High accretion rates in magnetised Keplerian discs mediated by a Parker instability driven dynamo

Astronomy and Astrophysics

Volumn 490, Issue 2, 2008, Pages 501-514

  Johansen, A ^a,b   Levin, Y ^a  

^a LEIDEN UNIVERSITY   (Netherlands)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Accretion, accretion disks; Galaxy: center; Instabilities; Magnetohydrodynamics (MHD); Turbulence

Indexed keywords

BUOYANCY; DC GENERATORS; ELECTRIC GENERATORS; FLUID DYNAMICS; GALAXIES; HYDRODYNAMICS; INTERACTIVE DEVICES; MAGNETIC FIELD EFFECTS; MAGNETIC FIELD MEASUREMENT; MAGNETIC FIELDS; MAGNETISM; MAGNETOHYDRODYNAMICS; SATELLITE OBSERVATORIES; TURBULENCE;

ACCRETION DISCS; ACCRETION RATES; ACCRETION, ACCRETION DISKS; AZIMUTHAL FIELDS; AZIMUTHAL MAGNETIC FIELDS; BENDING; BINARY SYSTEMS; EQUILIBRIUM CONFIGURATIONS; FIELD LINES; GALAXY: CENTER; GRAVITY FIELDS; HIGHEST RESOLUTIONS; INSTABILITIES; MAGNETIC; MAGNETIC BUOYANCIES; MAGNETIC FIELD LINES; MAGNETISATION; MAGNETOHYDRODYNAMIC SIMULATIONS; MAGNETOHYDRODYNAMICS (MHD); MAGNETOROTATIONAL INSTABILITIES; SHEAR INSTABILITIES; THERMAL PRESSURES; TRANSITION TO TURBULENCES; VERTICAL FIELDS; YIELDING;

MAGNETIC MATERIALS;

EID: 54549085661     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810385     Document Type: Article

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