1.4k citations · 5k across the 61 of their papers we have counts for
62 papers
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…
Improving Solar EUV Irradiance Modeling with Differential Emission Measure Informed Spectra
Courtney L. Peck, Shah M. Bahauddin, Daniel B. Seaton +3
Solar extreme ultraviolet (EUV) irradiance predominantly originates from the chromosphere and corona, and variations in EUV irradiance are a significant driver of space weather at…
Machine learning in solar physics
A. Asensio Ramos, M. C. M. Cheung, I. Chifu +1
The application of machine learning in solar physics has the potential to greatly enhance our understanding of the complex processes that take place in the atmosphere of the Sun. B…
Hybrid data-driven magnetofrictional and magnetohydrodynamic simulations of an eruptive solar active region
A. Afanasyev, Y. Fan, M. Kazachenko +1
We present first results of the hybrid data-driven magnetofrictional (MF) and data-constrained magnetohydrodynamic (MHD) simulations of solar active region NOAA 11158, which produc…
Comprehensive radiative MHD simulations of eruptive flares above collisional polarity inversion lines
Matthias Rempel, Georgios Chintzoglou, Mark C. M. Cheung +2
We present a new simulation setup using the MURaM radiative Magnetohydrodynamic (MHD) code that allows to study the formation of collisional polarity inversion lines (cPILs) in the…
Surface Flux Transport on the Sun
Anthony R. Yeates, Mark C. M. Cheung, Jie Jiang +2
We review the surface flux transport model for the evolution of magnetic flux patterns on the Sun's surface. Our underlying motivation is to understand the model's prediction of th…