Sun-as-a-star analyses in which observational data is spatially integrated are useful for
interpreting stellar data. For future applications to stellar observations, we performed Sun-as …

This paper presents a multiwavelength Sun-as-a-star analysis of the M8. 7 flare on 2022
October 2, which was associated with a filament eruption and the subsequent coronal mass …

Stellar flares are characterized by sudden enhancement of electromagnetic radiation from
the atmospheres of stars. Compared to their solar counterparts, our knowledge on the …

Flares, sometimes accompanied by coronal mass ejections (CMEs), are the result of sudden
changes in the magnetic field of stars with high energy release through magnetic …

Context. Stellar coronal mass ejections (CMEs) are the primary driver of exoplanetary space
weather and may affect the habitability of exoplanets. However, detections of possible stellar …

Context. Coronal dimmings are localized regions of reduced emission in the extreme-
ultraviolet (EUV) and soft X-rays formed as a result of the expansion and mass loss by …

Solar filaments often exhibit rotation and deflection during eruptions, which would
significantly affect the geoeffectiveness of the corresponding coronal mass ejections …

The solar active region NOAA 12887 produced a strong X1. 0 flare on 2021 October 28,
which exhibits X-shaped flare ribbons and a circle-shaped erupting filament. To understand …

Solar filament eruptions, flares, and coronal mass ejections (CMEs) are manifestations of
drastic releases of energy in the magnetic field, which are related to many eruptive …

Stellar coronal mass ejections (CMEs) from host stars are an important factor that affects the
habitability of exoplanets. Although their solar counterparts have been well observed for …