Magnetic Waves The Sun's Secret Heat
Beneath the Sun’s blazing surface lies a mystery that has puzzled scientists for decades — why is the Sun’s outer atmosphere, the corona, millions of degrees hotter than its surface? Magnetic Waves: The Sun’s Secret Heat explores this cosmic enigma through the lens of magnetohydrodynamics, where powerful magnetic fields twist, snap, and ripple through solar plasma. These magnetic waves — known as Alfvén waves — carry immense energy from the Sun’s interior and may hold the key to explaining the Sun’s extreme coronal temperatures. Journey into the heart of solar physics to uncover how invisible magnetic vibrations heat the solar atmosphere, drive solar winds, and shape space weather that reaches Earth.
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