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.
202025/12/23 20:003252°34°328109214558
192025/12/23 15:123252°50°32684214529
182025/12/23 03:40125°16211155183
172025/12/23 00:22327°40°21496114371
162025/12/22 11:363106°42°370106110502
152025/12/22 05:00585°88°2827399417
142025/12/22 05:00582°106°15738100243II
132025/12/22 00:125135°12°102399108
122025/12/22 00:00268°15653105227
112025/12/21 21:36173°12°23635223315
102025/12/21 16:241150°7104774401562
92025/12/21 15:12161°12012028921420
82025/12/20 21:48269°24°1041829191201
72025/12/20 21:481220°14°702121459781
62025/12/20 16:48173°148826813581953
52025/12/20 12:36155°20°7374446001749
42025/12/20 08:24179°60°278107145578
32025/12/20 06:48717°36°19236126265
22025/12/19 14:242308°14°1955119531956
12025/12/19 00:481255°16°639168488951

Data credit: SIDC - Cactus

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