NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
2009 ◽
Vol 5
(H15)
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pp. 468-469
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Keyword(s):
AbstractHigh-resolution non-ideal magnetohydrodynamical simulations of the turbulent magnetized ISM, powered by supernovae types Ia and II at Galactic rate, including self-gravity and non-equilibriuim ionization (NEI), taking into account the time evolution of the ionization structure of H, He, C, N, O, Ne, Mg, Si, S and Fe, were carried out. These runs cover a wide range (from kpc to sub-parsec) of scales, providing resolution independent information on the injection scale, extended self-similarity and the fractal dmension of the most dissipative structures.
1988 ◽
Vol 46
◽
pp. 978-979
Keyword(s):
1993 ◽
Vol 51
◽
pp. 972-973
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Keyword(s):
1989 ◽
Vol 47
◽
pp. 330-331
Keyword(s):
Keyword(s):
Keyword(s):
Keyword(s):
2019 ◽
Vol 67
◽
pp. 568-576
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