35 citations · 227 across the 15 of their papers we have counts for
15 papers
Influence of Solar Polar Magnetic Fields on the Propagation of Coronal Mass Ejection
Xiao Zhang, Liping Yang, Xueshang Feng +9
Understanding the propagation of coronal mass ejections (CMEs) through interplanetary space is essential for space weather forecasting. Due to observational limitations, measuremen…
Scaling anisotropy with stationary background field in the near-Sun solar wind turbulence
Honghong Wu, Jiansen He, Shiyong Huang +3
The scaling of magnetic fluctuations provides crucial information for the understanding of solar wind turbulence. However, the observed magnetic fluctuations contain not only turbu…
On the scaling and anisotropy of two subranges in the inertial range of solar wind turbulence
Honghong Wu, Jiansen He, Liping Yang +3
Intermittency and anisotropy are two important aspects of plasma turbulence, which the solar wind provides a natural laboratory to investigate. However, their forms and nature are…
Large Amplitude Switchback Turbulence: Possible Magnetic Velocity Alignment Structures
Honghong Wu, Chuanyi Tu, Xin Wang +1
Switchbacks are widely acknowledged phenomena observed by the Parker Solar Probe and appear to occur in patches. Previous studies focused on the fluctuations at the magnetic revers…
Encounter of Parker Solar Probe and a Comet-like Object During Their Perihelia: Model Predictions and Measurements
Jiansen He, Bo Cui, Liping Yang +15
Parker Solar Probe (PSP) aims at exploring the nascent solar wind close to the Sun. Meanwhile, PSP is also expected to encounter small objects like comets and asteroids. In this wo…
Isotropic Scaling Features Measured Locally in the Solar Wind Turbulence with Stationary Background Field
Honghong Wu, Chuanyi Tu, Xin Wang +3
The scaling anisotropy is crucial to interpret the nonlinear interactions in solar wind turbulence. Previous observations provide diverse results and the structure function analyse…
Energy Supply for Heating the Slow Solar Wind Observed by Parker Solar Probe between 0.17 and 0.7 au
Honghong Wu, Chuanyi Tu, Xin Wang +2
Energy supply sources for the heating process in the slow solar wind remain unknown. The Parker Solar Probe (PSP) mission provides a good opportunity to study this issue. Recently,…
Fast Magnetic Reconnection with Turbulence in High Lundquist Number Limit
Yang Liping, Li Hui, Guo Fan +5
We use extensive 3D resistive MHD simulations to study how large-scale current sheets will undergo fast reconnection in the high Lundquist number limit (above ), whe…
Possible Generation Mechanism for Compressional Alfvénic Spikes as Observed by Parker Solar Probe
Jiansen He, Xingyu Zhu, Liping Yang +4
The solar wind is found by Parker Solar Probe (PSP) to be abundant with Alfvénic velocity spikes and magnetic field kinks. Temperature enhancement is another remarkable feature ass…
Multi-scale Pressure-balanced Structures in Three-dimensional Magnetohydrodynamic Turbulence
Liping Yang, Jiansen He, Chuanyi Tu +6
Observations of solar wind turbulence indicate the existence of multi-scale pressure-balanced structures (PBSs) in the solar wind. In this work, we conduct a numerical simulation t…
Origin of Both the Fast Hot Jet and the Slow Cool Jet from Magnetic Flux Emergence and Advection in the Solar Transition Region
Liping Yang, Hardi Peter, Jiansen He +4
In the solar atmosphere, the jets are ubiquitous and found to be at various spatia-temporal scales. They are significant to understand energy and mass transport in the solar atmosp…
A Numerical Investigation of the Recurrent High-speed Jets as a Possibility of Solar Wind Origin
Liping Yang, Jiansen He, Hardi Peter +5
In the solar atmosphere, jets are prevalent and they are significant for the mass and energy transport. Here we conduct numerical simulations to investigate the mass and energy con…
Formation of Rotational Discontinuities in Compressive three-dimensional MHD Turbulence
Liping Yang, Lei Zhang, Jiansen He +6
Measurements of solar wind turbulence reveal the ubiquity of discontinuities. In this study, we investigate how the discontinuities, especially rotational discontinuities (RDs), ar…
Occurrence Rates and Heating Effects of Tangential and Rotational Discontinuities as Obtained from Three-dimensional Simulation of Magnetohydrodynamic Turbulence
Lei Zhang, Jiansen He, Chuanyi Tu +4
In solar wind, magnetohydrodynamic (MHD) discontinuities are ubiquitous and often found to be at the origin of turbulence intermittency. They may also play a key role in the turbul…
Numerical Simulation of Superhalo Electrons Generated by Magnetic Reconnection in the Solar Wind Source Region
L. -P. Yang, L. -H. Wang, J. -S. He +4
Superhalo electrons appear to be continuously present in the interplanetary medium, even at very quiet times, with a power-law spectrum at energies above 2 keV. Here we numer…