My primary focus is on the research of accretion disks and the physical processes of planets.
This involves the study of various aspects, such as the formation of planets within planetary disks and the subsequent evolution of their internal structures.
Additionally, I study the propagation and dissipation of tidal waves within planetary interiors, as well as numerous methods in detecting radio emissions from exoplanets.
To gain a comprehensive understanding of these phenomena would require a sophisticated knowledge of orbital dynamics, fluid dynamics, electrodynamics, and magnetohydrodynamics.
Personally, I prefer the pen-and-paper working style, which involves employing techniques like order-of-magnitude estimations, analytical reasoning, and small-scale numerical computations.
Completed a 3-month internship at National Astronomical Observatories (NAOC), Chinese Academy of Sciences (CAS).Detailed responsibilities included:
Conducted research under the supervision of Prof. Xing Wei. The main area of my study is coupling of orbital dynamics and tidal resonances. The study applied Laplace's theory to the study of surface tides in rapidly rotating stars and planets. This model can also be used to explain the tides that occur in the atmospheres of stars and planets or in the oceans of neutron stars. The detailed study:
Computer skills: Python, Matlab
Language: Chinese, English, Japanese