850 citations · 2.3k across the 47 of their papers we have counts for
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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…
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…
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…
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$…
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…
Formation Of The Lyman Continuum During Solar Flares
Shaun A. McLaughlin, Ryan O. Milligan, Graham S. Kerr +3
The Lyman Continuum (LyC; Å) forms at the top of the chromosphere in the quiet-Sun, making LyC a powerful tool for probing the chromospheric plasma during solar flares. To…