Published August 16, 2022 | Version v3
Journal article Open

Movies for "Hybrid simulations of the cusp and dayside magnetosheath dynamics under quasi-radial interplanetary magnetic fields"

  • 1. UMD
  • 2. NASA GSFC
  • 3. SSI/Trinum Research
  • 4. University of Alabama in Huntsville
  • 5. Laboratoire d'astrophysique de Bordeaux, Univ. Bordeaux, CNRS

Description

rho0_nw and rho0_sw show the time evolution of the density in the northward and southward IMF simulations used in the article submitted to JGR. 

A 175x250x250 subset of the simulation domain is shown, and the inner boundary is represented by the grey hemisphere. 

bz_sw_nw shows the evolution of Bz GSM in the GSM y = 0 plane.

panels_sw_jet2 shows the evolution of the density and dynamic pressure in the quasi-radial southward IMF simulation.

panels_nw_jet shows the evolution of the density and dynamic pressure in the quasi-radial northward IMF simulation.

 

Files

bz_sw_nw.mp4

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