Emma Davies

Publications

• A Catalog of Interplanetary Coronal Mass Ejections Observed by Juno between 1 and 5.4 au
• In-Situ Multi-Spacecraft and Remote Imaging Observations of the First CME Detected by Solar Orbiter and BepiColombo
• On the Radial and Longitudinal Variation of a Magnetic Cloud: ACE, Wind, ARTEMIS and Juno Observations
• Three Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection
• Overview of interplanetary coronal mass ejections observed by Solar Orbiter, Parker Solar Probe, Bepi Colombo, Wind and STEREO-A
• Triple-point magnetic flux rope analysis for the 2020 April 19 CME observed in situ by Solar Orbiter, Bepi Colombo, and WIND
• The sheath region of April 2020 magnetic cloud and the associated energetic ions
• Ripples in the Heliospheric Current Sheet: Dependence on Latitude and Transient Outflows
• Multi-spacecraft study of the solar wind at solar minimum: Dependence on latitude and transient outflows
• Causes and Consequences of Magnetic Complexity Changes within Interplanetary Coronal Mass Ejections: A Statistical Study
• Multipoint Interplanetary Coronal Mass Ejections Observed with Solar Orbiter, BepiColombo, Parker Solar Probe, Wind, and STEREO-A
• Magnetic complexity changes within interplanetary coronal mass ejections: insights from a statistical study based on radially-aligned spacecraft observations
• Multi-spacecraft Observations of Interplanetary Coronal Mass Ejections between 0.3 and 2.2 AU: Conjunctions with the Juno Spacecraft
• A Coronal Mass Ejection and Magnetic Ejecta Observed In Situ by STEREO-A and Wind at 55° Angular Separation
• Using In-Situ Juno Observations to Understand the Evolution of Interplanetary Coronal Mass Ejections Within 1 AU and Beyond
• The sheath region of April 2020 magnetic cloud and the associated energetic ions
• Multi-Spacecraft Observations of a Unique Type of High-Latitude ICME
• In situ multi-spacecraft and remote imaging observations of the first CME detected by Solar Orbiter and BepiColombo
• Multi-spacecraft Observations of the Evolution of Interplanetary Coronal Mass Ejections between 0.3 and 2.2 au: Conjunctions with the Juno Spacecraft
• Successive Interacting Coronal Mass Ejections: How to Create a Perfect Storm
• Characterizing Interplanetary Coronal Mass Ejection-related Forbush Decreases at Mercury Using MESSENGER Observations: Identification of a One- or Two-step Structure
• Successive interacting coronal mass ejections: Preconditioning, magnetic reconnection and flux erosion: How to create a perfect storm?
• Forecasting southward pointing magnetic fields in solar coronal mass ejections
• The effect of magnetic reconnection on ICME-related GCR modulation
• How Magnetic Reconnection May Affect the Coherence of Interplanetary Coronal Mass Ejections
• Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers)
• Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers)
• The Eruption of a Magnetic Flux Rope Observed by Solar Orbiter and Parker Solar Probe
• Investigating the Magnetic Structure of Interplanetary Coronal Mass Ejections Using Simultaneous Multispacecraft In Situ Measurements
• Where Does the Inner Heliosphere End?
• The Effect of Magnetic Field Line Topology on ICME-related GCR Modulation
• Combining STEREO heliospheric imagers and Solar Orbiter to investigate the evolution of the 2022 March 10 CME
• A Community Data Set for Comparing Automated Coronal Hole Detection Schemes
• Properties of an Interplanetary Shock Observed at 0.07 and 0.7 au by Parker Solar Probe and Solar Orbiter
• 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
• The Width of Magnetic Ejecta Measured near 1 au: Lessons from STEREO-A Measurements in 2021–2022
• Understanding the effects of spacecraft trajectories through solar coronal mass ejection flux ropes using 3DCOREweb
• Investigating the coherency and expansion of ICMEs using multi-spacecraft observations
• A Community Dataset for Comparing Automated Coronal Hole Detection Schemes and its Imprint on Magnetic Models
• The Space Weather Research on Coronal Mass Ejections Required Before Operational Sub-L1 Monitors
• Using STEREO-A data from April to November 2023 as a sub-L1 monitor
• A Survey of Coronal Mass Ejections Measured In Situ by Parker Solar Probe during 2018–2022