3 papers
astro-ph.SR2026
Synthetic Fe XIII 1074.7 nm Observations of Torsional Alfvén Waves in Coronal Waveguides
Samuel Skirvin, Richard Morton, Thomas Schad
Torsional Alfvén waves are a promising mechanism for transporting energy through the solar atmosphere, with implications for coronal heating and solar wind acceleration. Recently,…
astro-ph.SR2025
Ubiquitous high-frequency waves and disturbances in the active region corona observed with DKIST/Cryo-NIRSP
Momchil E. Molnar, Richard Morton, Alin Paraschiv +4
The plasma of the solar corona harbors a multitude of coronal wave modes, some of which could be dissipated to provide the required energy and momentum to heat the corona and accel…
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…