Aims. The expansion with height of the solar photospheric magnetic field and the plasma
flows is investigated for three isolated bright points (BPs). Methods. The BPs were observed …

The evolution of the physical parameters of magnetic bright points (MBPs) located in the
quiet Sun (mainly in the interwork) during their lifetime is studied. First, we concentrate on …

Context. The solar magnetic field is responsible for all aspects of solar activity. Thus,
emergence of magnetic flux at the surface is the first manifestation of the ensuing solar …

Context. Bright points (BPs) are small-scale, magnetic features ubiquitous across the solar
surface. Previously, we have observed and noted their properties for quiet Sun regions …

Context. Small-scale magnetic features are present everywhere in the solar photosphere.
Theoretical models, numerical calculations, and simulations describing the formation of …

Context. To deepen our understanding of the role of small-scale magnetic fields in active
regions (ARs) and in the quiet Sun (QS) on the solar irradiance, it is fundamental to …

Aims. We aim to improve our picture of the low chromosphere in the quiet-Sun internetwork
by investigating the intensity, horizontal velocity, size and lifetime variations of small bright …

Aims. In this paper we aim to investigate the evolution of plasma properties and Stokes
parameters in photospheric magnetic bright points using 3D magneto-hydrodynamical …

Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often
found with field strengths of the order of a kilogauss within intergranular lanes in the …

Aims. We study the breakout model using multiple flux emergence to produce the magnetic
configuration and the trigger. We do not impose any artificial motions on the boundaries …