activity
20132026
most citedPositive and negative feedback of AGN outflows in NGC 5728

93 citations · 292 across the 22 of their papers we have counts for

collaborators

23 papers

astro-ph.SR2026

Evidence for anisotropic non-Maxwellian velocity distributions in the solar transition region

Paola Testa, Bart De Pontieu, Kyuhyoun Cho +2

Spectroscopic observations of the solar transition region have long shown excess line broadening and non-Gaussian profiles, but their spatial distribution and prevalence are not we…

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★ 5 cited

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★ 2 cited

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★ 6 cited

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…

astro-ph.SR2022★ 12 cited

A Statistical Study of IRIS Observational Signatures of Nanoflares and Non-thermal Particles

Kyuhyoun Cho, Paola Testa, Bart De Pontieu +1

Nanoflares are regarded as one of the major mechanisms of magnetic energy release and coronal heating in the solar outer atmosphere. We conduct a statistical study on the response…

astro-ph.SR2021★ 4 cited

Investigation of the subsurface structure of a sunspot based on the spatial distribution of oscillation centers inferred from umbral flashes

Kyuhyoun Cho, Jongchul Chae, Maria S. Madjarska

The subsurface structure of a solar sunspot is important in the stability of the sunspots and the energy transport therein. Two subsurface structure models have been proposed, the…

astro-ph.SR2020

The chromospheric component of coronal bright points. Coronal and chromospheric responses to magnetic-flux emergence

Maria S. Madjarska, Jongchul Chae, Fernando Moreno-Insertis +5

We investigate the chromospheric counterpart of small-scale coronal loops constituting a coronal bright point (CBP) and its response to a photospheric magnetic-flux increase accomp…

astro-ph.SR2020★ 1 cited

Impulsive wave excitation by rapidly changing granules

Hannah Kwak, Jongchul Chae, Maria S. Madjarska +2

It is not yet fully understood how magnetohydrodynamic waves in the interior and atmosphere of the Sun are excited. Traditionally, turbulent convection in the interior is considere…

astro-ph.SR2020

Inference of chromospheric plasma parameters on the Sun

Jongchul Chae, Maria S. Madjarska, Hannah Kwak +1

The solar chromosphere can be observed well through strong absorption lines. We infer the physical parameters of chromospheric plasmas from these lines using a multilayer spectral…

astro-ph.SR2020★ 5 cited

The Application of the Filtered Backprojection Algorithm to Solar Rotational Tomography

Kyuhyoun Cho, Jongchul Chae, Ryun-Young Kwon +2

Solar rotational tomography (SRT) is an important method to reconstruct the physical parameters of the three-dimensional solar corona. Here we propose an approach to apply the filt…

astro-ph.SR2020★ 21 cited

Strong Blue Asymmetry in Hα line as a Preflare Activity

Kyuhyoun Cho, Jeongwoo Lee, Jongchul Chae +5

Chromospheric activities prior to solar flares provide important clues to solar flare initiation, but are as yet poorly understood. We report a significant and rapid H line broa…

astro-ph.SR2020★ 13 cited

Source Depth of Three-minute Umbral Oscillations

Kyuhyoun Cho, Jongchul Chae

We infer the depth of the internal sources giving rise to three-minute umbral oscillations. Recent observations of ripple-like velocity patterns of umbral oscillations supported th…

astro-ph.GA2019★ 93 cited

Positive and negative feedback of AGN outflows in NGC 5728

Jaejin Shin, Jong-Hak Woo, Aeree Chung +4

We present a spatially-resolved analysis of ionized and molecular gas in a nearby Seyfert 2 galaxy NGC 5728, using the VLT/MUSE and ALMA data. We find ionized gas outflows out to ~…

astro-ph.SR2019★ 12 cited

The Observational Evidence for the Internal Excitation of Sunspot Oscillations Inferred from the Fe I 5435 A Line

Kyuhyoun Cho, Jongchul Chae, Eun-kyung Lim +1

The umbral oscillations of velocity are commonly observed in the chromosphere of a sunspot. Their sources are considered to be either the external p-mode driving or the internal ex…

astro-ph.SR2019★ 26 cited

The Physical Nature of Spiral Wave Patterns in Sunspots

Juhyung Kang, Jongchul Chae, Valery M. Nakariakov +3

Recently, spiral wave patterns (SWPs) have been detected in 3 minute oscillations of sunspot umbrae, but the nature of this phenomenon has remained elusive. We present a theoretica…

astro-ph.SR2017★ 8 cited

Observation of a Large-scale Quasi-circular Secondary Ribbon associated with Successive Flares and a Halo CME

Eun-Kyung Lim, Vasyl Yurchyshyn, Pankaj Kumar +7

Solar flare ribbons provide an important clue to the magnetic reconnection process and associated magnetic field topology in the solar corona. We detected a large-scale secondary f…

astro-ph.SR2017★ 23 cited

Chromospheric Plasma Ejections in a Light Bridge of a Sunspot

Donguk Song, Jongchul Chae, Vasyl Yurchyshyn +5

It is well-known that light bridges inside a sunspot produce small-scale plasma ejections and transient brightenings in the chromosphere, but the nature and origin of such phenomen…

astro-ph.SR2016

A New Method to Determine the Temperature of CMEs Using a Coronagraph Filter System

Kyuhyoun Cho, Jongchul Chae, Eun-kyung Lim +3

The coronagraph is an instrument enables the investigation of faint features in the vicinity of the Sun, particularly coronal mass ejections (CMEs). So far coronagraphic observatio…

astro-ph.SR2016★ 42 cited

Ultra-narrow Negative Flare Front Observed in Helium-10830~Å using the 1.6 m New Solar Telescope

Yan Xu, Wenda Cao, Mingde Ding +10

Solar flares are sudden flashes of brightness on the Sun and are often associated with coronal mass ejections and solar energetic particles which have adverse effects in the near E…

astro-ph.SR2015★ 19 cited

Observations of a Series of Flares and Associated Jet-like Eruptions Driven by the Emergence of Twisted Magnetic Fields

Eun-Kyung Lim, Vasyl Yurchyshyn, Sung-Hong Park +8

We studied temporal changes of morphological and magnetic properties of a succession of four confined flares followed by an eruptive flare using the high-resolution New Solar Teles…

astro-ph.SR2013

Chromospheric Sunspot Oscillations in H-alpha and Ca II 8542A

Ram Ajor Maurya, Jongchul Chae, Hyungmin Park +3

We study chromospheric oscillations including umbral flashes and running penumbral waves in a sunspot of active region (AR) using scanning spectroscopy in H-alpha and Ca II 8542A,…