activity
20052026
most citedAn Observational Overview of Solar Flares

850 citations · 2.3k across the 47 of their papers we have counts for

collaborators

48 papers

astro-ph.SR2026

Delayed, Line-dependent Reorganization of Pore Oscillations Following a Compact C8.2 Flare Observed by Sunrise III/SUSI

Shahin Jafarzadeh, David B. Jess, Marco Stangalini +34

Magnetic oscillations permeating the solar atmosphere can be altered by flares. This could be due to changes in the atmospheric magnetic waveguide, the thermodynamic stratification…

astro-ph.SR2024

On the Instrumental Discrepancies in Lyman-alpha Observations of Solar Flares

Harry J. Greatorex, Ryan O. Milligan, Ingolf E. Dammasch

Despite the energetic significance of Lyman-alpha (Lyα; 1216Å) emission from solar flares, regular observations of flare related Lyα have been relatively scarce until recently. Adv…

astro-ph.SR2024

The Solar eruptioN Integral Field Spectrograph

Vicki L. Herde, Phillip C. Chamberlin, Don Schmit +17

The Solar eruptioN Integral Field Spectrograph (SNIFS) is a solar-gazing spectrograph scheduled to fly in the summer of 2025 on a NASA sounding rocket. Its goal is to view the sola…

astro-ph.SR2023

Observational Analysis of Lyman-alpha Emission in Equivalent Magnitude Solar Flares

Harry J. Greatorex, Ryan O. Milligan, Phillip C. Chamberlin

The chromospheric Lyman-alpha line of neutral hydrogen (Ly; 1216 Å) is the most intense emission line in the solar spectrum, yet until recently observations of flare-related Ly$…

astro-ph.IM2023★ 2 cited

The need for focused, hard X-ray investigations of the Sun

Lindsay Glesener, Albert Y. Shih, Amir Caspi +46

Understanding the nature of energetic particles in the solar atmosphere is one of the most important outstanding problems in heliophysics. Flare-accelerated particles compose a hug…

astro-ph.SR2023★ 19 cited

Prospects of Detecting Non-thermal Protons in Solar Flares via Lyman Line Spectroscopy: Revisiting the Orrall-Zirker Effect

Graham S. Kerr, Joel C. Allred, Adam F. Kowalski +5

Solar flares are efficient particle accelerators, with a substantial fraction of the energy released manifesting as non-thermal particles. While the role that non-thermal electrons…