Fast acceleration of Ring Current Ions by ULF waves (Invited)

Friday, 5 September 2014: 2:20 PM
Regency Ballroom (Hyatt Regency)
Qiugang Zong, Peking University, Beijing, China
Abstract:
We have investigated the response of the Earth’s ring current ions including oxygen ions to ULF waves induced by interplanetary shocks. Both Earth’s ring current ions -- hydrogen and oxygen ions are found to be accelerated significantly with their temperature enhanced by a factor of two and three immediately after the shock arrival respectively. Multiple energy dispersion signatures of ring current ions were found in the parallel and anti-parallel direction to the magnetic field immediately after the interplanetary shock impact. The energy dispersions in the anti-parallel direction preceded those in the parallel direction. Multiple dispersion signatures can be explained by the flux modulations of local plasmaspheric ions (rather than the ions from the Earth’s ionosphere) by ULF waves. It is found that both cold plasmaspheric plasma and hot thermal ions (10 eV to 40 keV) are accelerated and decelerated with the various phases of ULF wave electric field. We then demonstrate that ion acceleration due to the interplanetary shock compression on the

Earth’s magnetic field is rather limited, whereas the major contribution to acceleration comes from the electric field carried by ULF waves via drift-bounce resonance for both the hydrogen and oxygen ions. The integrated hydrogen and oxygen ion flux with the poloidal

mode ULF waves are highly coherent (>0.9) whereas the coherence with the toroidal mode ULF waves is negligible, implying that the poloidal mode ULF waves are much more efficient in accelerating hydrogen and oxygen ions in the inner magnetosphere than the toroidal mode ULF waves.