activity
20242026
collaborators

5 papers

astro-ph.SR2026

Comprehensive MHD modelling of ten successive CMEs driving a historic geomagnetic storm -- The 2024 Mothers Day event

Shirsh Lata Soni, Anwesha Maharana, Sanchita Pal +1

Interacting coronal mass ejections (CMEs) result in complex heliospheric structures that can dramatically enhance their geoeffectiveness compared to isolated events. A striking exa…

astro-ph.SR2025

Rotation of flux ropes in the low corona

Brigitte Schmieder, Anwesha Maharana, Jin Han Guo +2

Eruptions of filaments are defined by different parameters, specially, sigmoid handedness and direction of the eruption, which are important parameters for forecasting the geoeffec…

astro-ph.SR2025

Flare energetics, CME launch and heliospheric propagation for the May 2024 events, as derived from ensemble MHD modelling

Brigitte Schmieder, Jinhan Guo, Guillaume Aulanier +2

Many questions must be answered before understanding the relationship between the emerging magnetic flux through the solar surface and the extreme geoeffective events. The main ing…

physics.space-ph2024

Toroidal modified Miller-Turner CME model in EUHFORIA: II. Validation and comparison with flux rope and spheromak

Anwesha Maharana, Luis Linan, Stefaan Poedts +1

Rising concerns about the impact of space weather-related disruptions demand modelling and reliable forecasting of coronal mass ejection (CME) impacts. In this study, we demonstrat…

astro-ph.SR2024

Validation of EUHFORIA cone and spheromak Coronal Mass Ejection Models

L. Rodriguez, D. Shukhobodskaia, A. Niemela +15

Aims. We present the validation results for arrival times and geomagnetic impact of Coronal Mass Ejections (CMEs), using the cone and spheromak CME models implemented in EUropean H…