TESTING CONVERGENCE FOR GLOBAL ACCRETION DISKS

Global disk simulations provide a powerful tool for investigating accretion and the underlying magnetohydrodynamic turbulence driven by magneto-rotational instability (MRI). We use the flux-conservative Athena code to conduct a series of experiments on disks having a variety of magnetic topologies t...

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Published inThe Astrophysical journal Vol. 772; no. 2; pp. 1 - 17
Main Authors Hawley, John F, Richers, Sherwood A, Guan, Xiaoyue, Krolik, Julian H
Format Journal Article
LanguageEnglish
Published United States 01.08.2013
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Abstract Global disk simulations provide a powerful tool for investigating accretion and the underlying magnetohydrodynamic turbulence driven by magneto-rotational instability (MRI). We use the flux-conservative Athena code to conduct a series of experiments on disks having a variety of magnetic topologies to determine what constitutes adequate resolution. We develop and apply several resolution metrics: [left angle bracket]Q sub(z)[right angle bracket] and [left angle bracket]Q sub([phi])[right angle bracket], the ratio of the grid zone size to the characteristic MRI wavelength, alpha sub(mag), the ratio of the Maxwell stress to the magnetic pressure, and [left angle bracket]B super(2)R[right angle bracket]/[left angle bracket]B super(2)[phi][right angle bracket], the ratio of radial to toroidal magnetic field energy. For the initial conditions considered here, adequate resolution is characterized by [left angle bracket]Q sub(z)[right angle bracket] [> or =, slanted] 15, [left angle bracket]Q sub([phi])[right angle bracket] [> or =, slanted] 20, alpha sub(mag) approximately 0.45, and [left angle bracket]B super(2)R[right angle bracket]/[left angle bracket]B super(2)[phi][right angle bracket] approximately 0.2. Use of the Harten-Lax-van Leer-Einfeldt flux solver or second-order interpolation can significantly degrade the effective resolution compared to the Harten-Lax-van Leer discontinuities flux solver and third-order interpolation.
AbstractList Global disk simulations provide a powerful tool for investigating accretion and the underlying magnetohydrodynamic turbulence driven by magneto-rotational instability (MRI). Using them to accurately predict quantities such as stress, accretion rate, and surface brightness profile requires that purely numerical effects, arising from both resolution and algorithm, be understood and controlled. We use the flux-conservative Athena code to conduct a series of experiments on disks having a variety of magnetic topologies to determine what constitutes adequate resolution. We develop and apply several resolution metrics: (Q{sub z} ) and (Q{sub {phi}}), the ratio of the grid zone size to the characteristic MRI wavelength, {alpha}{sub mag}, the ratio of the Maxwell stress to the magnetic pressure, and <B{sub R}{sup 2}>/<B{sub {phi}}{sup 2}>, the ratio of radial to toroidal magnetic field energy. For the initial conditions considered here, adequate resolution is characterized by (Q{sub z} ) {>=} 15, (Q{sub {phi}}) {>=} 20, {alpha}{sub mag} Almost-Equal-To 0.45, and <B{sub R}{sup 2}>/<B{sub {phi}}{sup 2}>{approx}0.2. These values are associated with {>=}35 zones per scaleheight H, a result consistent with shearing box simulations. Numerical algorithm is also important. Use of the Harten-Lax-van Leer-Einfeldt flux solver or second-order interpolation can significantly degrade the effective resolution compared to the Harten-Lax-van Leer discontinuities flux solver and third-order interpolation. Resolution at this standard can be achieved only with large numbers of grid zones, arranged in a fashion that matches the symmetries of the problem and the scientific goals of the simulation. Without it, however, quantitative measures important to predictions of observables are subject to large systematic errors.
Global disk simulations provide a powerful tool for investigating accretion and the underlying magnetohydrodynamic turbulence driven by magneto-rotational instability (MRI). We use the flux-conservative Athena code to conduct a series of experiments on disks having a variety of magnetic topologies to determine what constitutes adequate resolution. We develop and apply several resolution metrics: [left angle bracket]Q sub(z)[right angle bracket] and [left angle bracket]Q sub([phi])[right angle bracket], the ratio of the grid zone size to the characteristic MRI wavelength, alpha sub(mag), the ratio of the Maxwell stress to the magnetic pressure, and [left angle bracket]B super(2)R[right angle bracket]/[left angle bracket]B super(2)[phi][right angle bracket], the ratio of radial to toroidal magnetic field energy. For the initial conditions considered here, adequate resolution is characterized by [left angle bracket]Q sub(z)[right angle bracket] [> or =, slanted] 15, [left angle bracket]Q sub([phi])[right angle bracket] [> or =, slanted] 20, alpha sub(mag) approximately 0.45, and [left angle bracket]B super(2)R[right angle bracket]/[left angle bracket]B super(2)[phi][right angle bracket] approximately 0.2. Use of the Harten-Lax-van Leer-Einfeldt flux solver or second-order interpolation can significantly degrade the effective resolution compared to the Harten-Lax-van Leer discontinuities flux solver and third-order interpolation.
Author Richers, Sherwood A
Hawley, John F
Guan, Xiaoyue
Krolik, Julian H
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Snippet Global disk simulations provide a powerful tool for investigating accretion and the underlying magnetohydrodynamic turbulence driven by magneto-rotational...
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StartPage 1
SubjectTerms ACCRETION DISKS
ALGORITHMS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BLACK HOLES
Brackets
BRIGHTNESS
CONVERGENCE
Flux
Initial conditions
Instability
INTERPOLATION
MAGNETIC FIELDS
MAGNETOHYDRODYNAMICS
SIMULATION
Solvers
SYMMETRY
TURBULENCE
WAVELENGTHS
Title TESTING CONVERGENCE FOR GLOBAL ACCRETION DISKS
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