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Solar Flares: From Emergence To Eruption

This visualization is an animation of the solar flare modeled in the new study. The violet color represent plasma with temperature less than 1 million Kelvin. Red represents temperatures between 1 million and 10 million Kelvin, and green represents temperatures above 10 million Kelvin. Image Credit: Mark Cheung and Matthias Rempel

January 14, 2019 – A team of scientists has, for the first time, used a single, cohesive computer model to simulate the entire life cycle of a solar flare: from the buildup of energy thousands of kilometers below the solar surface, to the emergence of tangled magnetic field lines, to the explosive release of energy in a brilliant flash. Read More

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