most citedDual Origins of Rapid Flare Ribbon Downflows in an X9-class Solar Flare

2 citations · 2 across the 7 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

Measured energy exchange in coronal hole solar wind from its solar origins to the heliosphere

Yeimy J. Rivera, Alin R. Paraschiv, Samuel T. Badman +33

Coordinated ground- and space-based remote observations are used to provide a comprehensive, multi-perspective view of the solar atmosphere that we connect with in situ measurement…

astro-ph.SR2026

Elemental Composition Evolution during the 2024 September 30 Solar Eruption: A Comparison of Hot and Cool Plasma Components with Solar Orbiter/SPICE, Hinode/EIS, and Chandrayaan-2/XSM

Momchil Molnar, Joseph Plowman, Amir Caspi +7

Solar plasma composition differs between the photosphere and corona over a range of timescales, with preferential enhancement of elements with low first ionization potential (FIP).…

astro-ph.SR2026

SADCat: A Catalog of Supra-Arcade Downflow Events in Solar Flares

Trestan F. Simon, Ryan J. French

Supra-arcade downflows (SADs) are sunward-traveling features routinely observed in hot fan structures above magnetic loop arcades during eruptive solar flares. We manually compiled…

astro-ph.SR2026

Investigating Pre-flare Signatures in Spectroscopic Observations of an X9-class Solar Flare

Louis Seyfritz, Maria Kazachenko, Ryan French

On October 3rd, 2024, the Sun emitted an X9.0-class flare from active region NOAA 13842. The event was recorded by multiple space-based instruments, beginning hours before the erup…

astro-ph.SR2026

Evolution of Spatial Complexity in Flare Ribbon Substructure and Its Relationship to Magnetic Reconnection Dynamics

Marcel F. Corchado Albelo, Maria D. Kazachenko, Ryan J. French +5

Recent three-dimensional flare models suggest that flare-ribbon substructure is linked to the fragmentation of the reconnecting current sheet in the corona. Flare-ribbon substructu…

astro-ph.SR2026

Spectroscopic analysis and RHD modeling of the first Ca II H and H-epsilon flare spectra from DKIST/ViSP

Cole Tamburri, Adam Kowalski, Gianna Cauzzi +7

We analyze decay phase observations of the GOES class C6.7 flare SOL2022-08-19T20:31 by the Visible Spectropolarimeter (ViSP) on the National Science Foundation's Daniel K. Inouye…

astro-ph.SR2025

Evolution of Flare Ribbon Bead-like Structures in a Solar Flare

Ryan J. French, Maria D. Kazachenko, David Berghmans +6

We present fast cadence and high resolution observations of flare ribbons from the Solar Orbiter Extreme Ultraviolet Imager (EUI). Utilizing the short-exposure observations from th…

astro-ph.SR2025★ 2 cited

Dual Origins of Rapid Flare Ribbon Downflows in an X9-class Solar Flare

Ryan J. French, William H. Ashfield, Cole A. Tamburri +4

We detect rapid downflows of 150-217 km/s in IRIS Si IV 1402.77 nm measurements of an X9-class solar flare on 2024 October 3rd. The fast redshift values persist for over 15 minutes…

astro-ph.SR2025

Unveiling Unprecedented Fine Structure in Coronal Flare Loops with the DKIST

Cole A. Tamburri, Maria D. Kazachenko, Gianna Cauzzi +8

We present the highest-resolution H observations of a solar flare to date, collected during the decay phase of an X1.3-class flare on 8 August 2024 at 20:12 UT. Observations wit…

astro-ph.SR2025

Multi-line Spectropolarimetric Observation of Flare Ribbon Fine Structures with ViSP/DKIST

Rahul Yadav, Maria D. Kazachenko, Gianna Cauzzi +3

We present an analysis of flare ribbon fine structure observed during a GOES C2-class flare using high spatial and spectral resolution multi-line spectropolarimetric observations f…