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 57 minutes ago (2023-09-30 18:03 UTC)
Last detected flare:
   1 hours and 9 minutes ago (2023-09-30 17:51 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 14620
Flare 14620


Details for flare #: 14620          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2023-09-06 10:42:0014.62515.9-45.6-0.69, 0.190.7202886774
2023-09-06 10:45:00212.45515.8-45.3-0.69, 0.190.7102886775
2023-09-06 10:48:00320.08415.8-45.3-0.69, 0.190.7102886776
2023-09-06 10:51:00427.112015.9-45.2-0.69, 0.190.7102886777
2023-09-06 10:54:00529.712615.9-45.2-0.69, 0.190.7102886786
2023-09-06 10:57:00630.413415.9-45.1-0.69, 0.190.7102886787
2023-09-06 11:00:00727.613515.9-45.2-0.69, 0.190.7102886788
2023-09-06 11:03:00824.713315.9-45.2-0.69, 0.190.7102886789
2023-09-06 11:06:00922.712315.9-45.3-0.69, 0.190.7102886790
2023-09-06 11:09:001023.912815.9-45.3-0.69, 0.190.7202886791
2023-09-06 11:12:001122.312515.8-45.3-0.69, 0.190.7202886792
2023-09-06 11:15:001219.211315.8-45.4-0.69, 0.190.7202886793
2023-09-06 11:18:001314.89415.8-45.4-0.69, 0.190.7202886800
2023-09-06 11:21:00149.25915.8-45.6-0.69, 0.190.7202886801
2023-09-06 11:24:00156.54615.7-45.6-0.69, 0.190.7202886802
2023-09-06 11:27:00163.52615.6-45.9-0.70, 0.180.7202886803
2023-09-06 11:30:00172.21815.6-45.9-0.70, 0.180.7202886804

Solar Demon estimated flare class:
C1

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 )