The purpose of this paper is to introduce the main scientific results made by the one-meter
New Vacuum Solar Telescope (NVST), which was put into commission on 2010. NVST is …

The low solar atmosphere is composed of mostly neutral particles, but the importance of the
magnetic field for understanding observed dynamics means that interactions between …

This paper reports the first possible evidence for the development of the Kelvin–Helmholtz
(KH) instability at the border of coronal holes separating the associated fast wind from the …

Aims. To understand the formation mechanism of large plumes in solar prominences, we
investigate the formation process of two such phenomena. Methods. We studied the …

Recent observations show cool, oscillating prominence threads fading when observed in
cool spectral lines and appearing in warm spectral lines. A proposed mechanism to explain …

The recently developed discrete Boltzmann method (DBM), which is based on a set of
uniform linear evolution equations and has high parallel efficiency, is employed to …

Context. Threads are the main constituents of prominences. They are dynamic structures
that display oscillations, usually interpreted as magnetohydrodynamic (MHD) waves …

Context. Solar filaments or prominences are common features in the Sun's atmosphere that
contain cool chromospheric material suspended within the hot corona. However, the …

Partially ionized plasmas (PIP) are essential constituents of many astrophysical
environments, including the solar atmosphere, the interstellar medium, molecular clouds …

Abstract The Kelvin–Helmholtz (KH) instability is commonly found in many astrophysical,
laboratory, and space plasmas. It could mix plasma components of different properties and …