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux

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Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux. / W. Davis, S.; M. Stone, J.; Pessah, Martin Elias.

I: Astrophysical Journal, Bind 713, Nr. 1, 10.04.2010, s. 52-65.

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Harvard

W. Davis, S, M. Stone, J & Pessah, ME 2010, 'Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux', Astrophysical Journal, bind 713, nr. 1, s. 52-65. https://doi.org/10.1088/0004-637X/713/1/52

APA

W. Davis, S., M. Stone, J., & Pessah, M. E. (2010). Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux. Astrophysical Journal, 713(1), 52-65. https://doi.org/10.1088/0004-637X/713/1/52

Vancouver

W. Davis S, M. Stone J, Pessah ME. Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux. Astrophysical Journal. 2010 apr. 10;713(1):52-65. https://doi.org/10.1088/0004-637X/713/1/52

Author

W. Davis, S. ; M. Stone, J. ; Pessah, Martin Elias. / Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux. I: Astrophysical Journal. 2010 ; Bind 713, Nr. 1. s. 52-65.

Bibtex

@article{1a65dbe6737c4a1e8c7858d79b6bdbf7,
title = "Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux",
abstract = "We examine the effects of density stratification on magnetohydrodynamic turbulence driven by the magnetorotational instability in local simulations that adopt the shearing box approximation. Our primary result is that, even in the absence of explicit dissipation, the addition of vertical gravity leads to convergence in the turbulent energy densities and stresses as the resolution increases, contrary to results for zero net flux, unstratified boxes. The ratio of total stress to midplane pressure has a mean of ~0.01, although there can be significant fluctuations on long (>~50 orbit) timescales. We find that the time averaged stresses are largely insensitive to both the radial or vertical aspect ratio of our simulation domain. For simulations with explicit dissipation, we find that stratification extends the range of Reynolds and magnetic Prandtl numbers for which turbulence is sustained. Confirming the results of previous studies, we find oscillations in the large scale toroidal field with periods of ~10 orbits and describe the dynamo process that underlies these cycles.",
keywords = "astro-ph.HE",
author = "{W. Davis}, S. and {M. Stone}, J. and Pessah, {Martin Elias}",
year = "2010",
month = apr,
day = "10",
doi = "10.1088/0004-637X/713/1/52",
language = "English",
volume = "713",
pages = "52--65",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "1",

}

RIS

TY - JOUR

T1 - Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux

AU - W. Davis, S.

AU - M. Stone, J.

AU - Pessah, Martin Elias

PY - 2010/4/10

Y1 - 2010/4/10

N2 - We examine the effects of density stratification on magnetohydrodynamic turbulence driven by the magnetorotational instability in local simulations that adopt the shearing box approximation. Our primary result is that, even in the absence of explicit dissipation, the addition of vertical gravity leads to convergence in the turbulent energy densities and stresses as the resolution increases, contrary to results for zero net flux, unstratified boxes. The ratio of total stress to midplane pressure has a mean of ~0.01, although there can be significant fluctuations on long (>~50 orbit) timescales. We find that the time averaged stresses are largely insensitive to both the radial or vertical aspect ratio of our simulation domain. For simulations with explicit dissipation, we find that stratification extends the range of Reynolds and magnetic Prandtl numbers for which turbulence is sustained. Confirming the results of previous studies, we find oscillations in the large scale toroidal field with periods of ~10 orbits and describe the dynamo process that underlies these cycles.

AB - We examine the effects of density stratification on magnetohydrodynamic turbulence driven by the magnetorotational instability in local simulations that adopt the shearing box approximation. Our primary result is that, even in the absence of explicit dissipation, the addition of vertical gravity leads to convergence in the turbulent energy densities and stresses as the resolution increases, contrary to results for zero net flux, unstratified boxes. The ratio of total stress to midplane pressure has a mean of ~0.01, although there can be significant fluctuations on long (>~50 orbit) timescales. We find that the time averaged stresses are largely insensitive to both the radial or vertical aspect ratio of our simulation domain. For simulations with explicit dissipation, we find that stratification extends the range of Reynolds and magnetic Prandtl numbers for which turbulence is sustained. Confirming the results of previous studies, we find oscillations in the large scale toroidal field with periods of ~10 orbits and describe the dynamo process that underlies these cycles.

KW - astro-ph.HE

U2 - 10.1088/0004-637X/713/1/52

DO - 10.1088/0004-637X/713/1/52

M3 - Journal article

VL - 713

SP - 52

EP - 65

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

ER -

ID: 34383018