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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.
222026/03/05 03:120283°28°2509237265
212026/03/04 21:12196°10°27129233317
202026/03/04 20:121289°8°730120530844
192026/03/04 11:121290°30°31533244359
182026/03/04 01:481123°36°31743237425
172026/03/04 00:361299°16°11423966811890
162026/03/03 12:001210°14°367112181568
152026/03/03 11:481337°8°516206157601
142026/03/03 11:362356°34°29580135466
132026/03/03 11:01292°82°727110453844
122026/03/03 06:48092°10°32446234367
112026/03/02 20:3624°6°7275214661737
102026/03/02 18:004216°6°197138184473
92026/03/02 15:485282°38°24692103440
82026/03/02 11:013277°36°43943355512
72026/03/02 09:1211357°68°25070153446
62026/03/02 01:36218°14°291116271578
52026/03/01 05:0024°10°337126252600
42026/03/01 02:12568°30°29385117440
32026/02/28 22:36198°10°20890134390
22026/02/28 20:2424°22°584165162744
12026/02/28 18:000308°18°29211269309

Data credit: SIDC - Cactus

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