MHD Turbulence: Scaling Laws and Astrophysical Implications
- 28 February 2003
- book chapter
- Published by Springer Nature
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- Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud ModelsThe Astrophysical Journal, 2001
- The small-scale structure in interstellar H i: a resolvable puzzleMonthly Notices of the Royal Astronomical Society, 2000
- Mean magnetic field renormalization and Kolmogorov’s energy spectrum in magnetohydrodynamic turbulencePhysics of Plasmas, 1999
- Observational constraints on the dynamics of the interplanetary magnetic field dissipation rangeJournal of Geophysical Research, 1998
- Quasi‐linear Theory of Cosmic Ray Transport and Acceleration: The Role of Oblique Magnetohydrodynamic Waves and Transit‐Time DampingThe Astrophysical Journal, 1998
- Diffuse Ionised Gas in Edge-on GalaxiesPublications of the Astronomical Society of Australia, 1998
- Nearly incompressible fluids. II: Magnetohydrodynamics, turbulence, and wavesPhysics of Fluids A: Fluid Dynamics, 1993
- Forbidden S II H-alpha intensity ratios in faint, extended H II regions and the origin of the interstellar emission-line backgroundThe Astrophysical Journal, 1988
- Turbulent velocity structure in interstellar cloudsThe Astrophysical Journal, 1984
- The structure of isotropic turbulence at very high Reynolds numbersJournal of Fluid Mechanics, 1959