James R. Beattie
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    • Characterising magnetic field structure across scales - X and O point detection in three dimensions
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    • Growth or decay - decaying magnetohydrodynamics meets the turbulent dynamo
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    • Growth or Decay - I: universality of the turbulent dynamo saturation
    • Turbulent diffusion of streaming cosmic rays in compressible, partially ionized plasma
    • The density distribution and physical origins of intermittency in supersonic, highly magnetized turbulence with diverse modes of driving
    • Availability, outage, and capacity of spatially correlated, Australasian free-space optical networks
    • Energy balance and Alfvén Mach numbers in compressible magnetohydrodynamic turbulence with a large-scale magnetic field
    • Magnetized compressible turbulence with a fluctuation dynamo and Reynolds numbers over a million
    • Fundamental scales in the kinematic phase of the turbulent dynamo
    • A multishock model for the density variance of anisotropic, highly magnetized, supersonic turbulence
    • The sonic scale of interstellar turbulence
    • Magnetic field fluctuations in anisotropic, supersonic turbulence
    • Filaments and striations: anisotropies in observed, supersonic, highly magnetized turbulent clouds
    • The relation between the turbulent Mach number and observed fractal dimensions of turbulent clouds
    • The relation between the true and observed fractal dimensions of turbulent clouds
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🎉 ICM talk at Galaxy Clusters & Radio Relics II, Center for Astrophysics | Harvard & Smithsonian

Sep 6, 2024·
James R. Beattie
James R. Beattie
· 0 min read
Image description: my talk title slide!
Last updated on Sep 6, 2024
Conference Talks
James R. Beattie
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James R. Beattie
Postdoctoral Research Fellow at Princeton / CITA
← 🎉 I was a commentator in a CNN article on the Starry Night Sep 18, 2024
🎉 10k simulation featured in the Leibniz Supercomputing Centre newsletter for July! Jul 8, 2024 →

© 2024 James R. Beattie. This work is licensed under CC BY NC ND 4.0

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