output
19982026
most citedA Database of Flare Ribbon Properties From Solar Dynamics Observatory I: Reconnection Flux

144 citations

21 papers

cs.CV2026

Pixel-Level Pavement Distress Assessment Using Instance Segmentation

Logan Dewick, Bibesh Pyakurel, Kong Pheng Yang +2

Automated pavement distress assessment requires more than image-level classification or coarse bounding box detection, demanding precise localization of thin, branching, and irregu…

math.OC2026

Reconfiguring flexibility in renewable power-to-ammonia systems using molten-salt thermal energy storage in the ammonia synthesis loop: A coordinated electro-hydrogen-thermal scheduling approach

Yiwei Qiu, Qingjie Sun, Yangjun Zeng +7

In renewable power-to-ammonia (ReP2A) systems, the intermittency of wind and solar generation propagates through electrolytic hydrogen production and induces thermal instability in…

astro-ph.SR2025★ 2 cited

Multi-height probing of horizontal flows in the solar photosphere

Teodor Kostić, Ivan Milić, Matthias Rempel +4

We tested whether simultaneous spectropolarimetric imaging in two magnetically sensitive optical spectral lines, which probe two different layers of the solar atmosphere (the photo…

cs.CV2025

Conditional Synthetic Live and Spoof Fingerprint Generation

Syed Konain Abbas, Sandip Purnapatra, M. G. Sarwar Murshed +5

Large fingerprint datasets, while important for training and evaluation, are time-consuming and expensive to collect and require strict privacy measures. Researchers are exploring…

astro-ph.SR2022

Photospheric Imprints of Coronal Electric Currents, I. Magnetic Structure Near Polarity Inversion Lines

Brian T. Welsch, Peter W. Schuck, Mark G. Linton

Flares and coronal mass ejections (CMEs) are powered by magnetic energy stored in coronal electric currents. Here, we use photospheric vector magnetic field observations to study c…

astro-ph.SR2022

Reconstruction of photospheric velocity fields from highly corrupted data

Erico L. Rempel, Roman Chertovskih, Kamilla R. Davletshina +3

The analysis of the photospheric velocity field is essential for understanding plasma turbulence in the solar surface, which may be responsible for driving processes such as magnet…