The top panel shows IMF Bz at the time during half hours of projected STORM orbit. The second panel shows solar wind density (cyan) and solar wind velocity (x-component) at the time. The lower three panels show simulated X-ray emissivity integrated along the line-of-sight [Kuntz et al 2015], energy flux of diffuse aurora, and simulated ENA flux. The images are observed from projected STORM orbit, especially when STORM is near the north pole.
thestormmission.com 