James R. Beattie
  • Home
  • Featured Science
  • News
  • Collaborators
  • Papers
  • Student Projects
  • Notes
  • Data
  • Recent & Upcoming Talks
    • Example Talk
  • Lecture Notes & Talks
    • The interstellar cascade II - supernova driven turbulence
    • The interstellar cascade I - the world’s largest turbulent MHD box experiment
    • From fast growth to saturation of the intracluster medium dynamo
    • Aspects of magnetic field growth and the turbulent dynamo
  • Blog
    • Off to Lyon and Chateau de Goutelas
    • 🎉 I was a commentator in a CNN article on the Starry Night
    • 🎉 ICM talk at Galaxy Clusters & Radio Relics II, Center for Astrophysics | Harvard & Smithsonian
    • 🎉 10k simulation featured in the Leibniz Supercomputing Centre newsletter for July!
    • 🎉 New Scientist features the 10k MHD simulation in print!
    • 🎉Results from the world's largest MHD turbulence simulation hits the arXiv!
    • ✈️I'm off to Tallahassee for the HEDLA meeting!
  • Student Projects
    • Characterising magnetic field structure across scales - X and O point detection in three dimensions
    • Developing a turbulence-regulated star formation theory in a medium with non-lognormal gas density statistics.
    • Exploring streaming cosmic ray propagation in zoom-in molecular cloud simulations
    • Growth or decay - decaying magnetohydrodynamics meets the turbulent dynamo
    • Investigating compressible and incompressible mode coupling in supersonic turbulent dynamos relevant to the interstellar medium
    • Kinetic helicity and chiral velocity modes in supernova driven turbulence
    • Reconstructing three-dimensional moments from anisotropic two-dimensional fields
    • Supersonic vortices - understanding the building blocks of supersonic, sub-Alfvenic magnetohydrodynamic turbulence
    • The secret life of over-dense regions in interstellar turbulence
    • The transport and flux of magnetic helicity fluctuations
  • Publications
    • Magnetized compressible turbulence with a fluctuation dynamo and Reynolds numbers over a million
    • Taking control of compressible modes: bulk viscosity and the turbulent dynamo
    • Fundamental MHD scales -- II: the kinematic phase of the supersonic small-scale dynamo
    • 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
    • Is The Starry Night Turbulent?
  • Experience
  • Teaching
    • Learn JavaScript
    • Learn Python

🎉 New Scientist features the 10k MHD simulation in print!

Jun 8, 2024·
James R. Beattie
James R. Beattie
· 0 min read
Image credit: Alex Wilkins, New Scientist
Last updated on Jun 8, 2024
Visualization Outreach Science Communication
James R. Beattie
Authors
James R. Beattie
Postdoctoral Research Fellow at Princeton / CITA
← 🎉 10k simulation featured in the Leibniz Supercomputing Centre newsletter for July! Jul 8, 2024
🎉Results from the world's largest MHD turbulence simulation hits the arXiv! May 29, 2024 →

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

Published with Hugo Blox Builder — the free, open source website builder that empowers creators.