Showing 1–20 of 44 results
/ Date/ Name
Jul 25, 2021Forward Modeling of Solar Coronal Magnetic Field Measurements Based on a Magnetic-field-induced Transition in Fe XMar 9, 2022Doppler shifts of spectral lines formed in the solar transition region and coronaNov 12, 2024Bidirectional propagating brightenings in arch filament systems observed by Solar Orbiter/EUIApr 22, 2021Transient small-scale brightenings in the quiet solar corona: a model for campfires observed with Solar OrbiterNov 17, 2024Investigating explosive events in a 3D quiet-Sun model: Transition region and coronal responseFeb 21, 2023Solar coronal magnetic field measurements using spectral lines available in Hinode/EIS observations: Strong and weak field techniques and temperature diagnosticsAug 18, 2021Measurements of the magnetic field strengths at the bases of stellar coronae using the magnetic-field-induced transition theoryDec 6, 2022Application of a magnetic-field-induced transition in Fe X to solar and stellar coronal magnetic field measurementsSep 15, 2025Magnetic reconnection sustains the mass budget of the solar windDec 25, 2025A self-consistent 3D MHD model producing a solar blowout jetAug 7, 2020Global maps of the magnetic field in the solar coronaFeb 26, 2022Three-dimensional Propagation of the Global EUV Wave associated with a solar eruption on 2021 October 28Apr 7, 2022Can we detect coronal mass ejections through asymmetries of Sun-as-a-star extreme-ultraviolet spectral line profiles?Feb 14, 2025Deep Tree Tensor Networks for Image RecognitionMar 12, 2025Unveiling the Dynamics and Genesis of Small-scale Fine Structure Loops in the Lower Solar AtmosphereAug 7, 2020Mapping the magnetic field in the solar corona through magnetoseismologyJun 3, 2020Generation of Solar Spicules and Subsequent Atmospheric HeatingNov 16, 2020A Magnetic Reconnection model for Hot Explosions in the Cool Atmosphere of the SunMar 5, 2019Flame-like Ellerman Bombs and Their Connection to Solar UV BurstsJul 5, 2022A new post-hoc flat field measurement method for the Solar X-ray and Extreme Ultraviolet Imager onboard the Fengyun-3E satellite