As one of the most common features in the solar atmosphere, filaments are significant not
only in solar physics but also in stellar and laboratory plasma physics. With the New Vacuum …

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 …

Filaments are one of the most common features in the solar atmosphere and are of
significance in solar, stellar, and laboratory plasma physics. Using data from the Chinese Hα …

Failed filament eruptions are solar eruptions that are not associated with coronal mass
ejections. In a failed filament eruption, the filament materials usually show some ascending …

Solar filament eruptions are often associated with solar flares and coronal mass ejections,
which have the greatest impact on space weather. However, the fine structures and the …

Solar filaments can be formed via chromospheric evaporation followed by condensation in
the corona or by the direct injection of cool plasma from the chromosphere to the corona. We …

Although the magnetic field structures of solar filaments have been studied for several
decades, the detailed evolution of the structure around a filament prior to its eruption is …

We examine the buildup to and onset of an active region filament confined eruption of 2010
May 12, using EUV imaging data from the Solar Dynamics Observatory (SDO) Atmospheric …

Partial eruptions of solar filaments are the typical representatives of solar eruptive behavior
diversity. Here we investigate a typical filament partial eruption event and present integrated …

We follow the eruption of two related intermediate filaments observed in Hα (from GONG)
and EUV (from Solar Dynamics Observatory SDO/Atmospheric Imaging assembly AIA) and …