
Aditya-L1 uncovers magnetic fix behind the Sun's scorching corona
New findings from India's Aditya-L1 mission show the Sun's outer atmosphere, the corona, is heated mainly by magnetic-field-line reconnection (≈93%), with surface waves contributing about 7%. By analyzing a highly energetic CME on 5 August 2024, scientists quantified energy replenishment and confirmed the corona remains exceptionally hot despite repeated eruptions; the results, published in Astrophysical Journal Letters, provide a key benchmark for solar physics.













