ABSTRACT G-band bright points (GBPs) are thought to be the foot-points of magnetic flux
tubes. The aim of this paper is to investigate the relation between the diffusion regimes of …

G-band bright points (GBPs) are regarded as good manifestations of magnetic flux
concentrations. We aim to investigate the relation between the dynamic properties of GBPs …

Aims. Magnetic elements are thought to be described by flux tube models, and are well
reproduced by MHD simulations. However, these simulations are only partially constrained …

Photospheric bright points (PBPs) and chromospheric bright points (CBPs) reflect the cross
sections of magnetic flux tubes at different heights of the lower solar atmosphere. We aim to …

The 7 nonthermal filamentary structures located in the Galactic center region (l<| 1deg|) are
believed to manifest strong (few mG) vertical magnetic field lines coherent over the tens of …

New low-frequency 74 and 330 MHz observations of the Galactic center (GC) region reveal
the presence of a large-scale (6× 2) diffuse source of nonthermal synchrotron emission. A …

Cotemporal observations in the 4305 Å G-band and Ca II λ 3933 K-line, Fe I 6302 Å
magnetograms, and 6563 Å H α images are used to study the relation of G-band bright …

The unsigned magnetic flux content in the flux concentrations of two active regions is
calculated by using a set of 248 high-resolution Solar and Heliospheric Observatory …

Context. Small-scale magnetic fields in the solar photosphere can be identified in high-
resolution magnetograms or in the G-band as magnetic bright points (MBPs). Rapid motions …

Context. G-band bright points are small-sized features characterized by high photometric
contrast. Theoretical investigations indicate that these features have associated magnetic …