activity
20162026
most citedUnderstanding the Physical Nature of Coronal "EIT Waves"

92 citations · 232 across the 37 of their papers we have counts for

collaborators
Showing 2025Show all

11 papers · 1 filter

astro-ph.SR2025

Height and Energy Evolution of X-ray Double Sources in a Solar Flare

Hanya Pan, Astrid M. Veronig, Rui Liu

In the standard model, magnetic reconnection at a vertical current sheet above the flare arcade is key to explaining many aspects of solar eruptions. The supra-arcade region is whe…

astro-ph.SR2025

Height-dependent thermal properties of extreme-ultraviolet campfires in the quiet Sun

O. Podladchikova, A. Warmuth, L. Harra +30

Small-scale impulsive energy-release events are widely considered a key ingredient of quiet-Sun coronal heating. We quantified the thermal-energy content of extreme-ultraviolet (EU…

astro-ph.SR2025

Coronal mass ejection arrival forecasting with the drag-based assimilation of satellite observations

Zaina Abu-Shaar, Tatiana Podladchikova, Astrid M. Veronig +2

Forecasting the arrival of coronal mass ejections (CMEs) is vital for protecting satellites, power systems, and human spaceflight. We present HELIOPANDA: Heliospheric Observer for…

astro-ph.SR2025

Image calibration between the Extreme Ultraviolet Imagers on Solar Orbiter and the Solar Dynamics Observatory

Christoph Schirninger, Robert Jarolim, Astrid M. Veronig +6

To study and monitor the Sun and its atmosphere, various space missions have been launched in the past decades. With the rapid improvement in technology and different mission requi…

astro-ph.SR2025

Magnetic structure and asymmetric eruption of a 500 Mm filament rooted in weak-field regions

Stefan Purkhart, Astrid M. Veronig, Robert Jarolim +2

We performed a detailed analysis of the magnetic structure and asymmetric eruption of a large (about 500 Mm) inverse S-shaped filament partially located in AR 13229 on February 24,…

astro-ph.EP2025

Flares on TRAPPIST-1 reveal the spectrum of magnetic features on its surface

Valeriy Vasilyev, Nadiia Kostogryz, Alexander I. Shapiro +11

TRAPPIST-1 is an M8 dwarf hosting seven known exoplanets and is currently one of the most frequently observed targets of the James Webb Space Telescope (JWST). However, it is notor…

astro-ph.SR2025★ 2 cited

Extreme ultraviolet late-phase flares as observed by EVE and AIA on board the Solar Dynamics Observatory

Sascha Ornig, Astrid M. Veronig, Karin Dissauer

Context. Extreme ultraviolet (EUV) late-phase (ELP) flares exhibit a second peak in warm coronal emissions minutes to hours after the main peak of the flare. This phase is all but…

astro-ph.SR2025★ 5 cited

Coronal dimmings from active region 13664 during the May 2024 solar energetic events

Amaia Razquin, Astrid M. Veronig, Karin Dissauer +2

Coronal dimmings are regions of transiently reduced brightness in extreme ultraviolet (EUV) and soft X-ray (SXR) emissions associated with coronal mass ejections (CMEs), providing…

astro-ph.SR2025★ 7 cited

Deep learning image burst stacking to reconstruct high-resolution ground-based solar observations

Christoph Schirninger, Robert Jarolim, Astrid M. Veronig +1

Large aperture ground based solar telescopes allow the solar atmosphere to be resolved in unprecedented detail. However, observations are limited by Earths turbulent atmosphere, re…

astro-ph.SR2025

Spatiotemporal evolution of UV pulsations and their connection to 3D magnetic reconnection and particle acceleration

Stefan Purkhart, Hannah Collier, Laura A. Hayes +3

Quasi-periodic pulsations (QPPs) are a common feature of impulsive solar flare emissions, yet their driving mechanism(s) remain unresolved. We study long-period (3.4 min) QPPs in t…

astro-ph.SR2025

Conditioning of the solar corona due to large flares

Julia K. Thalmann, Manu Gupta, Astrid M. Veronig +1

We aim to better characterize the conditions of the solar corona, especially with respect to the occurrence of confined and eruptive flares. In this work, we model the coronal evol…