Physics
Scientific paper
Nov 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..106...77s&link_type=abstract
Icarus, vol. 106, p. 77
Physics
23
Solar Corona, Angular Momentum, Dynamo Theory, Accretion Disks, Magnetohydrodynamics, Kinematic Equations, Ionization, Stellar Envelopes, Lorentz Force, Stress Tensors
Scientific paper
The present investigation of the solar nebula in view of a steady-state accretion disk model, while establishing the criteria for a plausible nebular dynamo, reveals a nebular magnetic gap where ionization is insufficient for gas-magnetic field coupling. It is established, on the basis of dynamical constraints, that the magnetic field thus generated saturates at a strength equalling equiapartition with the turbulence's kinetic energy. The influence exerted by Maxwell stresses due to both large- and small-scale magnetic fields is discussed.
Reyes-Ruiz Mauricio
Stepinski Tomasz F.
Vanhala Harri A. T.
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