Turbulent Ambipolar Diffusion: Numerical Studies in 2D
Turbulent Ambipolar Diffusion: Numerical Studies in 2D
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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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 thought to be too slow to play a significant role in the IS...
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Turbulent Ambipolar Diffusion: Numerical Studies in 2D
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TN_cdi_proquest_journals_2088798527
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2088798527
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E-ISSN
2331-8422
DOI
10.48550/arxiv.0309306
