activity
20162025
most citedModeling observations of solar coronal mass ejections with heliospheric imagers verified with the Heliophysics System Observatory

105 citations · 994 across the 34 of their papers we have counts for

collaborators

34 papers

physics.space-ph2025

Influence of the Deformation of Coronal Mass Ejections on Their In-Situ Fitting with Circular-Cross-Section Flux Rope Models

Bin Zhuang, Noé Lugaz, Nada Al-Haddad +8

Understanding the properties, especially the magnetohydrodynamic (MHD) invariants, of coronal mass ejections (CMEs) measured in-situ is key to bridging the CME properties from the…

physics.space-ph2024

Can Alfvénic Fluctuations Affect the Correlation and Complexity of Magnetic Fields in Magnetic Ejecta? A Case Study Based on Multi-Spacecraft Measurements at 1~au

Camilla Scolini, Bin Zhuang, Noé Lugaz +4

We investigate whether Alfvénic fluctuations (AFs) can affect the structure of magnetic ejecta (MEs) within interplanetary coronal mass ejections (ICMEs). We study an ICME observed…

astro-ph.SR2023

On the Role of Alfvenic Fluctuations as Mediators of Coherence within Interplanetary Coronal Mass Ejections: Investigation of Multi-Spacecraft Measurements at 1 au

Camilla Scolini, Noe Lugaz, Reka M. Winslow +3

Interplanetary coronal mass ejections (ICMEs) are defined as ''coherent'' if they are capable of responding to external perturbations in a collective manner. This implies that info…

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.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.IM2023

Work-Life Balance Starts with Proper Deadlines and Exemplary Agencies

Noé Lugaz, Réka M. Winslow, Nada Al-Haddad +12

Diversity, equity and inclusion (DEI) programs can only be implemented successfully if proper work-life balance is possible in Heliophysics (and in STEM field in general). One of t…

astro-ph.SR2023★ 14 cited

Evolution of the Radial Size and Expansion of Coronal Mass Ejections Investigated by Combining Remote and In-Situ Observations

Bin Zhuang, Noé Lugaz, Nada Al-Haddad +4

A fundamental property of coronal mass ejections (CMEs) is their radial expansion, which determines the increase in the CME radial size and the decrease in the CME magnetic field s…

physics.space-ph2022★ 5 cited

Characterizing ICME-related Forbush Decreases at Mercury using MESSENGER Observations: Identification of a One or Two-Step Structure

Emma E. Davies, Réka M. Winslow, David J. Lawrence

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

astro-ph.SR2022★ 17 cited

Characteristic Scales of Complexity and Coherence within Interplanetary Coronal Mass Ejections: Insights from Spacecraft Swarms in Global Heliospheric Simulations

Camilla Scolini, Reka M. Winslow, Noé Lugaz +1

Many aspects of the three-dimensional (3-D) structure and evolution of interplanetary coronal mass ejections (ICMEs) remain unexplained. Here, we investigate two main topics: (1) t…

astro-ph.IM2022★ 5 cited

Connecting Solar and Stellar Flares/CMEs: Expanding Heliophysics to Encompass Exoplanetary Space Weather

B. J. Lynch, B. E. Wood, M. Jin +25

The aim of this white paper is to briefly summarize some of the outstanding gaps in the observations and modeling of stellar flares, CMEs, and exoplanetary space weather, and to di…

astro-ph.GA2022★ 33 cited

Mixing Interstellar Clouds Surrounding the Sun

Paweł Swaczyna, Nathan A. Schwadron, Eberhard Möbius +9

On its journey through the Galaxy, the Sun passes through diverse regions of the interstellar medium. High-resolution spectroscopic measurements of interstellar absorption lines in…

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-ph2022★ 27 cited

A Coronal Mass Ejection and Magnetic Ejecta Observed In Situ by STEREO-A and Wind at 55 Angular Separation

Noé Lugaz, Tarik M. Salman, Charles J. Farrugia +8

We present an analysis of {\it in situ} and remote-sensing measurements of a coronal mass ejection (CME) that erupted on 2021 February 20 and impacted both the Solar TErrestrial RE…

astro-ph.SR2021★ 27 cited

Causes and Consequences of Magnetic Complexity Changes within Interplanetary Coronal Mass Ejections: a Statistical Study

Camilla Scolini, Réka M. Winslow, Noé Lugaz +3

We present the first statistical analysis of complexity changes affecting the magnetic structure of interplanetary coronal mass ejections (ICMEs), with the aim of answering the que…

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★ 18 cited

Categorization of Coronal Mass Ejection Driven Sheath Regions: Characteristics of STEREO Events

T. M. Salman, N. Lugaz, R. M. Winslow +3

We present a comprehensive statistical analysis of 106 sheath regions driven by coronal mass ejections (CMEs) and measured near 1 AU. Using data from the STEREO probes, this extend…

astro-ph.SR2021★ 22 cited

Evolution of interplanetary coronal mass ejection complexity: a numerical study through a swarm of simulated spacecraft

Camilla Scolini, Reka M. Winslow, Noé Lugaz +1

In-situ measurements carried out by spacecraft in radial alignment are critical to advance our knowledge on the evolutionary behavior of coronal mass ejections (CMEs) and their mag…

astro-ph.SR2021★ 36 cited

First simultaneous in situ measurements of a coronal mass ejection by Parker Solar Probe and STEREO-A

Reka M. Winslow, Noé Lugaz, Camilla Scolini +1

We present the first PSP-observed CME that hits a second spacecraft before the end of the PSP encounter, providing an excellent opportunity to study short-term CME evolution. The C…

astro-ph.SR2021★ 30 cited

The effect of stream interaction regions on ICME structures observed in longitudinal conjunction

Reka M. Winslow, Camilla Scolini, Noé Lugaz +1

We study two interplanetary coronal mass ejections (ICMEs) observed at Mercury and 1 AU by spacecraft in longitudinal conjunction, investigating the question: what causes the drast…

physics.space-ph2020★ 23 cited

Properties of the Sheath Regions of Coronal Mass Ejections with or without Shocks from STEREO in situ Observations near 1 AU

T. M. Salman, N. Lugaz, C. J. Farrugia +3

We examine 188 coronal mass ejections (CMEs) measured by the twin STEREO spacecraft during 2007-2016 to investigate the generic features of the CME sheath and the magnetic ejecta (…

physics.space-ph2020★ 39 cited

Inconsistencies Between Local and Global Measures of CME Radial Expansion as Revealed by Spacecraft Conjunctions

N. Lugaz, T. M. Salman, R. M. Winslow +4

The radial expansion of coronal mass ejections (CMEs) is known to occur from remote observations; from the variation of their properties with radial distance; and from local in sit…

physics.space-ph2019★ 64 cited

Radial Evolution of Coronal Mass Ejections Between MESSENGER, Venus Express, STEREO, and L1: Catalog and Analysis

T. M. Salman, R. M. Winslow, N. Lugaz

Our knowledge of the properties of Coronal Mass Ejections (CMEs) in the inner heliosphere is constrained by the relative lack of plasma observations between Sun and 1 AU. In this w…

physics.space-ph2019★ 37 cited

Evolution of a Long-Duration Coronal Mass Ejection and its Sheath Region Between Mercury and Earth on 2013 July 9-14

N. Lugaz, R. M. Winslow, C. J. Farrugia

Using in situ measurements and remote-sensing observations, we study a coronal mass ejection (CME) that left the Sun on 9 July 2013 and impacted both Mercury and Earth while the pl…