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On the reduced mhd for compressible fluids
Turbulence in the di use ionized component of the Interstellar Medium isoften described in terms of the reduced magnetohydrodynamics (RMHD). We showthat this description does not require small gradients in the directions of the ambientmagnetic eld. When the of the plasma is far from unity, the tran...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autors principals: | , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2000
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57100917 |
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