"Why Is the Sun So Hot?" | "Magnetic Waves Explained!" (Hindi)

"Scientists have long puzzled over the solar heating mystery – why the sun's corona is hundreds of times hotter than its visible surface. New research suggests that magnetic fields and small-scale waves known as kinetic Alfvén waves (KAWs) could be the key. Led by Syed Ayaz from the University of Alabama in Huntsville, this study proposes that as KAWs propagate through the sun's atmosphere, they dissipate and heat the corona. Discover how this groundbreaking research could solve the longstanding enigma of coronal heating and unlock new understanding of our closest star.