A coronal mass ejection encountered by four spacecraft within 1 au from the Sun: ensemble modelling of propagation and magnetic structure
E Palmerio, C Kay, N Al-Haddad… - Monthly Notices of …, 2025 - academic.oup.com
Understanding and predicting the structure and evolution of coronal mass ejections (CMEs)
in the heliosphere remains one of the most sought-after goals in heliophysics and space …
in the heliosphere remains one of the most sought-after goals in heliophysics and space …
[HTML][HTML] Toroidal modified Miller-Turner CME model in EUHFORIA: Validation and comparison with flux rope and spheromak
A Maharana, L Linan, S Poedts… - Astronomy & …, 2024 - aanda.org
Context. Rising concerns about the impact of space-weather-related disruptions demand
modelling and reliable forecasting of coronal mass ejection (CME) impacts. Aims. In this …
modelling and reliable forecasting of coronal mass ejection (CME) impacts. Aims. In this …
Solar Active Regions Emergence Prediction Using Long Short-Term Memory Networks
S Kasapis, IN Kitiashvili, AG Kosovichev… - arXiv preprint arXiv …, 2024 - arxiv.org
We developed Long Short-Term Memory (LSTM) models to predict the formation of active
regions (ARs) on the solar surface. Using the Doppler shift velocity, the continuum intensity …
regions (ARs) on the solar surface. Using the Doppler shift velocity, the continuum intensity …