![]() Two bright ribbons clearly appeared underneath the erupting mini-filament as it quickly ascended, and subsequently, some dark materials blew out when the erupting mini-filament interacted with the outer ambient loops, thus forming a blowout jet characterized by a widening spire. Here, with a combination of 174 Å images of high spatio-temporal resolution taken by the Extreme Ultraviolet Imager on board Solar Orbiter and images of the Atmospheric Imaging Assembly on board Solar Dynamics Observatory, we investigate in detail an erupting mini-filament over a weak magnetic field region on 2022 March 4. ![]() However, their eruption mechanisms are still not understood thoroughly. Mini-filament eruptions are one of the most common small-scale transients in the solar atmosphere. Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119992 Moscow, Russia Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center, 7260 Davos Dorf, SwitzerlandĮTH-Zürich, Wolfgang-Pauli-Str. Université Paris-Saclay, CNRS, Institut d’Astrophysique Spatiale, 91405 Orsay, France UCL-Mullard Space Science Laboratory, Holmbury St. ![]() Solar-Terrestrial Centre of Excellence – SIDC, Royal Observatory of Belgium, Ringlaan 3 Av. Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany School of Astronomy and Space Science, Nanjing University, Nanjing 210046, PR ChinaĮ-mail: Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, PR China Astronomical objects: linking to databases.Including author names using non-Roman alphabets.Suggested resources for more tips on language editing in the sciences Punctuation and style concerns regarding equations, figures, tables, and footnotes
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