OBSERVATIONS OF VECTOR MAGNETIC-FIELDS IN FLARING ACTIVE REGIONS

We present vector magnetograph data of 6 active regions, all of which produced major flares. Of the 20 M-class (or above) flares, 7 satisfy the flare conditions prescribed by Hagyard (high shear and strong tran sverse fields), Strong photospheric shear, however, is not necessarily a condition for a flare. We find an increase in the shear for two fla res, a 6-deg shear increase along the neutral Line after a X-2 flare a nd a 13-deg increase after a M-1.9 flare. For other flares, we did not detect substantial shear changes.