From the 1 of 7 linked papers with an AI index.
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The Internal Magnetic Field Structure of ICMEs in the Heliosphere
Ziwei Huang, Zhenjun Zhou, Yudong Ye +7
The paper analyzes 96 interplanetary coronal mass ejection magnetic clouds observed by multiple spacecraft, using a uniform‑twist Gold–Hoyle flux‑rope model to characterize how the…
On the magnetic field evolution of interplanetary coronal mass ejections from 0.07 to 5.4 au
Christian Möstl, Emma E. Davies, Eva Weiler +8
A central question for understanding interplanetary coronal mass ejection (ICME) physics and improving space weather forecasting is how ICMEs evolve in interplanetary space. We hav…
Spatio-Temporal Evolution of the March 2022 ICME Revealed by Multi-Point Observations of Forbush Decreases
Gaku Kinoshita, Beatriz Sanchez-Cano, Yoshizumi Miyoshi +13
Interplanetary coronal mass ejections (ICMEs) cause Forbush Decreases (FDs) effects, which are local decreases in background galactic cosmic rays (GCR). Even though FDs can be obse…
A coronal mass ejection encountered by four spacecraft within 1 au from the Sun: Ensemble modelling of propagation and magnetic structure
Erika Palmerio, Christina Kay, Nada Al-Haddad +11
Understanding and predicting the structure and evolution of coronal mass ejections (CMEs) in the heliosphere remains one of the most sought-after goals in heliophysics and space we…
Interplanetary Rotation of 2021 December 4 CME
Mengxuan Ma, Liping Yang, Fang Shen +9
The magnetic orientation of coronal mass ejections (CMEs) is of great importance to understand their space weather effects. Although many evidences suggest that CMEs can undergo si…