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Deformation of the CME and CME-driven shock due to interaction with the ambient solar wind: I. Modelling with Cone Model
A. Niemela, A. Valentino, J. Magdalenic
Context. The near-Earth environment is continuously impacted by the solar wind and the transients embedded in it. The largest eruptions of plasma and magnetic field at the Sun are…
Modelling non-radially propagating coronal mass ejections and forecasting the time of their arrival at Earth
Angelos Valentino, Jasmina Magdalenic
We present the study of two solar eruptive events observed on December 7 2020 and October 28 2021.Both events were associated with full halo CMEs and flares.These events were chose…
Study with WhoSGlAd of the acoustic depth of the helium glitch across the seismic HR diagram and its impact on the inferred helium abundance
Martin Farnir, Angelo Valentino, Marc-Antoine Dupret +1
The acoustic glitches' signature present in solar-like stars holds invaluable information. Indeed, it is caused by a sharp variation in the sound speed, therefore carrying localise…