Latest CMEs detected by Cactus Ayuda

Coronal Mass Ejections can occur during solar flares unleashing a giant cloud of solar wind particles into space. Here you'll find an overview of the latest CMEs that where detected by the Cactus software of the SIDC. The Cactus software autonomously detects CMEs in image sequences from the LASCO instrument on board SOHO, the result is a list of detections by the software with the characteristics of the CME.

CME Onset time Duration Angle Angular width Velocidad Halo?
Median Variation Mín. Máx.
142026/06/22 16:02261°2114207217
132026/06/22 06:48383°48°5632861301201
122026/06/22 04:12350°30°22482101351
112026/06/22 02:481201°32°21186183390
102026/06/21 23:12441°28°21069101355
92026/06/21 20:00192°94°21348113336II
82026/06/21 13:481214°38°5832252881058
72026/06/21 08:121214°26°31224260336
62026/06/20 07:480273°976968681115
52026/06/20 03:12232°70°55381372743
42026/06/20 02:12191°76°24529175297
32026/06/18 23:481280°14°61273480727
22026/06/18 06:481229°5785465121561
12026/06/18 06:241280°42°8681724951116

Data credit: SIDC - Cactus

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