Non-thermal broadening of IRIS Fe XXI line caused by turbulent plasma flows in the magnetic reconnection region during solar eruptions

Overview of attention for article published in Frontiers in Astronomy and Space Sciences, February 2023

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Frontiers | Non-thermal broadening of IRIS Fe XXI line caused by turbulent plasma flows in the magnetic reconnection region during solar eruptions https://t.co/FoU1MKz60b

03 Feb 2023

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New Research: Non-thermal broadening of IRIS Fe XXI line caused by turbulent plasma flows in the magnetic reconnection region during solar eruptions https://t.co/g4zTy1Ubzf #SpaceSci

02 Feb 2023

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