Heliosphere =========== 2D slice animations of the heliospheric MHD solution. Each row shows one quantity for equatorial and meridional cuts. For time-dependent runs the MHD solution evolves each frame, while for steady-state runs the background is fixed and spacecraft positions change through it. Density and radial field are scaled by :math:`r^2` to remove the geometric :math:`1/r^2` falloff, revealing intrinsic structure in the solar wind. .. admonition:: Run :class: note **bgtest_superlowres** — CR2121, MAST3, Steady-State ---- .. raw:: html