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
✦ LIBER ✦
Solar-wind model including the effects of rotation, magnetic fields, and anisotropic heat conduction
✍ Scribed by S. Grzędzielski
- Publisher
- Springer Netherlands
- Year
- 1969
- Tongue
- English
- Weight
- 601 KB
- Volume
- 3
- Category
- Article
- ISSN
- 0004-640X
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