A. H. Sulaiman

A Dynamic Auroral Ionospheric Density Profile Reveals a Planetary-Scale Cavity at Jupiter

Low-altitude measurements above Jupiter’s main auroras have shown the presence of persistent auroral density depletions. This low density regime strongly favors auroral acceleration by inertial Alfvén waves to explain the predominance of energetic (100–1000 keV) broadband electro...

Plasma wave observations from Juno spacecraft at the Jovian bow shock

Recent observations of Jupiter’s bow shock have provided new insights into the energy dissipation mechanisms associated with bow shocks of outer planets. At greater distances from the Sun, the typically increasing super-Alfvénic nature of the solar wind leads to higher-energy bow...