Solar Demon Flare Detection (qlk)

Quick-look! running in real time on SDO/AIA 94 QKL data
3 minute cadence, typical delay 15 minutes
(detection version 1.00)
(view all Solar Demon detection tools)

Detector 24h operating status:

Last processed image:    
   0 hours and 23 minutes ago (2026-05-03 11:48 UTC)
Last detected flare:
   4 hours and 47 minutes ago (2026-05-03 07:24 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 34500
Flare 34500


Details for flare #: 34500          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2026-04-28 18:21:0013.3239.2-20.8-0.35, 0.230.4203746296
2026-04-28 18:24:36221.61039.0-20.1-0.34, 0.230.4103746297
2026-04-28 18:27:00315.11008.9-20.4-0.35, 0.230.4203746300
2026-04-28 18:30:00429.51728.7-21.2-0.36, 0.220.4203746303
2026-04-28 18:33:00534.51868.4-22.0-0.37, 0.220.4303746304
2026-04-28 18:36:00640.32208.2-22.5-0.38, 0.220.4403746305
2026-04-28 18:39:00739.62418.2-22.8-0.39, 0.220.4403746308
2026-04-28 18:42:00834.82438.3-23.1-0.39, 0.220.4503746309
2026-04-28 18:45:00933.22428.3-23.4-0.40, 0.220.4503746312
2026-04-28 18:48:121056.53307.6-24.1-0.41, 0.200.4603746313
2026-04-28 18:51:001170.63907.5-24.2-0.41, 0.200.4603746316
2026-04-28 18:54:001270.54527.7-24.8-0.42, 0.210.4703746317
2026-04-28 18:57:001364.54398.0-25.4-0.43, 0.210.4803746320
2026-04-28 19:00:001449.43558.2-25.6-0.43, 0.210.4803746321
2026-04-28 19:03:001532.22498.4-25.7-0.43, 0.220.4803746324
2026-04-28 19:06:001618.21548.5-25.5-0.43, 0.220.4803746325
2026-04-28 19:09:00176.5588.8-25.1-0.42, 0.220.4803746328

Solar Demon estimated flare class:
C2

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 )