On Why Disks Generate Magnetic Towers and Collimate Jets
arXiv:astro-ph/0208388 · doi:10.1046/j.1365-8711.2003.06506.x
Abstract
We show that accretion disks with magnetic fields in them ought to make jets provided that their electrical conductivity prevents slippage and there is an ambient pressure in their surroundings. We study equilibria of highly wound magnetic structures. General Energy theorems demonstrate that they form tall magnetic towers whose height grows with every turn at a velocity related to the circular velocity in the accretion disk. The pinch effect amplifies the magnetic pressures toward the axis of the towers whose stability is briefly considered.
13 Pages, LaTex, 4 EPS figures
References in corpus (3)
Cited by in corpus (132)
- Hot Accretion Flows Around Black Holes
- Accretion disc viscosity: how big is alpha?
- Cool Outflows in Galaxies and their Implications
- Magnetically Driven Jets in the Kerr Metric
- Magnetic processes in a collapsing dense core. I Accretion and Ejection
- A new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulence
- The Influence of Magnetic Field Geometry on the Evolution of Black Hole Accretion Flows: Similar Disks, Drastically Different Jets
- Magnetic Braking and Protostellar Disk Formation: The Ideal MHD Limit
- Polarization and structure of relativistic parsec-scale AGN jets
- Outflows and Jets from Collapsing Magnetized Cloud Cores
- Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach
- MHD simulations of jet acceleration from Keplerian accretion disks: the effects of disk resistivity
- Magneto-thermal Disk Wind from Protoplanetary Disks
- The evolution of magnetic tower jets in the laboratory
- Magnetically Arrested Disks and Origin of Poynting Jets: Numerical Study
- Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics
- Modeling jet and outflow feedback during star cluster formation
- A robust numerical scheme for highly compressible magnetohydrodynamics: Nonlinear stability, implementation and tests
- The impact of companions on stellar evolution
- Helical Magnetic Fields Associated with the Relativistic Jets of Four BL Lac Objects
- Magnetic Tower Outflows from a Radial Wire Array Z-pinch
- Magnetic field amplification in turbulent astrophysical plasmas
- Thermalization in Relativistic Outflows and the Correlation between Spectral Hardness and Apparent Luminosity in Gamma-ray Bursts
- The Disc-Jet Symbiosis Emerges: Modeling the Emission of Sagittarius A* with Electron Thermodynamics
- The Proto-neutron Star Phase of the Collapsar Model and the Route to Long-soft Gamma-ray Bursts and Hypernovae
- Plasma Physics of Extreme Astrophysical Environments
- Magnetohydrodynamic models of astrophysical jets
- Magnetic Fields in Astrophysical Jets: From Launch to Termination
- Massive star formation via high accretion rates and early disk-driven outflows
- Magnetic fields during the early stages of massive star formation - II. A generalised outflow criterion
- Stellar Explosions by Magnetic Towers
- Magnetically-driven explosions of rapidly-rotating white dwarfs following Accretion-Induced Collapse
- The Role of Magnetic Fields in Protostellar Outflows and Star Formation
- Simulating the Formation of Massive Protostars: I. Radiative Feedback and Accretion Disks
- Kink instabilities in jets from rotating magnetic fields
- Advection/Diffusion of Large-Scale B-Field in Accretion Disks
- Magnetar-energized supernova explosions and GRB-jets
- Testing Models of Accretion-driven Coronal Heating and Stellar Wind Acceleration for T Tauri Stars
- Relativistic Poynting Jets from Accretion Disks
- Collimated jets from the first core
- Outflows and mass accretion in collapsing dense cores with misaligned rotation axis and magnetic field
- Gamma-Ray Burst Dynamics and Afterglow Radiation from Adaptive Mesh Refinement, Special Relativistic Hydrodynamic Simulations
- The early history of protostellar disks, outflows, and binary stars
- Dynamic and Stagnating Plasma Flow Leading to Magnetic Flux Tube Collimation
- The collapse of a molecular cloud core to stellar densities using radiation non-ideal magnetohydrodynamics
- The Wisconsin Plasma Astrophysics Laboratory
- Structure of Magnetic Tower Jets in Stratified Atmospheres
- Massive Outflows Driven by Magnetic Effects in Star Forming Clouds with High Mass Accretion Rates
- Zooming in on Individual Star Formation: Low- and High-mass Stars
- Three-Dimensional Simulations of Dynamics of Accretion Flows Irradiated by a Quasar
- Using Kinematic Properties of Pre-Planetary Nebulae to Constrain Engine Paradigms
- The First Two Thousand Years of Star Formation
- Jets and outflows of massive protostars - From cloud collapse to jet launching and cloud dispersal
- A universal scaling for short and long gamma-ray bursts: E_{X,iso}-E_{gamma,iso}-E_{pk}
- Magnetic Interaction between Stars and Accretion Disks
- Magnetic Jets from Swirling Disks
- Long-Term Evolution of Slowly Rotating Collapsar in Special Relativistic Magnetohydrodynamics
- From Poloidal to Toroidal: Detection of Well-ordered Magnetic Field in High-mass Proto-cluster G35.2-0.74N
- Magnetically-dominated jets inside collapsing stars as a model for gamma-ray bursts and supernova explosions
- Modeling the inner part of the jet in M87: Confronting jet morphology with theory
- Interpreting the radio/X-ray correlation of black hole sources based on the accretion-jet model
- Modeling astrophysical outflows via the unified Dynamo-Reverse Dynamo mechanism
- GRMHD Simulations of Accreting Neutron Stars with Non-Dipole Fields
- Origin of Misalignments: Protostellar Jet, Outflow, Circumstellar Disc, and Magnetic Field
- On the structure and stability of magnetic tower jets
- Binary Star Formation and the Outflows from their Discs
- Interaction of young stellar object jets with their accretion disk
- A High-Order WENO-based Staggered Godunov-type Scheme with Constrained Transport for Force-free Electrodynamics
- Magnetic inhibition of the recollimation instability in relativistic jets
- Collapse of turbulent massive cores with ambipolar diffusion and hybrid radiative transfer II. Outflows
- Relativistic MHD Simulations of Poynting Flux-Driven Jets
- Global axisymmetric simulations of photoevaporation and magnetically driven protoplanetary disk winds
- The role of initial magnetic field structure in the launching of protostellar jets
- The Effects of Magnetic Fields and Outflow Feedback on the Shape and Evolution of the Density PDF in Turbulent Star-Forming Clouds
- Are molecular outflows around high-mass stars driven by ionization feedback?
- Protostellar outflows with Smoothed Particle Magnetohydrodynamics (SPMHD)
- Modeling disks and magnetic outflows around a forming massive star: I. Investigating the two layer-structure of the accretion disk
- Hot Electromagnetic Outflows. III. Displaced Fireball in a Strong Magnetic Field
- Large-scale dynamics of winds originated from black hole accretion flows: (II) Magnetohydrodynamics
- Experimental demonstration of an inertial collimation mechanism in nested outflows
- Three-Dimensional MHD Simulation of Caltech Plasma Jet Experiment: First Results
- Modeling disks and magnetic outflows around a forming massive star: II. Dynamics of jets from massive protostars
- Three-dimensional magnetohydrodynamical simulations of the morphology of head-tail radio galaxies based on magnetic tower jet model
- Different Modes of Star Formation II: Gas Accretion Phase of Initially Subcritical Star-Forming Clouds
- Structure of magnetic fields in intracluster cavities
- Evidence for bipolar jets from the optical spectra of the prototypical symbiotic star Z Andromedae
- Magnetic field structure of relativistic jets without current sheets
- Jets from main sequence and white dwarf companions during common envelope evolution
- Comparisons and Connections between Mean Field Dynamo Theory and Accretion Disc Theory
- Evolution of Hubble wedges in episodic protostellar outflows
- Persistent mysteries of jet engines, formation, propagation, and particle acceleration: have they been addressed experimentally?
- Laboratory Plasma Dynamos, Astrophysical Dynamos, and Magnetic Helicity Evolution
- FSRQ/BL Lac dichotomy as the magnetized advective accretion process around black holes: a unified classification of blazars
- The impact of episodic outflow feedback on stellar multiplicity and the star formation efficiency
- Jet in jet in M87
- Impact of the disk magnetization on MHD disk wind signature
- New Clues to Jet Launching: The inner disks in radio loud quasars may be more stable
- 3D MHD Simulations of Laboratory Plasma Jets
- Astrophysics in 2006
- Electromagnetic Fields in Jets
- Driving Conditions of Protostellar Outflows in Different Star-Forming Environments
- Coupled axisymmetric pulsar magnetospheres
- Distinguishing Propagation vs. Launch Physics of Astrophysical Jets and the Role of Experiments
- Spin of the M87 black hole
- Estimating the Jet Power of Mrk\,231 During the 2017-2018 Flare
- Toward Coupling Flow Driven and Magnetically Driven Dynamos
- Time Evolution of 3D Disk Formation with Misaligned Magnetic Field and Rotation Axes
- MHD simulations of disk-star interaction
- Influence of the turbulent magnetic pressure on isothermal jet emitting disks
- Decoupling of a supermassive black hole binary from its magnetically arrested circumbinary accretion disk
- Laboratory Studies of Astrophysical Jets
- Dynamics of rising magnetized cavities and UHECR acceleration in clusters of galaxies
- Hyper-Resistive Model of Ultra High Energy Cosmic Ray Acceleration by Magnetically Collimated Jets Created by Active Galactic Nuclei
- Morphologies of protostellar outflows: An ALMA view
- Protostellar Outflows at the EarliesT Stages (POETS) V. The launching mechanism of protostellar winds via water masers
- Polarization of Astrophysical Events with Precessing Jets
- A general relativistic effect in quasi-spherical objects as the possible origin of relativistic jets
- Protostellar Outflows: a window to the past
- Dust-driven Dynamos in Accretion Disks
- Spherically-symmetric, cold collapse: the exact solutions and a comparison with self-similar solutions
- Large jets from small-scale magnetic fields
- A New Interpretation for the Hot Corona in Active Galactic Nuclei
- Self-similar Solution of Hot Accretion Flow with Thermal Conduction and Anisotropic Pressure
- Hadronic Processes, Plasma Evolution and Neutrino Emission in Magnetic Towers of Neutron-Star Merger Remnants
- Modelling magnetically dominated and radiatively cooling jets
- Plasma Pressure Driven Asymmetric Supernovae and Highly Collimated Gamma-Ray Bursts
- Logarithmic Separable Solutions of Force-Free Magnetic Fields in Plane-Parallel and Axial Symmetry
- Interacting Kerr-Newman Electromagnetic Fields
- Star Formation
- Self-similar solution of hot accretion flow: the role of kinematic viscosity coefficient
- On the technique for the recovery of the spectrum of turbulence in astrophysical disks
- The Topology of Canonical Flux Tubes in Flared Jet Geometry