activity
20242026
collaborators

6 papers

astro-ph.SR2026

A Major Geomagnetic Storm in 2024 October Linked to Sympathetic CME--Prominence Eruptions

Rui Wang, Huidong Hu, Xiaowei Zhao +11

Improving predictions of the geomagnetic impact of coronal mass ejections (CMEs) requires understanding how solar source properties relate to in-situ measurements at Earth. However…

physics.space-ph2026

Proton Temperature Anisotropy Across Interplanetary Shocks: A Statistical Analysis with WIND observations

Zeping Jin, Lingling Zhao, Xingyu Zhu +6

Interplanetary (IP) shocks efficiently modify the proton temperature anisotropy of the solar wind. Analyzing ~800 IP shocks observed by the Wind spacecraft from 1997-2024, we prese…

physics.space-ph2025

Lateral Deformation of Large-scale Coronal Mass Ejections during the Transition from Non-radial to Radial Propagation

Huidong Hu, Chong Chen, Yiming Jiao +4

Many coronal mass ejections (CMEs) initially propagate non-radially, and then transition to radial propagation in the corona. This directional transition is a significant process t…

astro-ph.SR2025

Inertial-range Turbulence Anisotropy of the Young Solar Wind from Different Source Regions

Wenshuai Cheng, Ming Xiong, Yiming Jiao +4

We investigate the wavevector and variance anisotropies in the inertial range of the young solar wind observed by the Parker Solar Probe (PSP). Using the first 19 encounters of PSP…

astro-ph.SR2025

Multi-scale Energy Release Events in the Quiet Sun: A Possible Source for Coronal Heating

Rui Wang, Yiming Jiao, Xiaowei Zhao +1

The coronal heating problem remains one of the most challenging questions in solar physics. The energy driving coronal heating is widely understood to be associated with convective…

astro-ph.SR2024

On the Acceleration of the Young Solar Wind from Different Source Regions

Yiming Jiao, Ying D. Liu, Wenshuai Cheng +2

The acceleration of the young solar wind is studied using the first 17 encounters of Parker Solar Probe. We identify wind intervals from different source regions: coronal hole (CH)…