4 papers
Optimization Algorithm for Determining the Source Surface Radius Based on Parker Solar Probe in situ Measurements from Encounters 1 to 19
Shiouhe Wang, Fang Shen, Yi Yang +2
The Potential Field Source Surface (PFSS) extrapolation is a method for estimating the large scale coronal magnetic field from photospheric magnetograms. The source surface serves…
Imaging magnetically driven astrospheres: a forward modelling approach
Ziqi Wu, Tom Van Doorsselaere, Jiansen He +5
An astrosphere is a vast, tailed bubble-like volume around a star, formed through the interaction between the stellar magnetic field, the stellar wind, and the interstellar medium…
A Non-Spherical Model for the Solar Coronal Magnetic Field
Ziqi Wu, Jiansen He, Chuanpeng Hou +7
The coronal magnetic field plays a fundamental role in governing coronal activities, driving space-weather events, and shaping the heliosphere. Due to a lack of direct observations…
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…