Hall-effect Controlled Gas Dynamics in Protoplanetary Disks: II. Full 3D Simulations toward the Outer Disk
arXiv:1409.2511 · doi:10.1088/0004-637X/798/2/84
Abstract
We perform 3D stratified shearing-box MHD simulations on the gas dynamics of protoplanetary disks threaded by net vertical magnetic field Bz. All three non-ideal MHD effects, Ohmic resistivity, the Hall effect and ambipolar diffusion are included in a self-consistent manner based on equilibrium chemistry. We focus on regions toward outer disk radii, from 5-60AU, where Ohmic resistivity tends to become negligible, ambipolar diffusion dominates over an extended region across disk height, and the Hall effect largely controls the dynamics near the disk midplane. We find that around R=5AU, the system launches a laminar/weakly turbulent magnetocentrifugal wind when the net vertical field Bz is not too weak, as expected. Moreover, the wind is able to achieve and maintain a configuration with reflection symmetry at disk midplane. The case with anti-aligned field polarity (Omega. Bz<0) is more susceptible to the MRI when Bz drops, leading to an outflow oscillating in radial directions and very inefficient angular momentum transport. At the outer disk around and beyond R=30AU, the system shows vigorous MRI turbulence in the surface layer due to far-UV ionization, which efficiently drives disk accretion. The Hall effect affects the stability of the midplane region to the MRI, leading to strong/weak Maxwell stress for aligned/anti-aligned field polarities. Nevertheless, the midplane region is only very weakly turbulent. Overall, the basic picture is analogous to the conventional layered accretion scenario applied to the outer disk. In addition, we find that the vertical magnetic flux is strongly concentrated into thin, azimuthally extended shells in most of our simulations beyond 15AU. This is a generic phenomenon unrelated to the Hall effect, and leads to enhanced zonal flow. Observational and theoretical implications, as well as future prospects are briefly discussed.
arXiv comment19 pages, 14 figures, submitted to ApJ in June
References in corpus (64)
- Theory of Star Formation
- The UMIST database for astrochemistry 2012
- Athena: A New Code for Astrophysical MHD
- Protoplanetary Disk Structures in Ophiuchus
- Wind-driven Accretion in Protoplanetary Disks. I: Suppression of the Magnetorotational Instability and Launching of the Magnetocentrifugal Wind
- Particle Clumping and Planetesimal Formation Depend Strongly on Metallicity
- Radiation-Hydrodynamic Models of X-Ray & EUV Photoevaporating Protoplanetary Discs
- Linear Analysis of the Hall Effect in Protostellar Disks
- Local Magnetohydrodynamical Models of Layered Accretion Disks
- Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux
- Thanatology in Protoplanetary Discs: the combined influence of Ohmic, Hall, and ambipolar diffusion on dead zones
- Time-Evolution of Viscous Circumstellar Disks due to Photoevaporation by FUV, EUV and X-ray Radiation from the Central Star
- The Balbus-Hawley instability in weakly ionised discs
- Disk Winds Driven by Magnetorotational Instability and Dispersal of Proto-Planetary Disks
- Local Study of Accretion Disks with a Strong Vertical Magnetic Field: Magnetorotational Instability and Disk Outflow
- Dust size distributions in coagulation/fragmentation equilibrium: Numerical solutions and analytical fits
- Magnetic fields in protoplanetary disks
- TADPOL: A 1.3 mm Survey of Dust Polarization in Star-forming Cores and Regions
- Assessing Quantitative Results in Accretion Simulations: From Local to Global
- Stellar Activity on the Young Suns of Orion: COUP Observations of K5-7 Pre-Main Sequence Stars
- Exclusion of Cosmic Rays in Protoplanetary Disks: Stellar and Magnetic Effects
- Effect of Ambipolar Diffusion on the Non-linear Evolution of Magnetorotational Instability in Weakly Ionized Disks
- Chemical Processes in Protoplanetary Disks
- Heat and Dust in Active Layers of Protostellar Disks
- Turbulence In the Outer Regions of Protoplanetary Disks. II. Strong Accretion Driven by a Vertical Magnetic Field
- Magnetorotational Instability Driven Accretion in Protoplanetary Disks
- The Effect of the Hall Term on the Nonlinear Evolution of the Magnetorotational Instability: II. Saturation Level and Critical Magnetic Reynolds Number
- The Effect of the Hall Term on the Nonlinear Evolution of the Magnetorotational Instability: I. Local Axisymmetric Simulations
- The structure and dynamics of molecular gas in planet-forming zones: A CRIRES spectro-astrometric survey
- Dead Zone Accretion Flows in Protostellar Disks
- Hall-effect Controlled Gas Dynamics in Protoplanetary Disks: I. Wind Solutions at the Inner Disk
- Chemical Processes in Protoplanetary Disks II. On the importance of photochemistry and X-ray ionization
- Empirical Constraints on Turbulence in Protoplanetary Accretion Disks
- Evidence for Disk Photoevaporation Driven by the Central Star
- Local outflows from turbulent accretion disks
- Magnetic self-organisation in Hall-dominated magnetorotational turbulence
- Surface Layer Accretion in Conventional and Transitional Disks Driven by Far-Ultraviolet Ionization
- Turbulence In the Outer Regions of Protoplanetary Disks. I. Weak Accretion with No Vertical Magnetic Flux
- Wind-driven Accretion in Protoplanetary Disks --- II: Radial Dependence and Global Picture
- Global Simulations of Accretion Disks I: Convergence and Comparisons with Local Models
- Magnetic Flux Concentration and Zonal Flows in Magnetorotational Instability Turbulence
- MHD Simulations of Global Accretion Disks with Vertical Magnetic Fields
- Spatially Resolved Magnetic Field Structure in the Disk of a T Tauri Star
- Molecule survival in magnetized protostellar disk winds. I. Chemical model and first results
- Understanding the origin of the [OI] low-velocity component from T Tauri stars
- Ambipolar Diffusion in the Magnetorotational Instability
- On the Linear Stability of Weakly-Ionized, Magnetized Planar Shear Flows
- Alignment Between Flattened Protostellar Infall Envelopes and Ambient Magnetic Fields
- A Disk-Wind Model for the Near-Infrared Excess Emission in Protostars
- What Is The Numerically Converged Amplitude of MHD Turbulence in Stratified Shearing Boxes?
- Grain Alignment and Polarized Emission from Magnetized T Tauri Disks
- Detection of a Magnetized Disk around a Very Young Protostar
- High resolution spectroscopy of Ne II emission from young stellar objects
- Dead zones as safe-havens for planetesimals: influence of disc mass and external magnetic field
- Efficiency of Particle Trapping in the Outer Regions of Protoplanetary Disks
- The Role of Tiny Grains on the Accretion Process in Protoplanetary Disks
- Disks and Outflows in CO Rovibrational Emission from Embedded, Low-Mass Young Stellar Objects
- Planetesimal Formation in Magnetorotationally Dead Zones: Critical Dependence on the Net Vertical Magnetic Flux
- Stringent Limits on the Polarized Submillimeter Emission from Protoplanetary Disks
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- On the ionisation fraction in protoplanetary disks III. The effect of X-ray flares on gas-phase chemistry
- Turbulent Linewidths in Protoplanetary Disks: Predictions from Numerical Simulations
- Interferometric Upper Limits on Millimeter Polarization of the Disks around DG Tau, GM Aur, and MWC 480
- Magnetorotational instability in magnetic diffusion dominated accretion discs
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- The weakly nonlinear magnetorotational instability in a local geometry
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