activity
20212026
most citedMatching temporal signatures of solar features to their corresponding solar wind outflows

5 citations · 5 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2026

Direct Measurement of Polar Coronal Hole-like Solar Wind in its Acceleration Phase

Samuel T. Badman, Yeimy J. Rivera, Michael L. Stevens +38

The early evolution of fast polar coronal hole (PCH) solar wind remains largely unconstrained by in situ measurements. In March 2025, Parker Solar Probe (Parker) at its closest app…

astro-ph.SR2026

A new methodology for inferring the plasma conditions in solar flare energetic electron source regions from in situ electron energy spectra

Samuel Carter, Natasha L. S. Jeffrey, Robert T. Wicks +1

The conditions within solar flares that lead to efficient electron acceleration are not well constrained. It is not clear whether the populations accelerated out into the heliosphe…

astro-ph.IM2025

Transformational astrophysics and exoplanet science with Habitable Worlds Observatory's High Resolution Imager

Vincent Van Eylen, Richard Massey, Saeeda Awan +167

Habitable Worlds Observatory (HWO) will be NASA's flagship space telescope of the 2040s, designed to search for life on other planets and to transform broad areas of astrophysics.…

astro-ph.SR2025

Local Particle Acceleration in an ICME-in-Sheath Structure Observed by Solar Orbiter

Xiaomin Chen, Chuan Li, Zigong Xu +5

Local particle acceleration in the shock sheath region formed during the interaction between multiple coronal mass ejections (CMEs) is a complicated process that is still under inv…

physics.space-ph2025

Langmuir Wave Excitation in Solar-wind Magnetic Holes

Jingting Liu, Daniel Verscharen, Jesse Coburn +8

Magnetic holes are structures commonly observed in various space plasma environments throughout the solar system, including the solar wind. These structures are characterized by a…

physics.space-ph2025

How does the limited resolution of space plasma analyzers affect the accuracy of space plasma measurements?

Georgios Nicolaou, Charalambos Ioannou, Christopher Owen +3

We investigate the systematic errors in measured plasma velocity distribution functions and their corresponding velocity moments, arising from the limited energy and angular resolu…

astro-ph.SR2024

Radial evolution of a density structure within a solar wind magnetic sector boundary

Etienne Berriot, Pascal Démoulin, Olga Alexandrova +3

This study focuses on a radial alignment between Parker Solar Probe (PSP) and Solar Orbiter (SolO) on the 29 of April 2021 (during a solar minimum), when the two spac…

astro-ph.SR2024

Observation of a Fully-formed Forward--Reverse Shock Pair Due to the Interaction Between Two Coronal Mass Ejections at 0.5 au

D. Trotta, A. Dimmock, X. Blanco-Cano +17

We report direct observations of a fast magnetosonic forward--reverse shock pair observed by Solar Orbiter on March 8, 2022 at the short heliocentric distance of 0.5 au. The struct…

physics.space-ph2024

The impact of non-equilibrium plasma distributions on solar wind measurements by Vigil's Plasma Analyser

Hongjie Zhang, Daniel Verscharen, Georgios Nicolaou

In order to protect society from space weather impacts, we must monitor space weather and obtain early warnings for extreme events if possible. For this purpose, the European Space…

astro-ph.SR2024

Probing Turbulent Scattering Effects on Suprathermal Electrons in the Solar Wind: Modeling, Observations and Implications

Arnaud Zaslavsky, Justin C. Kasper, Eduard P. Kontar +7

This study explores the impact of a turbulent scattering mechanism, akin to those influencing solar and galactic cosmic rays propagating in the interplanetary medium, on the popula…

astro-ph.SR2023

Solar Electron Beam -- Langmuir Wave Interactions and How They Modify Solar Electron Beam Spectra: Solar Orbiter Observations of a Match Made in the Heliosphere

Camille Y. Lorfing, Hamish A. S. Reid, Raul Gomez-Herrero +7

Solar Orbiter's four in-situ instruments have recorded numerous energetic electron events at heliocentric distances between 0.5 and 1au. We analyse energetic electron fluxes, spect…

astro-ph.SR2021★ 5 cited

Matching temporal signatures of solar features to their corresponding solar wind outflows

Diego de Pablos, David M. Long, Christopher J. Owen +3

The role of small-scale coronal eruptive phenomena in the generation and heating of the solar wind remains an open question. Here, we investigate the role played by coronal jets in…