activity
20172026
most citedThe Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action

112 citations · 357 across the 18 of their papers we have counts for

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Showing astro-ph.SRShow all

26 papers · 1 filter

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.SR2026

Constraining turbulent solar flare acceleration regions by connecting kinetic modeling and X-ray observations

Morgan Stores, Natasha Jeffrey, Ewan Dickson +2

Spatially-resolved X-ray observations are the key to understanding electron acceleration in solar flares. Currently, the underlying processes that efficiently energize solar flare…

astro-ph.SR2025

Time-dependent Turbulent Electron Acceleration and Transport in Solar Flares

Luiz A. C. A. Schiavo, Natasha L. S. Jeffrey, Gert J. J. Botha +1

Solar flares are explosive releases of magnetic energy stored in the solar corona, driven by magnetic reconnection. These events accelerate electrons, generating hard X-ray emissio…

astro-ph.SR2025

Multi-wavelength observations of substructures in solar flare ribbons

Vishal Singh, Eamon Scullion, Gert J. J. Botha +6

Solar flare ribbons are extensive brightenings in the chromosphere during flares, often showing fine scale structuring that reflects the underlying energy release. Using high caden…

astro-ph.SR2025★ 9 cited

Tracing the Heliospheric Magnetic Field via Anisotropic Radio-Wave Scattering

Daniel L. Clarkson, Eduard P. Kontar, Nicolina Chrysaphi +4

Astrophysical radio sources are embedded in turbulent magnetised environments. In the 1 MHz sky, solar radio bursts are the brightest sources, produced by electrons travelling alon…

astro-ph.SR2025

Exploring the Origin of Solar Energetic Electrons II: Investigating Turbulent Coronal Acceleration

Ross Pallister, Natasha L. S. Jeffrey, Morgan Stores

Non-thermal particle acceleration in the solar corona is evident from both remote hard X-ray (HXR) sources in the chromosphere and direct in-situ detection in the heliosphere. Corr…