In this review we focus on the fundamental theory of magnetohydrodynamic reconnection,
together with applications to understanding a wide range of dynamic processes in the solar …

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 …

Context. Solar coronal mass ejections (CMEs) can catch up and interact with preceding
CMEs and solar wind structures to undergo rotation and deflection during their propagation …

We study the physical mechanism of a major X-class solar flare that occurred in the super
NOAA active region (AR) 12192 using data-driven numerical magnetohydrodynamic (MHD) …

Solar flares are powerful radiations occurring in the Sun's atmosphere. They are powered by
magnetic reconnection, a phenomenon that can convert magnetic energy into other forms of …

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

Quasi-periodic pulsations (QPPs), which carry time features and plasma characteristics of
flare emissions, are frequently observed in light curves of solar/stellar flares. In this study, we …

Coronal mass ejections (CMEs) are large-scale explosions of the coronal magnetic field. It is
believed that magnetic reconnection significantly builds up the core structure of CMEs, a …

The observation of the high-temperature (≳ 10 MK) Fe xxi 1354.1 Å line with the Interface
Region Imaging Spectrograph has provided significant insights into the chromospheric …

Context. Bridging the gap between heliospheric and solar observations of eruptions requires
the mapping of interplanetary coronal mass ejection (CME) footpoints down to the Sun's …