Solar Demon Flare Detection (sc)

Science! running on SDO/AIA 94 Synoptic data
2 minute cadence, typical delay 7 days
(detection version 1.00)
(view all Solar Demon detection tools)

Detector 14 day operating status:

Last detected flare:
   214 hours and 35 minutes ago (2025-08-25 23:46 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 43051
Flare 43051


Details for flare #: 43051          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2025-08-06 07:42:0012.9261.00, 0.161.0108545808
2025-08-06 07:44:0027.1561.00, 0.161.0108545809
2025-08-06 07:46:00310.0711.00, 0.161.0108545810
2025-08-06 07:48:00412.4851.00, 0.161.0108545811
2025-08-06 07:50:00516.71030.99, 0.161.0108545812
2025-08-06 07:52:00624.01190.99, 0.151.0008545813
2025-08-06 07:54:00736.51500.99, 0.151.0108545814
2025-08-06 07:56:00856.31831.00, 0.151.0108545815
2025-08-06 07:58:00978.61991.00, 0.151.0108545816
2025-08-06 08:00:001094.72071.00, 0.151.0108545817
2025-08-06 08:02:0011102.82131.00, 0.151.0108545818
2025-08-06 08:04:0012102.22091.00, 0.151.0108545819
2025-08-06 08:06:001394.92041.00, 0.151.0108545820
2025-08-06 08:08:001482.71991.00, 0.151.0108545821
2025-08-06 08:10:001568.21841.00, 0.151.0108545822
2025-08-06 08:12:001655.31781.00, 0.151.0108545823
2025-08-06 08:14:001743.41631.00, 0.151.0108545824
2025-08-06 08:16:001833.91511.00, 0.151.0108545825
2025-08-06 08:18:001926.41381.00, 0.151.0108545826
2025-08-06 08:24:002010.2801.01, 0.151.0208545829
2025-08-06 08:26:00214.5361.01, 0.161.0208545830
2025-08-06 08:28:00222.3191.01, 0.161.0208545831

Solar Demon estimated flare class:
C3

Goes X-RAY flux timeline:

The research leading to these results has received funding from the European Commission's Seventh Framework Programme (FP7/2007-2013) under the grant agreement nr. 263506 [AFFECTS], and grant agreement nr. 263252 [COMESEP]
Solar Demon is still under construction.
( Legal notices - SWSC (Volume 5, A18, 2015) research article:Solar Demon - an approach to detecting flares, dimmings, and EUV waves on SDO/AIA images )