Effects of hot O+ ions on the growth of electromagnetic ion cyclotron waves

Electromagnetic ion cyclotron (EMIC) waves are believed to play a crucial role in the dynamics of the Earth’s magnetosphere. It has been widely accepted that plasma compositions can influence the growth rate of EMIC waves in the inner magnetosphere, but how hot O + ions change the wave growth rate is not well known. In this study, we investigate the impact of ring current O+ concentration on the EMIC growth rate during a specific storm when the O+ ion flux significantly increases. We calculate the growth rate of EMIC waves by using physics-based ion distributions output from the Ring current-Atmosphere interactions Model with Self-Consistent magnetic (B) and Electric (E) fields (RAM-SCBE) model. The percentage of hot O+ is experimentally varied to examine how the maximum EMIC growth rate changes over time and how the global distribution of the maximum EMIC growth rate is affected. We found that the maximum growth rate of H-band appears in the dusk-to-midnight sector near the plasmapause, while O-band is excited at a slightly outer region. With the increase of hot O+ density, the maximum growth rate of H-band EMIC wave is reduced, while that of O-band EMIC wave is increased. Such variation in the maximum EMIC growth rate implies a potential impact on the associated wave-particle interactions and change of the decay rate in the ring current.