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Latest CMEs detected by Cactus Help

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 Velocity Halo?
Median Variation Min. Max.
192026/03/14 02:364300°10°38555295426
182026/03/13 21:001124°14°284178197694
172026/03/13 12:480127°16°28940202336
162026/03/13 11:121290°10°29835234336
152026/03/13 05:48119°20°318156242625
142026/03/13 05:483342°110°30690117512II
132026/03/13 03:241194°10°7596094611783
122026/03/13 00:482242°14°33564226413
112026/03/13 00:481181°20°32226300365
102026/03/13 00:482166°18°26436234347
92026/03/13 00:360166°6°28845256363
82026/03/13 00:242220°62°28663169385
72026/03/12 16:362105°8°17228135214
62026/03/12 14:24297°24°477133335761
52026/03/10 21:121310°6°8915113361646
42026/03/10 15:121224°6°25641192294
32026/03/10 09:242321°36°4402891231116
22026/03/10 01:481105°12°505122297679
12026/03/09 11:24171°36°250178200782

Data credit: SIDC - Cactus

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