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.
182026/06/22 06:48383°48°5632871301201
172026/06/22 04:48062°10°38820355411
162026/06/22 04:12250°30°21881101351
152026/06/22 03:361225°20°216113187473
142026/06/22 03:12146°26°20048116297
132026/06/22 02:481201°32°21186183390
122026/06/21 23:12541°28°21166107355
112026/06/21 20:00192°94°21954112376II
102026/06/21 18:004247°12°16416145194
92026/06/21 13:481214°38°5832252881058
82026/06/21 08:121214°26°31224260336
72026/06/21 03:121115°44°24323201290
62026/06/20 07:480273°976968681115
52026/06/20 03:12232°70°55381372743
42026/06/20 02:12191°76°25430174297
32026/06/18 23:481280°14°61273480727
22026/06/18 06:481229°5785465121561
12026/06/18 06:241280°42°8681734951116

Data credit: SIDC - Cactus

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