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
• Flux rope modeling of the 2022 Sep 5 CME observed by Parker Solar Probe and Solar Orbiter from 0.07 to 0.69 au
• VizieR Online Data Catalog: ICMEs observed by Juno between 1 and 5.4au (Davies+, 2021)
• Characterizing ICME-related Forbush Decreases at Mercury
• A Catalogue of ICMEs Observed by Juno between 1 and 5.4 AU
• The Evolution of Interplanetary Coronal Mass Ejections in the Heliosphere
• In-Situ Multi-Spacecraft and Remote Imaging Observations of the First CME Detected by Solar Orbiter
• Using In-Situ Juno Observations to Understand the Radial Evolution of Interplanetary Coronal Mass Ejections.
• Unlocking the Potential of Simultaneous Measurements to Investigate CME Properties: A Proof of Concept
• Characterization of Small Flux Ropes using Juno Spacecraft Cruise Phase Data
• Using Solar Orbiter as an Upstream Solar Wind Monitor for Real Time Space Weather Predictions
• Multi-point magnetic flux rope analysis for the 2020 April 19 CME observed in situ by Solar Orbiter and Wind
• VizieR Online Data Catalog: Multipoint coronal mass ejections events (Mostl+, 2022)
• How Magnetic Reconnection Inside Coronal Mass Ejections May Affect Their Coherence
• Multi-spacecraft Study of the Solar Wind in Latitude
• Solar origins of a strong stealth CME detected by Solar Orbiter
• Multi-point analysis of coronal mass ejection flux ropes using combined data from Solar Orbiter, BepiColombo, and Wind
• Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter
• Redefining Flux Ropes in Heliophysics
• Sensing CME Magnetic Fields En Route to 1 AU
• On the importance of investigating CME complexity evolution during interplanetary propagation
• Learn to Walk Before You Run: A Case for Fundamental CME Research Utilizing Idealized MHD Models
• Connecting Solar and Stellar Flares/CMEs: Expanding Heliophysics to Encompass Exoplanetary Space Weather
• The Multi-spacecraft Heliospheric Mission (MHM)
• The Importance of Fundamental Research on the Upper Coronal and Heliospheric Evolution of Coronal Mass Ejections
• On the Need for a Coronal and Inner Heliospheric Panel for the 2024 Heliophysics Decadal Survey
• Heliophysics and space weather science at ∼1.5 AU: Knowledge gaps and need for space weather monitors at Mars
• On the importance of investigating CME complexity evolution during interplanetary propagation
• On the importance of investigating ICME complexity evolution during propagation
• Investigating CME properties using Simultaneous Multi-Spacecraft Measurements.
• Multipoint In Situ and Imaging Observations of Interplanetary Coronal Mass Ejections with Solar Orbiter, BepiColombo, Parker Solar Probe, Wind, and STEREO-A
• Evolution of Magnetic Complexity and Coherence within Interplanetary Coronal Mass Ejections: Novel Insights from Multi-Point Observational and Numerical Investigations
• CME-CME Interactions: Preconditioning, Collisions and Flux Erosion: How to Create a Perfect Storm?
• On the importance of investigating ICME complexity evolution during propagation
• Coronal Mass Ejections Observed In Situ by STEREO-A in 2021: Multi-spacecraft Measurements
• Characterization of Small Flux Ropes using Juno Spacecraft Data
• The 2021 February 24 Coronal Mass Ejection Measured Jointly by STEREO-A and Wind at 55° Separation: Consequences for CME Global Properties
• Multi-spacecraft observations of the structure of the sheath of an interplanetary coronal mass ejection and related energetic ion enhancement
• Study of two interacting interplanetary coronal mass ejections encountered by Solar Orbiter during its first perihelion passage. Observations and modeling
• Radial evolution of the April 2020 stealth coronal mass ejection between 0.8 and 1 AU. Comparison of Forbush decreases at Solar Orbiter and near the Earth
• What is a Heliospheric Flux Rope?
• Heliophysics and Space Weather Science at 1.5 AU: Knowledge Gaps and Need for Solar and Solar Wind Monitors at Mars
• Flux Rope Modeling of the 2022 September 5 Coronal Mass Ejection Observed by Parker Solar Probe and Solar Orbiter from 0.07 to 0.69 au
• Understanding the Effects of Spacecraft Trajectories through Solar Coronal Mass Ejection Flux Ropes Using 3DCOREweb
• Characterization of Small Flux Ropes Using Juno Spacecraft Cruise-phase Data
• The Need for a Sub‐L1 Space Weather Research Mission: Current Knowledge Gaps on Coronal Mass Ejections
• Advancing Space Weather Forecasting with Sub-L1 Monitors: A Statistical Analysis
• Multipoint coronal mass ejection events in solar cycle 25
• Prediction of coronal mass ejection geo-effectiveness using Solar Orbiter as a far upstream monitor in real-time
• First Observations of a Geomagnetic Superstorm With a Sub‐L1 Monitor
• Advancing Space Weather Forecasting with Sub-L1 Monitors: A Statistical Analysis
• Influence of the Deformation of Coronal Mass Ejections on Their in-Situ Fitting with Circular-Cross-Section Flux Rope Models
• Do All Mesoscales Matter? Analyzing Multi-Spacecraft Coronal Mass Ejection Data
• VizieR Online Data Catalog: Multi-spacecraft ICME Database (Davies+, 2022)
• Enhancing STEREO-HI beacon data with machine learning for efficient CME forecasting
• Understanding the Radial Expansion of Coronal Mass Ejections in the Heliosphere
• Space weather forecasting using STEREO-A as a sub-L1 solar wind monitor
• Recent Multi-Spacecraft Measurements of Large-Scale Transients Near 1 AU by STEREO-A and L1 Spacecraft
• The variability and evolution of interplanetary coronal mass ejections
• New Observations Needed to Advance Our Understanding of Coronal Mass Ejections
• Real-time prediction of geomagnetic storms using Solar Orbiter as a far upstream solar wind monitor