In the Solar Furnace: Latest Results from Solar Orbiter and Parker Solar Probe

24 September 2024
18 h 00 min | 19 h 30 min
Médiathèque José Cabanis (Grand Auditorium)
1 All. Jacques Chaban-Delmas - 31500 - Toulouse - (France)

By Alexis Rouillard, CNRS researcher, IRAP and Philippe Louarn, CNRS research director, IRAP

Why is the Sun’s atmosphere two hundred times hotter than its surface? How are solar winds and thunderstorms created? To answer these major questions in astrophysics, the Parker Solar Probe and Solar Orbiter space probes set out in 2018 and 2020 to discover the environment close to the Sun: the solar corona. After several years of observations, they have highlighted, very close to the Sun, an extremely dynamic environment constantly disturbed by ejections of material and thus provide new clues to the formation of solar winds and storms.


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