Latest CMEs detected by Cactus Hjälp

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 Hastighet Halo?
Median Variation Min. Max.
152025/12/15 00:003227°100°37691168512II
142025/12/14 08:123223°12°17525136202
132025/12/14 07:241233°52°35299212624
122025/12/14 06:361176°14°11374045781730
112025/12/13 11:122240°74°411121236694
102025/12/13 04:361292°30°28955228381
92025/12/13 02:480283°12°21274161381
82025/12/12 23:362194°22°10777371581953
72025/12/12 18:018179°48°4813011111201
62025/12/12 08:493173°36°255162103600
52025/12/12 07:008133°84°12952101266
42025/12/12 05:243243°72°38686177598
32025/12/11 13:251263°24°4882983291250
22025/12/11 02:002275°24°217104126449
12025/12/11 01:360103°20°23487229440

Data credit: SIDC - Cactus

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