activity
20172022
most citedSuccessive Two-sided loop Jets Caused by Magnetic Reconnection between Two adjacent Filamentary Threads

41 citations · 125 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.SR20227 cited

Spectroscopic and Imaging Observations of Spatially Extended Magnetic Reconnection in the Splitting of a Solar Filament Structure

Huidong Hu, Ying D. Liu, Lakshmi Pradeep Chitta +2

On the Sun, Doppler shifts of bidirectional outflows from the magnetic-reconnection site have been found only in confined regions through spectroscopic observations. Without spatia…

astro-ph.SR202211 cited

Analysis of the distribution, rotation and scale characteristics of solar wind switchbacks: comparison between the first and second encounters of Parker Solar Probe

Mingming Meng, Ying D. Liu, Chong Chen +1

The S-shaped magnetic structure in the solar wind formed by the twisting of magnetic field lines is called a switchback, whose main characteristics are the reversal of the magnetic…

physics.space-ph202116 cited

MMS direct observations of kinetic-scale shock self-reformation

Zhongwei Yang, Ying D. Liu, Andreas Johlander +6

Studies of shocks have long suggested that a shock can undergo cyclically self-reformation in a time scale of ion cyclotron period. This process has been proposed as a primary mech…

astro-ph.SR2021

Determination of Solar Wind Angular Momentum and Alfvén Radius from Parker Solar Probe Observations

Ying D. Liu, Chong Chen, Michael L. Stevens +1

As fundamental parameters of the Sun, the Alfvén radius and angular momentum loss determine how the solar wind changes from sub-Alfvénic to super-Alfvénic and how the Sun spins dow…

physics.space-ph2020

PIC simulations of microinstabilities and waves at near-Sun solar wind perpendicular shocks: Predictions for Parker Solar Probe and Solar Orbiter

Zhongwei Yang, Ying D. Liu, Shuichi Matsukiyo +6

Microinstabilities and waves excited at moderate-Mach-number perpendicular shocks in the near-Sun solar wind are investigated by full particle-in-cell (PIC) simulations. By analyzi…

astro-ph.SR202018 cited

Characteristics and Importance of "ICME-in-Sheath" Phenomenon and Upper Limit for Geomagnetic Storm Activity

Ying D. Liu, Chong Chen, Xiaowei Zhao

As an important source for large geomagnetic storms, an "ICME-in-sheath" is a completely shocked interplanetary coronal mass ejection (ICME) stuck in the sheath between a shock and…