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Published by: \apjl Published on: 02/2021
YEAR: 2021   DOI: 10.3847/2041-8213/abe1cb
Predictions of the impact of coronal mass ejections (CMEs) in the heliosphere mostly rely on cone CME models, whose performances are optimized for locations in the ecliptic plane and at 1 AU (e.g., at Earth). Progresses in the exploration of the inner heliosphere, however, advocate the need to assess their performances at both higher latitudes and smaller heliocentric distances. In this work, we perform 3-D magnetohydrodynamics simulations of artificial cone CMEs using the EUropean Heliospheric FORecasting Information Ass ...
Published by: Space Weather Published on: 03/2020
YEAR: 2020   DOI: 10.1029/2019SW002246