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Table 1:

Data on the halo CMEs and analyzed relevant eruptive events.
Day CME timea Linear speed Acceleration Gradual (g) Associated eventb Active region
  (UT) (km s-1) (m s-2) or impulsive (i) (Beg, Max, End)UT NOAA number
2000-02-10 02:30:05 944 11.4 g C7.3 (01:40, 02:08, 02:39) 8858
2000-04-10 00:30:05 409 2.5 g M3.1 (23:26, 23:42, 23:55) 8948
2000-08-09 16:30:05 720 2.8 g C2.3-ERU (15:19, 16:22, 17:00) 9114
2001-03-29 10:26:05 942 3.5 g X1.7 (09:57, 10:15, 10:32) 9393
2001-04-10 05:30:00 2411 211.6 g X2.3 (05:06, 05:26, 05:42) 9415
2002-07-15 20:30:05 1151 -25.6 i X3.0 (19:59, 20:08, 20:14) 10030
2002-07-16 16:02:58 1636 -41.0 i ERU (15:36, 15:39, 15:49) 10030
2002-08-16 12:30:05 1585 -67.1 i M5.2-ERU (11:32, 12:32, 13:07) 10069
2002-10-25 15:06:05 870 -23.4 i ERU (14:09, 14:11, 14:18) 10162
2002-12-19 22:06:05 1092 -36.2 i M2.7 (21:34, 21:53, 22:17) 10229
2003-05-27 06:50:05 509 -14.6 i M1.6 (05:06, 06:26, 07:16) 10365
2003-05-27 23:50:05 964 -9.6 i X1.3 (22:56, 23:07, 23:13) 10365

Notes. The data on the halo CMEs and on the eruptive events were deduced from the SOHO/LASCO Catalog and the Active Region Monitor websites, respectively. (a) The CME time indicates the time of first appearance in LASCO/C2. (b) ERU indicates the occurrence of an erupting filament.


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