Abstract
The evolution of vector photospheric magnetic fields has been studied in concert with photospheric spot motions for a flare-productive active region. Over a three-day period (5–7 April, 1980), sheared photospheric velocity fields inferred from spot motions are compared both with changes in the orientation of transverse magnetic fields and with the flare history of the region. Rapid spot motions and high inferred velocity shear coincide with increased field alignment along the B L= 0 line and with increased flare activity; a later decrease in velocity shear precedes a more relaxed magnetic configuration and decrease in flare activity. Crude energy estimates show that magnetic reconfiguration produced by the relative velocities of the spots could cause storage of ∼ 1032 erg day−1, while the flares occurring during this time expended ≲1031 erg day−1.
Maps of vertical current density suggest that parallel (as contrasted with antiparallel) currents flow along the stressed magnetic loops. For the active region, a constant-α, force-free magnetic field (J = αB) at the photosphere is ruled out by the observations.
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Presently located at NASA/MSFC, Huntsville, Ala. 35812, U.S.A.
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Krall, K.R., Smith, J.B., Hagyard, M.J. et al. Vector magnetic field evolution, energy storage, and associated photospheric velocity shear within a flare-productive active region. Sol Phys 79, 59–75 (1982). https://doi.org/10.1007/BF00146973
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DOI: https://doi.org/10.1007/BF00146973