We present simulation results on evolution development of orbital motion of short-period comets with the revolution period not exceeding 6–7 years, namely come
Using observations from the Michelson Doppler Imager(MDI) onboard Solar and Heliospheric Observatory(SOHO), we develop a computational algorithm to automaticall
We propose that sub-Keplerian accretion belts around stars might launch jets. The sub-Keplerian inflow does not form a rotationally supported accretion disk, bu
The solar transition region(TR) is the temperature regime from roughly 0.02 MK to 0.8 MK in the solar atmosphere. It is the transition layer from the collisiona