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Non-thermal Broadening of IRIS Fe XXI Line Caused by Turbulent Plasma Flows in the Magnetic Reconnection Region During Solar Eruptions
DOI: 10.3389/fspas.2023.1096133 Bibcode: 2023FrASS..1096133S

Reeves, Katharine K.; Polito, Vanessa; Chen, Bin +3 more

Magnetic reconnection is the key mechanism for energy release in solar eruptions, where the high-temperature emission is the primary diagnostic for investigating the plasma properties during the reconnection process. Non-thermal broadening of high-temperature lines has been observed in both the reconnection current sheet (CS) and flare loop-top re…

2023 Frontiers in Astronomy and Space Sciences
Hinode IRIS 8
On orbit performance of the solar flare trigger for the Hinode EUV imaging spectrometer
DOI: 10.3389/fspas.2023.1149831 Bibcode: 2023FrASS..1049831B

Warren, Harry P.; Ugarte-Urra, Ignacio; Brooks, David H. +1 more

We assess the on-orbit performance of the flare event trigger for the Hinode EUV Imaging Spectrometer. Our goal is to understand the time-delay between the occurrence of a flare, as defined by a prompt rise in soft X-ray emission, and the initiation of the response observing study. Wide (266″) slit patrol images in the He II 256.32 Å spectral line…

2023 Frontiers in Astronomy and Space Sciences
Hinode 0