activity
20222026
most citedOver-expansion of coronal mass ejections modelled using 3D MHD EUHFORIA simulations

12 citations · 25 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2026

Evidence of global periodicity in PSP data: can they be linked to long-period oscillations in solar active regions?

G. Dumbadze, B. M. Shergelashvili, M. Khodachenko +4

The presence of coherent oscillatory signatures in Parker Solar Probe SWEAP datasets, identified through a series of spectral analyses, is addressed, and their possible connection…

physics.space-ph2026

Advancing Heliophysics and Space Weather Modeling through Open Science

C. Corti, M. M. Kuznetsova, M. A. Reiss +85

We present a community-wide effort to develop a strategy and action plan to advance heliophysics and space weather modeling through open science. While open science has the potenti…

astro-ph.SR2026

Assessing VBz variations during CME propagation: a preparatory study for the HENON mission using EUHFORIA

G. Prete, A. Niemela, S. Poedts +21

Coronal mass ejections (CMEs) are among the main drivers of space weather hazards. In this context, HENON is a new space mission designed to carry out observations in the solar win…

astro-ph.SR2026

On the Constraints and Observational Manifestations of Failed Solar Eruptions in Toroidal Magnetic Cage

Jinhan Guo, Y. Guo, H. Wu +9

Observations show that many solar eruptions remain confined within strong overlying magnetic fields, forming a so-called magnetic cage. While confinement by poloidal overlying fiel…

astro-ph.SR2025★ 2 cited

Investigating the impact of the dynamic solar wind on the propagation of a coronal mass ejection with two models and multi-spacecraft measurements

Tinatin Baratashvili, Emma Davies, Eva Weiler +3

Coronal mass ejections (CMEs) are the main drivers of disturbances in the solar heliosphere because they propagate and interact with the magnetic field of the solar wind. It is cru…

astro-ph.SR2024★ 6 cited

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…

astro-ph.SR2024

Wide-band fluctuations of solar active regions probed with SHARP magnetograms

G. Dumbadze, B. M. Shergelashvili, M. L. Khodachenko +1

The power spectra of the fluctuation noise of the solar active region (AR) areas and magnetic fluxes sequentially observed in time contain information about their geometrical featu…

astro-ph.SR2022★ 12 cited

Over-expansion of coronal mass ejections modelled using 3D MHD EUHFORIA simulations

C. Verbeke, B. Schmieder, P. Démoulin +5

Coronal mass ejections (CMEs) are large scale eruptions observed close to the Sun. They are travelling through the heliosphere and possibly interacting with the Earth environment c…

astro-ph.SR2022★ 5 cited

Interaction of coronal mass ejections and the solar wind. A force analysis

Dana-Camelia Talpeanu, Stefaan Poedts, Elke D'Huys +2

Aims. Our goal is to thoroughly analyse the dynamics of single and multiple solar eruptions, as well as a stealth ejecta. The data were obtained through self-consistent numerical s…