Abstract
Magnetic fields play an important role in astrophysics and often dominate the behavior of ionized media. Their influence is carried out by hydro-magnetic (MHD) waves which efficiently propagate perturbations, ensure a turbulent pressure or may even cause the development of instabilities (Arons & Max, 1975).
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Arons, J. & Max, C.E., 1975, ApJ. Lett. 196, L77
Kulsrud, R. & Pearce, W., 1969, ApJ. 156, 445
Stone, J.M. & Norman, M.L., 1992, ApJSS. 80, 753
Tagger, M., Falgarone, E., & Shukurov, A., 1995, A& A. 299, 940
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© 1999 Springer Science+Business Media Dordrecht
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Franqueira, M., Tagger, M., De Castro, A.I.G. (1999). Simulation of the Ambipolar Filamentation of Turbulent Magnetic Fields. In: Miyama, S.M., Tomisaka, K., Hanawa, T. (eds) Numerical Astrophysics. Astrophysics and Space Science Library, vol 240. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4780-4_38
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DOI: https://doi.org/10.1007/978-94-011-4780-4_38
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