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 38 minutes ago (2024-08-31 22:15 UTC)
Last detected flare:
   0 hours and 38 minutes ago (2024-08-31 22:15 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 21996
Flare 21996


Details for flare #: 21996          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2024-07-22 18:18:0013.8230.98, 0.251.0103183343
2024-07-22 18:21:0025.5340.98, 0.251.0103183344
2024-07-22 18:24:0035.0330.98, 0.251.0103183345
2024-07-22 18:27:0044.3290.98, 0.241.0103183346
2024-07-22 18:30:0054.3300.98, 0.241.0103183347
2024-07-22 18:33:0064.2320.98, 0.241.0103183348
2024-07-22 18:36:0076.0460.98, 0.261.0103183355
2024-07-22 18:39:0087.4540.97, 0.271.0103183356
2024-07-22 18:42:0097.9580.97, 0.271.0103183357
2024-07-22 18:45:001011.2710.97, 0.281.0103183358
2024-07-22 18:48:001112.2660.97, 0.291.0103183359
2024-07-22 18:51:001212.4710.97, 0.291.0103183360
2024-07-22 18:54:001310.1650.97, 0.291.0103183361
2024-07-22 18:57:12147.7580.97, 0.281.0103183362
2024-07-22 19:00:00156.1490.98, 0.271.0103183371
2024-07-22 19:03:00165.0400.98, 0.251.0203183372
2024-07-22 19:06:00175.1390.99, 0.241.0203183373
2024-07-22 19:09:00185.3400.99, 0.241.0203183374
2024-07-22 19:12:00194.7360.99, 0.241.0203183375
2024-07-22 19:15:00203.0240.99, 0.241.0203183382
2024-07-22 19:18:00212.2190.99, 0.241.0203183383

Solar Demon estimated flare class:
B4

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 )