activity
20202026
most cited20 Years of ACE Data: How Superposed Epoch Analyses Reveal Generic Features in Interplanetary CME Profiles

38 citations · 84 across the 10 of their papers we have counts for

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Showing 2023Show all

6 papers · 1 filter

astro-ph.SR2023

The Width of Magnetic Ejecta Measured Near 1 au: Lessons from STEREO-A Measurements in 2021--2022

Noé Lugaz, Bin Zhuang, Camilla Scolini +7

Coronal mass ejections (CMEs) are large-scale eruptions with a typical radial size at 1 au of 0.21 au but their angular width in interplanetary space is still mostly unknown, espec…

astro-ph.SR2023★ 1 cited

Discrepancies in the Properties of a Coronal Mass Ejection on Scales of 0.03~au as Revealed by Simultaneous Measurements at Solar Orbiter and Wind: The 2021 November 3--5 Event

F. Regnault, N. Al-Haddad, N. Lugaz +4

Simultaneous in situ measurements of coronal mass ejections (CMEs), including both plasma and magnetic field, by two spacecraft in radial alignment have been extremely rare. Here,…

astro-ph.SR2023

Investigating the Magnetic Structure of Interplanetary Coronal Mass Ejections using Simultaneous Multi-Spacecraft In situ Measurements

F. Regnault, N. Al-Haddad, N. Lugaz +5

In situ measurements from spacecraft typically provide a time series at a single location through coronal mass ejections (CMEs) and they have been one of the main methods to invest…

astro-ph.IM2023★ 5 cited

New Observations Needed to Advance Our Understanding of Coronal Mass Ejections

Erika Palmerio, Benjamin J. Lynch, Christina O. Lee +19

Coronal mass ejections (CMEs) are large eruptions from the Sun that propagate through the heliosphere after launch. Observational studies of these transient phenomena are usually b…

astro-ph.SR2023

Impact of the solar activity on the propagation of ICMEs: Simulations of hydro, magnetic and median ICMEs at minimum and maximum of activity

Barbara Perri, Brigitte Schmieder, Pascal Démoulin +2

The propagation of Interplanetary Coronal Mass Ejections (ICMEs) in the heliosphere is influenced by many physical phenomena, related to the internal structure of the ICME and its…

astro-ph.SR2023★ 24 cited

Self-consistent propagation of flux ropes in realistic coronal simulations

L. Linan, F. Regnault, B. Perri +5

The aim of this paper is to demonstrate the possible use of the new coronal model COCONUT to compute a detailed representation of a numerical CME at 0.1~AU, after its injection at…