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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.
222025/12/15 00:003227°100°376130113710II
212025/12/14 08:122222°10°15424132201
202025/12/14 07:361234°54°34389214578
192025/12/14 07:001176°14°11374045781730
182025/12/13 11:122239°76°411119236694
172025/12/13 04:361292°30°28955228381
162025/12/13 02:480283°12°21274161381
152025/12/12 18:018179°48°4813091111201
142025/12/12 08:492173°36°255160103589
132025/12/12 07:008133°84°12948101244
122025/12/12 05:243242°74°40191177598
112025/12/11 13:251263°24°4882943321250
102025/12/11 02:002276°26°246111126473
92025/12/11 01:361103°20°23487229440
82025/12/10 22:363246°102°30054175446II
72025/12/10 22:241240°14°4425312021420
62025/12/10 14:481228°22°20631181267
52025/12/10 14:002242°70°20845152325
42025/12/10 10:362155°8°2425232244
32025/12/10 04:12237°8°47726434504
22025/12/10 03:480237°12°17940125233
12025/12/10 00:482166°18°7692174401179

Data credit: SIDC - Cactus

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