HELIOSKILL: Heliophysics simulations and artificial intelligence KU Leuven
One of the most important open questions in astrophysics is explaining why the solar wind is so hot. The solar surface is at about 6500K but quickly as one moves in the atmosphere of the Sun the temperature reaches millions of degrees and continues to increase more gently at larger distances before slowly starting to decrease. This goes against any intuition for an expanding gas that moves away from its source of heating. Two new missions ...