Area of research
Astronomy and Astrophysics · Geophysics
Research interest
Research interests include Physics, Electron, Van Allen radiation belt, Magnetosphere, Chorus, and Amplitude.
Acceleration of Electrons and Ions by an “Almost” Astrophysical Shock in the Heliosphere
Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum
Cross-scale physics and the acceleration of particles in collisionless plasmas throughout the Heliosphere and beyond: III. Radiation belts
A Climatology of Long‐Duration High 2‐MeV Electron Flux Periods in the Outer Radiation Belt
Switchbacks as signatures of magnetic flux ropes generated by interchange reconnection in the corona
Phase Decoherence Within Intense Chorus Wave Packets Constrains the Efficiency of Nonlinear Resonant Electron Acceleration
A Census of Magnetospheric Electrons From Several eV to 30 keV
Analytical Chorus Wave Model Derived from Van Allen Probe Observations
Time Scales for Electron Quasi‐linear Diffusion by Lower‐Band Chorus Waves: The Effects of <i>ω</i><sub>pe</sub>/<i>Ω</i><sub>ce</sub> Dependence on Geomagnetic Activity
Solitary Waves Across Supercritical Quasi‐Perpendicular Shocks
Spatial Extent and Temporal Correlation of Chorus and Hiss: Statistical Results From Multipoint THEMIS Observations
Synthetic Empirical Chorus Wave Model From Combined Van Allen Probes and Cluster Statistics
Electron‐acoustic solitons and double layers in the inner magnetosphere
Electron Scattering by High-frequency Whistler Waves at Earth’s Bow Shock
Diffusive scattering of electrons by electron holes around injection fronts
Oblique Whistler-Mode Waves in the Earth’s Inner Magnetosphere: Energy Distribution, Origins, and Role in Radiation Belt Dynamics
Wave-induced loss of ultra-relativistic electrons in the Van Allen radiation belts
Fast dropouts of multi‐MeV electrons due to combined effects of EMIC and whistler mode waves
Exclusion principle for very oblique and parallel lower band chorus waves
Nonlinear local parallel acceleration of electrons through Landau trapping by oblique whistler mode waves in the outer radiation belt
Empirical model of lower band chorus wave distribution in the outer radiation belt
The quasi‐electrostatic mode of chorus waves and electron nonlinear acceleration
Evidence of stronger pitch angle scattering loss caused by oblique whistler‐mode waves as compared with quasi‐parallel waves