TRANSIENTS ASSOCIATED WITH RECURRENT STORMS

From August 1993, to April 1994, in the declining phase of solar cycle 22, a broken series of eight storms recurred with successive passages of the same sector boundary in the course of 10 Solar rotations. Thre e of the strongest of these storms, on November 3-4, 1993, February 21 , 1994, and April 17, 1994, are the subjects of recent community studi es. All three have been associated with X ray events in Yohkoh data si gnaling the launch of coronal mass ejections (CMEs). Because of the cl ear morphology of these events, the associations are more obvious than past associations with flares. We find additional X ray events that c an be associated with the remaining five storms in the sequence. The a ssociations range from nearly certain for three of the four strongest storms to doubtful for the weakest storm. No X ray events occurred on the two rotations with no storms. Of the eight storms in total, four w ere associated with large arcades near the south polar crown, three wi th smaller-scale events in active regions bordering the northern coron al hole extension, and one with a medium arcade equatorward of the nor th polar crown. These sites apparently map out to the same sector boun dary at 1 AU. Although recurrent storms are usually associated with hi gh-speed streams from coronal holes, we infer that the southward inter planetary magnetic field responsible for peak activity is often brough t by CMEs from the base of the sector boundary between coronal holes. Coupled with corotating interaction regions (CIRs) created by any onco ming high-speed flow from the following coronal hole, the transient CM Es fall into the recurrence pattern and can account for the unpredicta bly wide range of recurrent storm strengths.