Abstract
In this paper we present a quantitative evaluation of the shear in the magnetic field along the neutral line in an active region during an epoch of flare activity. We define shear as the angular difference in the photosphere between the potential magnetic field, which fits the boundary conditions imposed by the observed line-of-sight field, and the observed magnetic field. For the active region studied, this angular difference (shear) is non-uniform along the neutral line with maxima occurring at the locations of repeated flare onsets. We suggest that continued magnetic evolution causes the field's maximum shear to exceed a critical value of shear, resulting in a flare around the site of maximum shear. Evidently, the field at the site of the flare must relax to a state of shear somewhat below the critical value (but still far from potential), with subsequent evolution returning the field to the critical threshold. We draw this inference because several flares occurred at sites of maximum photospheric shear which were persistent in location.
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NOAA, Boulder, Colorado.
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Hagyard, M.J., Smith, J.B., Teuber, D. et al. A quantitative study relating observed shear in photospheric magnetic fields to repeated flaring. Sol Phys 91, 115–126 (1984). https://doi.org/10.1007/BF00213618
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DOI: https://doi.org/10.1007/BF00213618