Fast reconnection of magnetic fields in turbulent fluids
Reconnection is the process by which magnetic elds in a conducting uidchange their topology. This process is essential for understanding a wide variety ofastrophysical processes, including stellar and galactic dynamos and astrophysicalturbulence. To account for solar ares, solar cycles, and the stru...
Furkejuvvon:
| Publikašuvnnas: | Revista Mexicana de Astronomía y Astrofísica |
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| Váldodahkkit: | , |
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
Universidad Nacional Autónoma de México
2000
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| Fáttát: | |
| Liŋkkat: | https://www.redalyc.org/articulo.oa?id=57100912 |
| Fáddágilkorat: |
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