activity
20242026
collaborators

6 papers

astro-ph.SR2026

Anisotropic non-Maxwellian velocity distributions in the solar transition region

Paola Testa, Bart De Pontieu, Kyuhyoun Cho +1

High resolution spectral observations of transition region spectral lines capture the signatures of energy deposition and redistribution at the boundary between the lower and upper…

astro-ph.SR2026

Predicting the thermodynamics in the chromosphere from the translation of SDO data into the IRIS inversion results using a visual transformer model

Alberto Sainz Dalda, Vishal Upendran, Juno Kim +4

We present SDO2IRIS: a visual transformer model that translates a combination of images of the chromosphere and transition region (TR), observed by AIA, and a line-of-sight mag…

astro-ph.SR2025

Coronal Abundance Fractionation Linked to Chromospheric Transverse MHD Waves in a Solar Active Region Observed with FISS/GST and EIS/Hinode

Kyoung-Sun Lee, Jongchul Chae, Hannah Kwak +5

Elemental abundances in the solar corona differ from those in the photosphere, with low first ionization potential (FIP) elements being enhanced, a phenomenon known as the FIP effe…

astro-ph.SR2024

On the Nature of Nonthermal Broadening of Spectral Lines Observed by IRIS

Kyuhyoun Cho, Bart De Pontieu, Paola Testa

The origin of nonthermal broadening in solar spectra is one of the long-standing questions in solar physics. Various processes have been invoked - including unresolved flows, waves…

astro-ph.SR2024

A model of umbral oscillations inherited from subphotospheric fast-body modes

Juhyung Kang, Jongchul Chae, Kyuhyoun Cho +2

Recently, complex horizontal patterns of umbral oscillations have been reported, but their physical nature and origin are still not fully understood. Here we show that the two-dime…

astro-ph.SR2024

Large-amplitude transverse MHD waves prevailing in the H chromosphere of a solar quiet region revealed by MiHI integrated field spectral observations

Jongchul Chae, Michiel van Noort, Maria S. Madjarska +3

The investigation of plasma motions in the solar chromosphere is crucial for understanding the transport of mechanical energy from the interior of the Sun to the outer atmosphere a…