The magnetic properties of photospheric magnetic bright points with high-resolution spectropolarimetry
The magnetic properties of photospheric magnetic bright points with high-resolution spectropolarimetry
Magnetic bright points are small-scale magnetic elements ubiquitous across the solar disk, with the prevailing theory suggesting that they form due to the process of convective collapse. Employing a unique full Stokes spectropolarimetric data set of a quiet Sun region close to disk centre obtained with the Swedish Solar Telescope, …