2023/08/04 by Andrew Hillier, Hillier, Andrew, I. Arregui +3 · 2 citations
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #FOS: Physical sciences #Fluid Dynamics (physics.flu-dyn) #Geomagnetism and Paleomagnetism Studies #Ionosphere and magnetosphere dynamics #Solar and Space Plasma Dynamics #Solar and Stellar Astrophysics (astro-ph.SR)
paper · pdf · doi:10.48550/arxiv.2308.02217
openalex publication_date 2023/08/04 · openalex created_date 2023/08/08 · openalex updated_date 2026/07/28
File is an IDL save file containing the data needed to reproduce the figures from Hillier, Arregui and Matsumoto (2024). This contains the x, y, z, and t axes of the simulation, the 2D density field (called density) at z=10, the 2D x-component of the velocity (called vx), The kinetic energy density of the x and y velocity field at z =10 for t=35.2 (called KEt352), the magnetic energy density of the x and y components of the magnetic field at z=0 for t=35.2 (called MEt352), the total internal energy of the simulation domain varying over time (called Einternal) , the z variation of the kinetic energy at two times given by the 150 and 200th element of the t array in a tube (called tubeke), the z variation of the magnetic energy at two times given by the 150 and 200th element of the t array in a tube (called tubeme), the shear layer density model for a density contrast of 1 to 3 calculated from the model of Hillier nad Arregui (2019) (called modeldensity), the mass above a given density threshold for the density field model density (called mT)