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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

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12 papers · 1 filter

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…

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…

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.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…

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…

astro-ph.SR2019★ 32 cited

Seed Population Pre-Conditioning and Acceleration Observed by Parker Solar Probe

N. A. Schwadron, S. Bale, J. Bonnell +42

A series of solar energetic particle (SEP) events were observed at Parker Solar Probe (PSP) by the Integrated Science Investigation of the Sun (\ISOIS) during the period from April…

astro-ph.SR2017★ 80 cited

Forward modeling of coronal mass ejection flux ropes in the inner heliosphere with 3DCORE

Christian Möstl, Tanja Amerstorfer, Erika Palmerio +7

Forecasting the geomagnetic effects of solar storms, known as coronal mass ejections (CMEs), is currently severely limited by our inability to predict the magnetic field configurat…

astro-ph.SR2017★ 105 cited

Modeling observations of solar coronal mass ejections with heliospheric imagers verified with the Heliophysics System Observatory

C. Möstl, A. Isavnin, P. D. Boakes +18

We present an advance towards accurately predicting the arrivals of coronal mass ejections (CMEs) at the terrestrial planets, including Earth. For the first time, we are able to as…