Frequent EUV microflashes at solar plume bases, each releasing ~10^24 erg, are identified as a new unipolar network event and suggested as a candidate mechanism to power the open corona and solar wind.
P., Peter, H., Solanki, S
3 Pith papers cite this work. Polarity classification is still indexing.
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CNN separation of He I 10830Å chromospheric signal from photospheric contamination in quiet Sun reveals R ≈ -0.84 anti-correlation with 304Å and magnetic-field-dependent EUV coupling.
Overview paper introducing the Sunrise III balloon-borne solar observatory, its 2024 flight, data volume, and the focus issue containing first scientific results.
citing papers explorer
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Extreme Ultraviolet Microflashes at Plume Bases: A Candidate for Powering the Corona and Solar Wind?
Frequent EUV microflashes at solar plume bases, each releasing ~10^24 erg, are identified as a new unipolar network event and suggested as a candidate mechanism to power the open corona and solar wind.
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Machine Learning-based Separation of the He I 10830{\AA} Chromospheric Signal: Quantitative Analysis of Chromosphere-Corona Intensity in the Quiet Sun
CNN separation of He I 10830Å chromospheric signal from photospheric contamination in quiet Sun reveals R ≈ -0.84 anti-correlation with 304Å and magnetic-field-dependent EUV coupling.
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Sunrise III: Instrument, mission, data, and first results
Overview paper introducing the Sunrise III balloon-borne solar observatory, its 2024 flight, data volume, and the focus issue containing first scientific results.