Turbulent viscosity, magnetic diffusivit
β
L. L. Kitchatinov; V. V. Pipin; G. RΓΌdiger
π
Article
π
1994
π
John Wiley and Sons
π
English
β 738 KB
The old problem of turbulent diffusion is addressed to define the influence of rotation and magnetic fieldthe usual ingredients of astrophysical bodieson the effective transport coefficients. Either rotation and magnetism produce the anisotropy and quenching. The tensorial structures of the diffusiv