Solar Nebula Magnetohydrodynamics
The dynamical state of the solar nebula depends critically upon whether or not the gas is magnetically coupled. The presence of a subthermal field will cause laminar flow to break down into turbulence. Magnetic coupling, in turn, depends upon the ionization fraction of the gas. The inner most region...
| Κύριοι συγγραφείς: | , |
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| Μορφή: | Conference item |
| Έκδοση: |
1999
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