The Sun’s outer layer, the corona, is millions of degrees hotter than its surface. That shouldn’t be possible; yet it is. Every time a solar storm blasts out, the Sun loses insane amounts of energy… and yet, it never cools down. Turns out, it’s not the waves from bubbling surface activity doing most of the work. Just 7% of the heat comes from that. The real hero? The Sun’s tangled magnetic field; constantly snapping, reconnecting, and pumping back 93% of the lost energy within hours. Thanks to Aditya-L1’s advanced sensors, we now have proof. This isn’t just space trivia; it helps us predict solar storms that could knock out satellites, power grids, and GPS. India’s solar mission didn’t just watch the Sun. It started decoding its secrets.