Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic
eruptive phenomena in our solar system and able to release a large quantity of plasma and …

Solar eruptions, observed as flares and coronal mass ejections (CMEs), are the most
energetic visible plasma phenomena in the solar system. CMEs are the central component …

With observations from the Interface Region Imaging Spectrograph, we track the complete
evolution of∼ 11 MK evaporation flows in an M1. 1 flare on 2014 September 6 and an X1. 6 …

We investigate observational signatures of explosive chromospheric evaporation during a
white-light flare (WLF) that occurred on 2022 August 27. Using the moment analysis …

As one of the payloads for the Advanced Space-based Solar Observatory (ASO-S) mission,
the Lyman-alpha (Lyα) Solar Telescope (LST) is aimed at imaging the Sun and the inner …

Abstract The Interface Region Imaging Spectrograph (IRIS) has been obtaining near-and far-
ultraviolet images and spectra of the solar atmosphere since July 2013. IRIS is the highest …

We report a failed solar filament eruption that involves external magnetic reconnection in a
quadrupolar magnetic configuration. The evolution exhibits three phases of kinematic …

ABSTRACT A model for strongly writhing confined solar eruptions suggests an origin in the
helical kink instability of a coronal flux rope that remains stable against the torus instability …

Using observations by the Solar Dynamics Observatory from 2010 June to 2017 December,
we have performed the first statistical investigation of circular-ribbon flares (CFs) and …

Context. A filament channel (FC), a plasma volume where the magnetic field is primarily
aligned with the polarity inversion line, is believed to be the pre-eruptive configuration of …