Solar jets are observed as collimated plasma beams over a large range of temperatures and
wavelengths. They have been observed in H α and optical lines for more than 50 years and …

We present the first Mg ii slit-raster spectra from the Interface Region Imaging Spectrograph
(IRIS) that fully capture the genesis and coronal-jet-generating eruption of a central-disk …

We report our results from a set of high-resolution, two-fluid, non-linear simulations of the
magnetized Rayleigh Taylor instability (RTI) at the interface between a solar prominence …

Context. Solar jets are an important field of study, as they may contribute to the mass and
energy transfer from the lower to the upper atmosphere. Aims. We use the Interface Region …

Context. Density decreases exponentially with height in the gravitationally stratified solar
atmosphere, and therefore collisional coupling between the ionized plasma and the neutrals …

Abstract An Ellerman Bomb (EB) is a kind of small scale reconnection event, which is
ubiquitously formed in the upper photosphere or the lower chromosphere. The low …

Solar quiet-and coronal-hole region coronal jets frequently clearly originate from erupting
minifilaments, but active-region jets often lack an obvious erupting-minifilament source. We …

Context. Large-amplitude oscillations (LAOs) are often detected in filaments. Using multi-
wavelength observations, their origin can be traced back to the interaction with eruptions …

Using photospheric vector magnetograms obtained by the Helioseismic and Magnetic
Imager onboard the Solar Dynamics Observatory and a magnetic connectivity-based …

Similar to the cases of anemone jets, two-sided loop solar jets can also be produced by
either flux emergence from the solar interior or small-scale filament eruptions. Using high …