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 39 minutes ago (2024-05-17 23:12 UTC)
Last detected flare:
   0 hours and 39 minutes ago (2024-05-17 23:12 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 19469
Flare 19469


Details for flare #: 19469          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2024-04-28 12:06:0015.437-7.230.60.51, -0.060.5103103824
2024-04-28 12:09:00212.592-6.931.00.52, -0.060.5203103825
2024-04-28 12:12:00316.1114-6.930.90.51, -0.060.5203103826
2024-04-28 12:15:00414.7104-6.730.90.51, -0.050.5203103827
2024-04-28 12:18:00516.2115-6.630.70.51, -0.050.5103103836
2024-04-28 12:21:00615.098-6.530.50.51, -0.050.5103103837
2024-04-28 12:24:00717.1105-6.530.20.50, -0.050.5103103838
2024-04-28 12:27:00821.1113-6.529.90.50, -0.050.5003103839
2024-04-28 12:30:00930.6137-6.529.90.50, -0.050.5003103840
2024-04-28 12:33:001045.6182-6.530.00.50, -0.050.5003103841
2024-04-28 12:36:001158.7203-6.530.00.50, -0.050.5003103848
2024-04-28 12:39:001268.5215-6.530.10.50, -0.050.5003103849
2024-04-28 12:42:001375.7229-6.530.10.50, -0.050.5103103850
2024-04-28 12:45:001479.0238-6.630.10.50, -0.050.5103103851
2024-04-28 12:48:001578.0241-6.630.10.50, -0.050.5103103852
2024-04-28 12:54:001667.4236-6.630.10.50, -0.050.5103103860
2024-04-28 12:57:001758.8223-6.630.20.50, -0.050.5103103861

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 )