Evershed effect
Quick Summary
The Evershed effect, discovered by English astronomer John Evershed in 1909, describes the outward horizontal motion of gases from the centers of sunspots. Sunspots are cooler, darker regions on the Sun's surface associated with strong magnetic fields.123
Within a sunspot, the dark central area is called the umbra, surrounded by a lighter ring known as the penumbra. The Evershed effect is observed in the penumbra, where gases flow outward at about one kilometer per second. In the chromosphere above a sunspot, a reverse flow occurs, with material spiraling inward. This phenomenon is a key aspect of understanding the complex dynamics within sunspots and their associated magnetic activity.32
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