By using a new method of forced-field extrapolation, we study the emerging flux region
AR11850 observed by the Interface Region Imaging Spectrograph and Solar Dynamical …

We present spectroscopic and imaging observations of small-scale reconnection events on
the Sun. Using Interface Region Imaging Spectrograph (IRIS) observations, one …

Context. Interface Region Imaging Spectrograph (IRIS) bursts are localised features thought
to be driven by magnetic reconnection. Although these events are well-studied, it remains …

Multiwavelength ultraviolet (UV) observations by the Interface Region Imaging Spectrograph
satellite in active region NOAA 12529 have recently pointed out the presence of long-lasting …

Our understanding of the process of fast reconnection has undergone a dramatic change in
the last 10 years driven, in part, by the availability of high-resolution numerical simulations …

We report multiwavelength ultraviolet observations taken with the IRIS satellite, concerning
the emergence phase in the upper chromosphere and transition region of an emerging flux …

Magnetic reconnection is the key mechanism for energy release in solar eruptions, where
the high-temperature emission is the primary diagnostic for investigating the plasma …

We investigate various dynamic processes including magnetic reconnection, chromospheric
evaporation, and coronal rain draining in two limb solar flares through imaging and …

The significance increase of the plasma temperature from the solar photosphere to the
corona up to 1MK is still unresolved. One of the candidates for this issue is waves and …

Recent observations by the Interface Region Imaging Spectrograph (IRIS) have revealed
pockets of hot gas (∼ 2–8× 10 4 K) potentially resulting from magnetic reconnection in the …