activity
20242026
collaborators

8 papers

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

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 wi…

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…

astro-ph.SR2025

First coordinated observations between Solar Orbiter and the Daniel K. Inouye Solar Telescope

Krzysztof Barczynski, Miho Janvier, Chris J. Nelson +8

Solar Orbiter and the Daniel K. Inouye Solar Telescope (DKIST) are two of the newest facilities available to the solar physics community. The first coordinated observations of the…

astro-ph.SR2025

The striated solar photosphere observed at 0."03, resolution

D. Kuridze, F. Wöger, H. Uitenbroek +5

Striated granular edges observed in the solar photosphere represent one of the smallest-scale phenomena on the Sun. They arise from the interaction of strongly coupled hydrodynamic…

astro-ph.SR2025

A High-resolution, Inversion-Based Synoptic Study of Solar Granulation

James Crowley, Ivan Milic, Gianna Cauzzi +1

The convectively driven, weakly magnetized regions of the solar photosphere dominate the Sun's surface at any given time, but the temporal variations of these quiet regions of the…