A Laboratory Plasma Experiment for Studying Magnetic Dynamics of Accretion Discs and Jets
arXiv:astro-ph/0202380 · doi:10.1046/j.1365-8711.2002.05422.x
Abstract
This work describes a laboratory plasma experiment and initial results which should give insight into the magnetic dynamics of accretion discs and jets. A high-speed multiple-frame CCD camera reveals images of the formation and helical instability of a collimated plasma, similar to MHD models of disc jets, and also plasma detachment associated with spheromak formation, which may have relevance to disc winds and flares. The plasmas are produced by a planar magnetized coaxial gun. The resulting magnetic topology is dependent on the details of magnetic helicity injection, namely the force-free state eigenvalue alpha_gun imposed by the coaxial gun.
accepted for publication in MNRAS
Cited by in corpus (39)
- A fossil origin for the magnetic fields of A-stars and white dwarfs
- On Why Disks Generate Magnetic Towers and Collimate Jets
- Magnetic Tower Outflows from a Radial Wire Array Z-pinch
- Experimental Identification of the Kink Instability as a Poloidal Flux Amplification Mechanism for Coaxial Gun Spheromak Formation
- Stellar Explosions by Magnetic Towers
- Advection/Diffusion of Large-Scale B-Field in Accretion Disks
- Stability Properties of Magnetic Tower Jets
- Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection
- On the jets, kinks, and spheromaks formed by a planar magnetized coaxial gun
- Episodic Magnetic Bubbles and Jets: Astrophysical Implications from Laboratory Experiments
- Dynamic and Stagnating Plasma Flow Leading to Magnetic Flux Tube Collimation
- The Wisconsin Plasma Astrophysics Laboratory
- Structure of Magnetic Tower Jets in Stratified Atmospheres
- Laboratory Space Physics: Investigating the Physics of Space Plasmas in the Laboratory
- Why current-carrying magnetic flux tubes gobble up plasma and become thin as a result
- Magnetically-dominated jets inside collapsing stars as a model for gamma-ray bursts and supernova explosions
- The Particle Content of Extragalactic Jets
- A Numerical Model of Hercules A by Magnetic Tower: Jet/Lobe Transition, Wiggling, and the Magnetic Field Distribution
- HST-Scale 3D simulations of MHD disc winds : A rotating two-component jet structure
- Magnetic Helicity and the Relaxation of Fossil Fields
- Stably stratified magnetized stars in general relativity
- Three-Dimensional MHD Simulation of Caltech Plasma Jet Experiment: First Results
- Experimental investigation of coaxial-gun-formed plasmas injected into a background transverse magnetic field or plasma
- Laboratory modeling of jets from young stars using plasma focus facilities
- Accretion Disks and Dynamos: Toward a Unified Mean Field Theory
- On the magnetic flux problem in star formation
- Vertical Structure of Stationary Accretion Disks with a Large-Scale Magnetic Field
- Enrichment of the dust-to-gas mass ratio in Bondi/Jeans accretion/cloud systems due to unequal changes in dust and gas incoming velocities
- Emergent kink stability of a magnetized plasma jet injected into a transverse background magnetic field
- Persistent mysteries of jet engines, formation, propagation, and particle acceleration: have they been addressed experimentally?
- Laboratory Plasma Dynamos, Astrophysical Dynamos, and Magnetic Helicity Evolution
- The Mochi.LabJet experiment for measurements of canonical helicity injection in a laboratory astrophysical jet
- Magnetohydrodynamic relaxation of AGN ejecta: radio bubbles in the intracluster medium
- Nonthermal ion acceleration by the kink instability in nonrelativistic jets
- Stably stratified stars containing magnetic fields whose toroidal components are much larger than the poloidal ones in general relativity: A perturbation analysis
- Distinguishing Propagation vs. Launch Physics of Astrophysical Jets and the Role of Experiments
- From pulsar scintillations to coronal heating: discontinuities in magnetohydrodynamics
- Toward Coupling Flow Driven and Magnetically Driven Dynamos
- Dust-driven Dynamos in Accretion Disks