activity
20242026
most citedUsing the STIX background detector as a proxy for GOES

13 citations · 28 across the 10 of their papers we have counts for

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Showing 2026Show all

6 papers · 1 filter

astro-ph.SR2026

First results from PADRE/MeDDEA: X-rays from a flare and its CME

Muriel Zoë Stiefel, Säm Krucker, Olivier Limousin +22

The MeDDEA hard X-ray spectrometer onboard NASAs PADRE CubeSat operates four flight-spare detectors from the Solar Orbiter/STIX instrument. This paper aims to evaluate the accuracy…

astro-ph.SR2026

Count-based spectral component imaging (CCI) of solar flares in X-rays

Alessia Guidetti, Muriel Zoë Stiefel, Paolo Massa +3

X-ray emission in solar flares is produced by both multi-thermal plasma and accelerated electrons. Classical imaging approaches reconstruct X-ray intensity maps which contain contr…

astro-ph.SR2026

Fine-scale flare structures and their energetic implications from short-exposure extreme-ultraviolet imaging

Laura A. Hayes, Hannah Collier, Säm Krucker +5

To capture the brightest and most rapidly evolving phases of solar flares, the Major Flare Solar Orbiter Observing Plan employed a dedicated short-exposure mode for the High Resolu…

astro-ph.SR2026

Non-thermal Sources from Stereoscopic Hard X-ray and Earth-based Microwave Observations in a Data-Constrained Magnetohydrodynamic Simulation

Keitarou Matsumoto, Satoshi Inoue, Meiqi Wang +5

We analyze the X7.1 flare on 2024 October 1 from NOAA AR 13842 using hard X-ray (HXR) imaging, microwave observations by the Expanded Owens Valley Solar Array (EOVSA), and a three-…

astro-ph.SR2026

The Non-Eruptive Reconfiguration of a Quiescent Filament After a Nearby Active Region Emergence

James McKevitt, Louise Harra, Gherardo Valori +13

The unpredictability of solar filament eruptions presents major challenges for forecasting space weather, as such eruptions frequently drive coronal mass ejections (CMEs) that impa…

astro-ph.SR2026★ 2 cited

Stereoscopic Observations of Solar X-ray Sources Explained by a Data-Constrained Magnetohydrodynamic Simulation

Keitarou Matsumoto, Satoshi Inoue, Meiqi Wang +6

We investigated the three-dimensional (3D) magnetic structures and dynamics responsible for particle acceleration in an X7.1-class flare that occurred on October 1, 2024, in NOAA a…