Trapping solids at the inner edge of the dead zone: 3-D global MHD simulations

Astronomy and Astrophysics

Volumn 515, Issue 8, 2010, Pages

  Dzyurkevich, N ^a   Flock, M ^a   Turner, N J ^a   Klahr, H ^a   Henning, Th ^a  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Accretion; Accretion disks; Instabilities; Magnetohydrodynamics; Methods: numerical; Planets and satellites: formation; Turbulence

Indexed keywords

COAGULATION; DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); IONIZATION OF GASES; MAGNETIC FIELDS; MAGNETIC MATERIALS; MAGNETOHYDRODYNAMICS; PLANETS; REYNOLDS NUMBER; SATELLITES; THREE DIMENSIONAL; TURBULENCE;

ACCRETION; ACCRETION DISKS; ACTIVE REGIONS; ACTIVE ZONE; AZIMUTHAL MAGNETIC FIELDS; COAGULATION PROCESS; DEAD ZONES; GLOBAL MHD SIMULATION; MAGNETIC DIFFUSIVITY; MEAN MAGNETIC FIELD; METHODS: NUMERICALS; PLANETS AND SATELLITES: FORMATION; PROTOPLANETARY DISKS; RADIAL STRUCTURE; RESISTIVITY DISTRIBUTIONS; REYNOLDS STRESS; SHARP INCREASE; SOLID MATERIAL; SOLID PARTICLES; STEADY STATE; SURFACE DENSITY; TRANSITION RADIUS; TURBULENT PROPERTIES; YOUNG STARS;

NUMERICAL METHODS;

EID: 77953366629     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912834     Document Type: Article

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