Turbulent ambipolar diffusion: numerical studies in two dimensions
<p>Under ideal MHD conditions the magnetic field strength should be correlated with density in the interstellar medium (ISM). However, observations indicate that this correlation is weak. Ambipolar diffusion can decrease the flux-to-mass ratio in weakly ionized media; however, it is generally...
| Egile Nagusiak: | , , , |
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| Formatua: | Journal article |
| Argitaratua: |
American Astronomical Society
2004
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