@jaztrophysicist A short #dataviz for a forthcoming local communication by the regional supercomputing center CALMIP, to illustrate our recent results on the measurement of turbulent magnetic diffusion at the solar surface.
The convection turbulent velocity field at the solar photosphere, with a resolution of 2500km and a time-sampling of 15 minutes, over a consecutive time-window of 6 days, was computed on the supercomputer based on 4096^2 NASA/SDO images of the photosphere with 45seconds sampling. Images on the right represent the distribution of magnetic fields at the photospheric level of the Sun, also obtained from the SDO MDI instrument. #astrodon #fluids #turbulence #science #ComplexSystems
https://www.aanda.org/articles/aa/full_html/2025/04/aa50476-24/aa50476-24.html