Empirical Scaling Relations for the Photospheric Magnetic Elements of the Flaring and Non-Flaring Active Regions

@inproceedings{MAMoradhaseli2021EmpiricalSR,
  title={Empirical Scaling Relations for the Photospheric Magnetic Elements of the Flaring and Non-Flaring Active Regions},
  author={M.A.Moradhaseli and M.Javaherian and N.Fathalian and H.Safari},
  year={2021}
}
Here, we analyzed magnetic elements of the solar active regions (ARs) observed in the line-of-sight magnetograms (the 6173 Å Fe I line) recorded with the Solar Dynamics Observatory (SDO)/Helioseismic and Magnetic Imager (HMI). The Yet Another Feature Tracking Algorithm (YAFTA) was employed to extract the statistical properties of these features (e.g. filling factor, magnetic flux, and lifetime) within the areas of 180′′ × 180′′ inside the flaring AR (NOAA 12443) and the non-flaring AR (NOAA… Expand

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