We review stereoscopic and tomographic methods used in the solar corona, including
ground-based and space-based measurements, using solar rotation or multiple spacecraft …

In the early 1990s, it was found that the strongest disturbances of the space–weather were
associated with huge ejections of plasma from the solar corona, which took the form of …

In this paper, we report our multiwavelength observations of a partial filament eruption event
in NOAA active region (AR) 11283 on 8 September 2011. A magnetic null point and the …

Context. Generation and dissipation of magnetic fields is a fundamental physical process on
the Sun. In comparison to flux emergence and the initial stages of sunspot formation, the …

In this paper, we present multiwavelength observations of helical kink instability as a trigger
of a coronal mass ejection (CME) which occurred in active region NOAA 11163 on 2011 …

We present a multiwavelength study of the X-class flare, which occurred in active region
(AR) NOAA 11339 on 3 November 2011. The extreme ultraviolet (EUV) images recorded by …

We present observations of a confined partial eruption of a filament on 2012 August 4, which
restores its initial shape within≈ 2 hr after eruption. From the Global Oscillation Network …

We present a multiwavelength study of the formation and ejection of a plasma blob and
associated extreme ultraviolet (EUV) waves in active region (AR) NOAA 11176, observed by …

We analyze multi-wavelength data of an M7. 9/1N class solar flare which occurred on 2006
April 27 in AR NOAA 10875. GOES soft X-ray images provide the most likely signature of two …

Multiwavelength observations of a prominence eruption provide an opportunity to uncover
the physical mechanism of the triggering and the evolution process of the eruption. In this …