Coronal bright points (CBPs) are a fundamental class of solar activity. They represent a set
of low-corona small-scale loops with enhanced emission in the extreme-ultraviolet and X-ray …

We present new insights into the physical nature of coronal mass ejections (CMEs) and
associated shock waves within the framework of the three-dimensional (3D) structure. We …

Coronal bright points (CBPs) are small-scale, long-lived coronal brightenings that always
correspond to photospheric network magnetic features of opposite polarity. In this paper, we …

Aims. The main aim of the present analysis is to decipher (i) the small-scale bright features
in solar images of the quiet Sun and active regions obtained with the Atacama Large …

Context. The three-dimensional fine structure of the solar atmosphere is still not fully
understood as most of the available observations are taken from a single vantage point …

Context. The study explores the photospheric magnetic properties of bright and faint small-
scale loop systems in the solar atmosphere of the quiet Sun, also known as X-ray or coronal …

We have explored the moving structures in a coronal bright point (CBP) observed by the
Solar Dynamic Observatory Atmospheric Imaging Assembly (AIA) on 2011 March 5. This …

Context. We report on the first of a series of studies on coronal bright points which
investigate the physical mechanism that generates these phenomena. Aims. The aim of this …

Context. We investigate the chromospheric counterpart of small-scale coronal loops
constituting a coronal bright point (CBP) and its response to a photospheric magnetic-flux …

Context. Coronal bright points (CBPs) are small-scale and long-duration brightenings in the
lower solar corona. They are often explained in terms of magnetic reconnection. Aims. We …