Relationship between magnetic field evolution and major flare event on July 14, 2000
Relationship between magnetic field evolution and major flare event on July 14, 2000
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DOI:
10.1051/0004-6361:20010550
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发表时间:
2001-06
影响因子:
6.5
通讯作者:
Yu Liu;Hongqi Zhang
中科院分区:
文献类型:
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作者:
Yu Liu;Hongqi Zhang
. On July 14, 2000 the active region NOAA 9077 produced one of the largest solar flares (3B/X5.7) seen in recent years associated with a violent halo coronal mass ejection (CME). It had a (cid:12)γ(cid:14) magnetic classi(cid:12)cation and the morphology of the sunspot group and magnetic (cid:12)eld changed obviously every day. We present here the relationship between the large scale motions of the spots and the major flare on July 14, based on precise measurements of the proper motions. We (cid:12)nd that: (1) The special magnetic morphology and quick, successive fragmentation caused the active region to be always in a high shear con(cid:12)guration; (2) There is a good spatial correspondence between the direction of the movement of one spotgroup and the place where the (cid:12)lament was cut o(cid:11) and activated; (3) The motion characteristics of the rapidly emerging flux system showed a good correlation between spot motions and the largest flares, suggesting that the initiation of the two-ribbon flare on July 14 was promoted by the successive emergence of the flux systems. The intensive major flare was always connected strongly with a newly emerging magnetic flux system (K(cid:19)alm(cid:19)an 1997). This con(cid:12)rms that (cid:14) -con(cid:12)gurations and dynamical processes are important in large flares.