activity
20142026
most citedConnecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU

168 citations · 368 across the 14 of their papers we have counts for

collaborators

14 papers

physics.space-ph2026

Investigating potential benefits of future sub-L1 missions with STEREO-A

Eva Weiler, Emma E. Davies, Christian Möstl +4

We present the first statistical study of geomagnetic storm forecasting using in situ data from the STEREO-A spacecraft as a sub-L1 monitor. Between November 2022 and June 2024, ST…

physics.space-ph2025

Real-time prediction of two geomagnetic storms using Solar Orbiter as a far upstream solar wind monitor

Emma E. Davies, Eva Weiler, Christian Möstl +6

We present the first real-time predictions of coronal mass ejection (CME) magnetic structure and resulting geomagnetic impact at Earth for two events using far-upstream observation…

astro-ph.SR2024★ 1 cited

Distorted Magnetic Flux Ropes within Interplanetary Coronal Mass Ejections

Andreas J. Weiss, Teresa Nieves-Chinchilla, Christian Möstl

Magnetic flux ropes within interplanetary coronal mass ejections are often characterized as simplistic cylindrical or toroidal tubes with field lines that twist around the cylinder…

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…

physics.space-ph2023★ 1 cited

The effect of magnetic field line topology on ICME-related GCR modulation

Emma E. Davies, Camilla Scolini, Réka M. Winslow +2

The large-scale magnetic structure of interplanetary coronal mass ejections (ICMEs) has been shown to affect the galactic cosmic ray (GCR) flux measured in situ by spacecraft, caus…

astro-ph.SR2023★ 18 cited

Turbulence Properties of Interplanetary Coronal Mass Ejections in the Inner Heliosphere: Dependence on Proton Beta and Flux Rope Structure

S. W. Good, O. K. Rantala, A. -S. M. Jylhä +3

Interplanetary coronal mass ejections (ICMEs) have low proton beta across a broad range of heliocentric distances and a magnetic flux rope structure at large scales, making them a…

astro-ph.SR2023★ 1 cited

L1 and off Sun-Earth line visible-light imaging of Earth-directed CMEs: An analysis of inconsistent observations

Richard A. Harrison, Jackie A. Davies, David Barnes +1

The efficacy of coronal mass ejection (CME) observations as a key input to space weather forecasting is explored by comparing on and off Sun-Earth line observations from the ESA/NA…

physics.space-ph2022★ 22 cited

Multi-Spacecraft Observations of the Evolution of Interplanetary Coronal Mass Ejections Between 0.3 and 2.2 AU: Conjunctions with the Juno Spacecraft

Emma E. Davies, Réka M. Winslow, Camilla Scolini +4

We present a catalogue of 35 interplanetary coronal mass ejections (ICMEs) observed by the Juno spacecraft and at least one other spacecraft during its cruise phase to Jupiter. We…

physics.space-ph2021★ 27 cited

A Catalog of Interplanetary Coronal Mass Ejections Observed by Juno between 1 and 5.4 AU

Emma E. Davies, Robert J. Forsyth, Réka M. Winslow +2

We use magnetic field measurements by the Juno spacecraft to catalog and investigate interplanetary coronal mass ejections (ICMEs) beyond 1 AU. During its cruise phase, Juno spent…

astro-ph.SR2021★ 52 cited

Multipoint interplanetary coronal mass ejections observed with Solar Orbiter, BepiColombo, Parker Solar Probe, Wind and STEREO-A

C. Möstl, A. J. Weiss, M. A. Reiss +12

We report the result of the first search for multipoint in situ and imaging observations of interplanetary coronal mass ejections (ICMEs) starting with the first Solar Orbiter (Sol…

astro-ph.SR2021★ 7 cited

Predicting CMEs using ELEvoHI with STEREO-HI beacon data

Maike Bauer, Tanja Amerstorfer, Jürgen Hinterreiter +6

Being able to accurately predict the arrival of coronal mass ejections (CMEs) at Earth has been a long-standing problem in space weather research and operations. In this study, we…

physics.space-ph2021★ 24 cited

Making waves: Mirror Mode structures around Mars observed by the MAVEN spacecraft

Cyril Simon Wedlund, Martin Volwerk, Christian Mazelle +4

We present an in-depth analysis of a time interval when quasi-linear mirror mode structures were detected by magnetic field and plasma measurements as observed by the NASA/Mars Atm…

astro-ph.SR2016★ 47 cited

Sun-to-Earth Characteristics of the 2012 July 12 Coronal Mass Ejection and Associated Geo-effectiveness

Huidong Hu, Ying D. Liu, Rui Wang +2

We analyze multi-spacecraft observations associated with the 2012 July 12 Coronal Mass Ejection (CME), covering the source region on the Sun from SDO, stereoscopic imaging observat…

astro-ph.SR2014★ 168 cited

Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU

C. Möstl, K. Amla, J. R. Hall +15

Forecasting the in situ properties of coronal mass ejections (CMEs) from remote images is expected to strongly enhance predictions of space weather, and is of general interest for…