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Project
Modelling of solar coronal oscillations
The research about the modelling of waves in the solar corona is conducted. In particular, global models for the solar corona, in which we model large-scale waves in coronal streamers, are constructed. These waves are excited by coronal mass ejections and allow to measure the magnetic field and speed of the solar wind with the aid of seismology.
Date:19 Oct 2021 → Today
Keywords:Solar Physics, Solar corona
Disciplines:Space plasma physics and solar physics
Project type:PhD project