activity
20112026
most citedHard X-ray and UV Observations of the 2005 January 15 Two-ribbon Flare

33 citations · 41 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2026

ESCAPE: a small explorer mission to study the stellar drivers of exoplanet evolution

Allison Youngblood, Kevin France, Brian Fleming +37

The long-term stability of exoplanetary atmospheres depends critically on the extreme-ultraviolet (EUV) photon and high-energy particle fluxes from the host star, which are poorly…

astro-ph.SR2026

Enigmatic Line Broadening During Solar Flares: Magnetic Field Broadening?

Thomas Gomez, Adam Kowalski, Cole Tamburri +2

The origin of the extreme broadening observed in chromospheric metal lines during solar and stellar flares, particularly Mg II h&k and Ca II H&K, remains poorly understood. These l…

astro-ph.IM2025

Understanding Solar Flares and Energetic Events: Open questions, observational requirements, and instrumental needs over the coming decade

Malcolm K. Druett, Graham S. Kerr, Joel C. Allred +15

Solar flares are the largest energy-release events in the Solar System, allowing us to study fundamental physical phenomena under extreme conditions. Those include magnetic reconne…

astro-ph.SR2025

Solar Orbiter's 2024 Major Flare Campaigns: An Overview

Daniel F. Ryan, Laura A. Hayes, Hannah Collier +17

Solar Orbiter conducted a series of flare-optimised observing campaigns in 2024 utilising the Major Flare Solar Orbiter Observing Plan (SOOP). Dedicated observations were performed…

astro-ph.SR2025

Fe XVIII and Fe XX Forbidden Lines Observed by Solar Orbiter/SPICE

Peter R. Young, Andrew R. Inglis, Graham S. Kerr +2

The first simultaneous observations of the Fe XVIII 974.86 Å and Fe XX 721.56 Å forbidden lines from the Spectral Imaging of the Coronal Environment (SPICE) spectrograph on Solar O…

astro-ph.IM2023★ 3 cited

Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…

astro-ph.IM2023★ 5 cited

COMPLETE: A flagship mission for complete understanding of 3D coronal magnetic energy release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

COMPLETE is a flagship mission concept combining broadband spectroscopic imaging and comprehensive magnetography from multiple viewpoints around the Sun to enable tomographic recon…

astro-ph.SR2011★ 33 cited

Hard X-ray and UV Observations of the 2005 January 15 Two-ribbon Flare

J. X. Cheng, G. Kerr, J. Qiu

In this paper, we present comprehensive analysis of a two-ribbon flare observed in UV 1600Å by Transition Region and Coronal Explorer and in HXRs by Reuven Ramaty High Energy Solar…