activity
20162026
most citedVerification of high-speed solar wind stream forecasts using operational solar wind models

96 citations · 210 across the 26 of their papers we have counts for

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Showing astro-ph.SRShow all

19 papers · 1 filter

astro-ph.SR2026

Tracing magnetic flux rope footpoints in AR 12975 with coronal dimmings and data-driven magnetofrictional simulations

Andreas Wagner, Amaia Razquin, Astrid M. Veronig +3

Coronal mass ejections (CMEs) are driven by the eruption of magnetic flux ropes (MFRs) whose footpoints are often observed indirectly as coronal dimming regions. However, the relat…

astro-ph.SR2026

Solar Soft X-ray Coronal Dimming in a Failed Eruption Associated with Plasma Cooling

Xinyue Wang, Astrid M. Veronig, Hechao Chen +1

Coronal dimmings are observed as sudden and localized reductions in the extreme-ultraviolet and X-ray emission of the solar corona. Traditionally, significant dimmings of spectral…

astro-ph.SR2026

The DIRECD coronal mass ejection direction catalog: three-dimensional propagation inferred from coronal dimmings

Shantanu Jain, Tatiana Podladchikova, Karin Dissauer +2

Coronal mass ejections (CMEs) are among the primary drivers of space weather disturbances at Earth, yet their early propagation in the low corona remains poorly constrained owing t…

astro-ph.SR2026

Stellar Forcing of (exo)Planetary Environments

Julián D. Alvarado-Gómez, Erika Palmerio, Manuel Güdel +13

The environments of exoplanets are fundamentally shaped by the magnetic activity of their host stars through radiative, plasma, and particle-driven processes. This article presents…

astro-ph.SR2026

Molecular hydrogen controls the temperatures of flares on TRAPPIST-1

Alexander I. Shapiro Nadiia Kostogryz Sara Seager Veronika Witzke Julien de Wit Valeriy Vasilyev Astrid M. Veronig Robert Cameron Hardi Peter Sami K. Solanki

Early JWST observations of TRAPPIST-1 have revealed an unexpected puzzle: energetic white-light flares ( erg) reach temperatures of only 3500--4000\,K, ne…

astro-ph.SR2025

New Bulgarian-Austrian project 'Joint observations and investigations of solar chromospheric and coronal activity'

Rositsa Miteva, Werner Pötzi, Astrid Veronig +9

We present the bilateral collaboration between Bulgarian and Austrian solar and space weather researchers on the topic of chromospheric and coronal activity. This new project will…

astro-ph.SR2025★ 1 cited

An analysis of the solar differential rotation in solar cycle No. 19 (1954-1964) determined using Kanzelhoehe sunspot group positions

Ivana Poljancic Beljan, Luka Sibenik, Tomislav Jurkic +7

We study solar differential rotation (DR) for solar cycle No. 19 (1954-1964) by tracing sunspot groups on the sunspot drawings of Kanzelhoehe Observatory for Solar and Environmenta…

astro-ph.SR2025★ 1 cited

Validating DIRECD: Statistical Evaluation of Coronal Mass Ejections Direction Estimates from Coronal Dimmings

Shantanu Jain, Tatiana Podladchikova, Karin Dissauer +2

Coronal mass ejections (CMEs) are among the most energetic phenomena in our solar system, with significant implications for space weather. Understanding their early dynamics remain…

astro-ph.SR2025★ 4 cited

Detecting Stellar Coronal Mass Ejections via Coronal Dimming in the Extreme Ultraviolet

James Paul Mason, Allison Youngblood, Kevin France +2

Stellar flares and coronal mass ejections (CMEs) can strip planetary atmospheres, reducing the potential habitability of terrestrial planets. While flares have been observed for de…

astro-ph.SR2025

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections

Astrid M. Veronig, Karin Dissauer, Bernhard Kliem +10

Coronal dimmings associated with coronal mass ejections (CME) from the Sun have gained much attention since the late 1990s when they were first observed in high-cadence imagery of…

astro-ph.SR2024★ 9 cited

Solar flares in the Solar Orbiter era: Short-exposure EUI/FSI observations of STIX flares

Hannah Collier, Laura A. Hayes, Stefan Purkhart +10

Aims: This paper aims to demonstrate the importance of short-exposure extreme ultraviolet (EUV) observations of solar flares in the study of particle acceleration, heating and ener…

astro-ph.SR2024

Recovery of coronal dimmings

Giulia M. Ronca, Galina Chikunova, Karin Dissauer +2

Coronal dimmings are regions of reduced emission in the lower corona, observed after coronal mass ejections (CMEs) and representing their footprints. In order to investigate the lo…

astro-ph.SR2024

High-resolution Observation of Blowout Jets Regulated by Sunspot Rotation

Tingyu Gou, Rui Liu, Yang Su +4

Coronal jets are believed to be the miniature version of large-scale solar eruptions. In particular, the eruption of a mini-filament inside the base arch is suggested to be the tri…

astro-ph.SR2024

Sun-as-a-star observations of obscuration dimmings caused by filament eruptions

Yu Xu, Hui Tian, Astrid M. Veronig +1

Filament eruptions often lead to coronal mass ejections (CMEs) on the Sun and are one of the most energetic eruptive phenomena in the atmospheres of other late-type stars. However,…

astro-ph.SR2024★ 28 cited

A Universal Method for Solar Filament Detection from H-alpha Observations using Semi-supervised Deep Learning

Andrea Diercke, Robert Jarolim, Christoph Kuckein +7

Filaments are omnipresent features in the solar atmosphere. Their location, properties and time evolution can provide information about changes in solar activity and assist the ope…

astro-ph.SR2024

A Modelling Investigation for Solar Flare X-ray Stereoscopy with Solar Orbiter/STIX and Earth Orbiting Missions

Natasha L. S. Jeffrey, Säm Krucker, Morgan Stores +9

The Spectrometer/Telescope for Imaging X-rays (STIX) on board Solar Orbiter (SolO) provides a unique opportunity to systematically perform stereoscopic X-ray observations of solar…

astro-ph.SR2023★ 25 cited

The existence of hot X-ray onsets in solar flares

Andrea Francesco Battaglia, Hugh Hudson, Alexander Warmuth +9

It is well known among the scientific community that solar flare activity often begins well before the main impulsive energy release. Our aim is to investigate the earliest phase o…

astro-ph.SR2022★ 14 cited

Variation in solar differential rotation and activity in the period 1964-2016 determined by the Kanzelhöhe data set

I. Poljančić Beljan, R. Jurdana-Šepić, T. Jurkić +8

We determined the differential rotation (DR) parameters and (corresponding to the equatorial rotation velocity and the gradient of the solar DR) by tracing sunspot groups i…

astro-ph.SR2016★ 6 cited

Temporal and spatial relationship of flare signatures and the force-free coronal magnetic field

Julia K. Thalmann, Astrid M. Veronig, Yang Su

We investigate the plasma and magnetic environment of active region NOAA 11261 on 2 August 2011 around a GOES M1.4 flare/CME (SOL2011-08-02T06:19). We compare coronal emission at (…