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19992026
most citedA Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953

388 citations · 2.3k across the 58 of their papers we have counts for

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37 papers · 1 filter

astro-ph.SR2026

Direct Numerical Comparison of Data Driving Strategies for Solar Flux Emergence in Magnetohydrodynamics: B-driving vs E-driving

Kyriakos Christos Tapinou, Axel Raboonik, David I. Pontin +3

Data driving is an important technique for modelling realistic magnetic field and plasma evolution in regions of the solar atmosphere where direct observations are either absent or…

astro-ph.SR2026

Validating Coronal Magnetic Field Models Using Gaussian Separation

Abhinav G. Iyer, Michael S. Wheatland, Brian T. Welsch +2

Nonlinear Force-free Field (NLFFF) models are widely used to investigate coronal magnetic field structure in solar active regions, but methods to validate them remain limited. Here…

astro-ph.SR2026★ 1 cited

A Convolutional Neural Network-Derived Catalog of Solar Flares from Soft X-Ray Observations

Nastaran Farhang, Michael. S. Wheatland, Andrew Melatos

A convolutional neural network (CNN) is used to construct a new catalog for solar flares based on high resolution (1-s cadence) Geostationary Operational Environmental Satellites (…

astro-ph.SR2023

Multi-epoch sampling of the radio star population with the Australian SKA Pathfinder

Joshua Pritchard, Tara Murphy, George Heald +5

The population of radio-loud stars has to date been studied primarily through either targeted observations of a small number of highly active stars or widefield, single-epoch surve…

astro-ph.SR2023

Complex Network View of the Sun's Magnetic Patches: I. Identification

Zahra Tajik, Nastaran Farhang, Hossein Safari +1

Solar and stellar magnetic patches (i.e., magnetic fluxes that reach the surface from the interior) are believed to be the primary sources of a star's atmospheric conditions. Hence…

astro-ph.SR2023★ 3 cited

A statistical search for a uniform trigger threshold in solar flares from individual active regions

Julian B. Carlin, Andrew Melatos, Michael S. Wheatland

Solar flares result from the sudden release of energy deposited by sub-photospheric motions into the magnetic field of the corona. The deposited energy accumulates secularly betwee…