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 19 minutes ago (2026-02-08 17:09 UTC)
Last detected flare:
   0 hours and 19 minutes ago (2026-02-08 17:09 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 33550
Flare 33550


Details for flare #: 33550          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2026-02-07 08:15:00111.741-18.236.30.57, -0.230.6103666585
2026-02-07 08:18:00242.986-18.136.50.57, -0.230.6103666586
2026-02-07 08:21:00382.8118-18.236.70.57, -0.230.6203666587
2026-02-07 08:24:00484.8125-18.236.90.58, -0.230.6203666592
2026-02-07 08:27:00565.8127-18.336.90.58, -0.230.6203666593
2026-02-07 08:30:00655.2128-18.337.10.58, -0.230.6203666596
2026-02-07 08:33:00744.0124-18.437.10.58, -0.230.6203666597
2026-02-07 08:36:00832.4116-18.537.20.58, -0.230.6203666600
2026-02-07 08:39:00923.699-18.837.10.58, -0.240.6203666601
2026-02-07 08:42:001019.085-18.837.30.58, -0.240.6303666604
2026-02-07 08:45:241118.478-18.637.70.59, -0.230.6303666605
2026-02-07 08:48:001218.278-18.637.80.59, -0.240.6303666606
2026-02-07 08:51:001314.467-18.637.90.59, -0.240.6303666607
2026-02-07 08:54:001410.154-18.737.90.59, -0.240.6303666612
2026-02-07 08:57:36156.139-18.738.00.59, -0.240.6303666613
2026-02-07 09:00:00164.128-18.738.00.59, -0.240.6303666616
2026-02-07 09:03:36172.419-18.738.00.59, -0.240.6403666617

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 )