Time-evolving model of the solar corona
Changes in the magnetic structures of the solar corona over the past days. Colours represent the polarity of the coronal magnetic field.
European Space Agency
ESA Space Weather Office - Eclipse prediction campaign
Live predictions of the total solar eclipse based on the numerical simulations of the COCONUT coronal model of KU Leuven.
Changes in the magnetic structures of the solar corona over the past days. Colours represent the polarity of the coronal magnetic field.
Solar light scattered towards the observers. Bright areas correspond to dense coronal structures extending into space.
Magnetic structures brought in evidence by processing of the coronal simulations.
Live transmission of the ESA Eclipse 2026 event from Leon, Spain