Magnetic topological analysis of coronal bright points
K. Galsgaard, M. S. Madjarska, F. Moreno-Insertis, Z. Huang, T., Wiegelmann

TL;DR
This study investigates the magnetic field structures associated with coronal bright points, revealing that most are located near magnetic null points within fan-dome configurations, enhancing understanding of their magnetic environment.
Contribution
The paper introduces a detailed magnetic field analysis of coronal bright points using potential and magneto-static extrapolation methods, highlighting the role of magnetic null points in their formation.
Findings
Most bright points are located near magnetic null points.
Bright points are often within fan-dome magnetic structures.
One bright point is in a bipolar loop system without a null point.
Abstract
{We report on the first of a series of studies on coronal bright points investigating the physical mechanism that generates these phenomena.} {The aim of this paper is to understand the magnetic-field structure that hosts the bright points.} {We use longitudinal magnetograms taken by the Solar Optical Telescope with the Narrowband Filter Imager. For a single case, magnetograms from the Helioseismic and Magnetic Imager were added to the analysis. The longitudinal magnetic field component is used to derive the potential magnetic fields of the large regions around the bright points. A magneto-static field extrapolation method is tested to verify the accuracy of the potential field modelling. The three dimensional magnetic fields are investigated for the presence of magnetic null points and their influence on the local magnetic domain.} {In 9 out of 10 cases the bright point resides in…
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