From the 1 of 4 linked papers with an AI index.
4 papers
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…
BepiColombo at Mercury: Three flybys, three magnetospheres
Hayley N. Williamson, Stas Barabash, Hans Nilsson +14
We examine the first three BepiColombo Mercury flybys Using data from the Miniature Ion Precipitation Analyzer (MIPA), an ion mass analyzer in the Search for Exospheric Refilling a…