Implications of mean field accretion disc theory for vorticity and magnetic field growth

Monthly Notices of the Royal Astronomical Society

Volumn 323, Issue 2, 2001, Pages 497-505

  Blackman, Eric G ^a,b  

^a UNIVERSITY OF ROCHESTER   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Accretion, accretion discs; Hydrodynamics; Instabilities; MHD; Planets and satellites: formation; Turbulence

Indexed keywords

MEAN FIELD THEORY; SATELLITES; SHEAR FLOW; SHEARING;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; DISK MODEL; MAGNETIC FIELD GROWTH; MEAN-FIELD; PLANETS AND SATELLITES: FORMATION; SCALAR-TRANSPORT; SIMPLE++; TURBULENT VISCOSITY; VORTICITY FIELD;

VORTICITY;

EID: 0042694637     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04225.x     Document Type: Article

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