activity
20022026
most citedAn Observational Overview of Solar Flares

850 citations · 6.8k across the 110 of their papers we have counts for

collaborators

110 papers

physics.space-ph2026

P2D - A Two-Dimensional Multi-Spacecraft Solar Wind Persistence Model

Daniel Milošić, Manuela Temmer, Stephan G. Heinemann +2

The background solar wind is a key component in space weather forecasting, as it contains geoeffective high-speed streams and provides the medium through which coronal mass ejectio…

astro-ph.SR2026

Comparative 3D Asymmetric Expansion and Angular Widths Evolution of Fast and Slow Coronal Mass Ejections

Anjali Agarwal, Wageesh Mishra, Jie Zhang +2

The radial and lateral dimensions of coronal mass ejections (CMEs) influence their duration and probability of encounter at Earth. These properties are linked to the expansion spee…

astro-ph.SR2026★ 1 cited

Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes

Suresh Karuppiah, Mateja Dumbović, Karmen Martinić +3

We investigate the deflection and rotation behavior of 49 Earth-directed coronal mass ejections (CMEs) spanning the period from 2010 to 2020 aiming to understand the potential infl…

astro-ph.IM2025

Millimeter-Wavelength Observations of the Active Sun: Unveiling the Origins of Space Weather

Sven Wedemeyer, Stefaan Poedts, Stanislav Gunár +15

Societal dependence on space-based services demands major advances in predicting the impacts of eruptive solar events. Millimeter-wavelength observations offer uniquely direct acce…

astro-ph.SR2025

Formation of a Coronal Hole by a quiet-Sun Filament Eruption

Stefan J. Hofmeister, Eleanna Asvestari, Karin Dissauer +9

A coronal hole formed as a result of a quiet-Sun filament eruption close to the solar disk center on 2014 June 25. We studied this formation using images from the Atmospheric Imagi…

astro-ph.SR2024★ 7 cited

The Link Between Non-Thermal Velocity and Free Magnetic Energy in Solar Flares

James McKevitt, Robert Jarolim, Sarah Matthews +5

The cause of excess spectral line broadening (non-thermal velocity) is not definitively known, but given its rise before and during flaring, the causal processes hold clues to unde…