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The magnetic properties of photospheric magnetic bright points with high resolution spectropolarimetry

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 نشر من قبل Peter Keys
 تاريخ النشر 2019
  مجال البحث فيزياء
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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, we look at general trends in the properties of magnetic bright points. In total we track 300 MBPs in the data set and we employ NICOLE



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