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 - I: universality of the turbulent dynamo saturation
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    • The density distribution and physical origins of intermittency in supersonic, highly magnetized turbulence with diverse modes of driving
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    • 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
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✈️I'm off to Tallahassee for the HEDLA meeting!

May 20, 2024·
James R. Beattie
James R. Beattie
· 0 min read
Left-to-right: me, Luca Orusa and Vicente Valenzuela-Villaseca enjoying the sunset in Tallahassee.
Last updated on May 20, 2024
Conference Laboratory Astrophysics
James R. Beattie
Authors
James R. Beattie
Postdoctoral Research Fellow at Princeton / CITA
← 🎉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

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