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Churning Prominence


A solar prominence rose up along the edge of the sun and twisted and churned for about two days before falling apart (Jan. 23-24, 2017). The dynamic action was generated by competing magnetic forces. The images were taken in a wavelength extreme ultraviolet light that observes activity close to the solar surface, perfect for capturing prominences, which are notoriously unstable clouds of plasma suspended above the sun. Credit: Solar Dynamic Observatory, NASA.

Search Tag(s): aia, 304, prominence




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