2 papers
astro-ph.SR2026
Neural Differential Equations for the Solar Dynamo
E. Illarionov, R. Stepanov, K. M. Kuzanyan +1
Physical models aimed to reproduce basic features of the solar sunspot cycle are typically based on the solar dynamo mechanism. Usually qualitative arguments are used to define par…
cs.LG2024
Machine learning for reconstruction of polarity inversion lines from solar filaments
V. Kisielius, E. Illarionov
Solar filaments are well-known tracers of polarity inversion lines that separate two opposite magnetic polarities on the solar photosphere. Because observations of filaments began…