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Magnetic plasma pulses excited by UK-size swirls in the solar atmosphere


The photospheric and chromospheric images were recorded with the Hinode satellite, while coloured lines between are visualizing the presence of magnetic field lines from the researchers' realistic numerical simulations using the Sheffield Advanced Code (SAC). Red and blue curves are swirls detected by the Automated Swirl Detection Algorithm (ASDA) developed by the researchers. (Credit: Liu et al. Nature Communications, 10:3504, 2019)

An international team of scientists led by the University of Sheffield have discovered previously undetected observational evidence of frequent energetic wave pulses the size of the UK, transporting energy from the solar surface to the higher solar atmosphere.

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