In 2013 June, the two scientific instruments on board the second Sunrise mission witnessed,
in detail, a small-scale magnetic flux emergence event as part of the birth of an active region …

A small flare ribbon above a sunspot umbra in active region 12205 was observed on
November 7, 2014, at 12: 00 UT in the blue imaging channel of the 1.5 m GREGOR …

The short-lived active region (AR) NOAA 7968 was thoroughly observed all along its disk
transit (June 3 to 10, 1996) from space and from the ground. During the early stage of its …

The physical properties and their contribution to the onset of a solar flare are still uncleare
even though chromospheric brightening is considered a precursor phenomenon of a flare …

Using high spatial and temporal data from the Solar Dynamics Observatory (SDO) and the
Interface Region Imaging Spectrograph (IRIS), several observational signatures of magnetic …

We investigate the origin, configuration, and evolution of moving magnetic features (MMFs)
in the moat and penumbra regions of NOAA AR 10930 using Hinode/SOT filtergrams and …

Taking advantage of the high spatiotemporal resolution observations from the Atmospheric
Imaging Assembly (AIA) and the Helioseismic and Magnetic Imager on board the Solar …

Magnetic reconnection is thought to drive a wide variety of dynamic phenomena in the solar
atmosphere. Yet, the detailed physical mechanisms driving reconnection are difficult to …

The focus of this investigation is to quantify the conversion of magnetic to thermal energy
initiated by a quiet Sun cancellation event and to explore the resulting dynamics from the …

Abstract Continuum (" white-light," WL) emission dominates the energetics of flares. Filter-
based observations, such as the IRIS SJI 2832 filter, show WL-like brightenings during …