D field configuration presented here, together with the recent sheared-core bipolar magnetic field model of Antiochos, Dahlburg, and Klimchuk (1994) and recent Yohkoh SXT observations of the coronal magnetic field configuration at and before the onset of large eruptive bipolar flares, supports the seminal 3-
(D field configuration; presented; L:here) (D field configuration presented here; supports; the seminal 3) (Dahlburg; [is] the recent sheared - core bipolar magnetic field model of; Antiochos)
D field configuration D field configuration presented here Dahlburg
presented supports [is] the recent sheared - core bipolar magnetic field model of
L:here
the seminal 3
Antiochos