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 34 minutes ago (2024-04-25 20:15 UTC)
Last detected flare:
   0 hours and 34 minutes ago (2024-04-25 20:15 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 9516
Flare 9516


Details for flare #: 9516          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2023-01-15 14:51:0014.326-16.155.60.80, -0.230.8302675345
2023-01-15 14:54:00215.866-16.055.30.80, -0.230.8302675347
2023-01-15 14:57:00327.6111-15.855.40.80, -0.230.8302675348
2023-01-15 15:00:12437.7124-15.955.40.80, -0.230.8302675349
2023-01-15 15:03:00547.4145-15.955.40.80, -0.230.8302675353
2023-01-15 15:06:36647.5156-15.955.50.80, -0.230.8302675354
2023-01-15 15:09:00742.5154-15.955.60.80, -0.230.8302675357
2023-01-15 15:12:00834.6146-15.955.70.80, -0.230.8302675359
2023-01-15 15:15:00925.3126-15.955.80.80, -0.230.8402675361
2023-01-15 15:18:001016.794-16.055.90.80, -0.230.8402675363
2023-01-15 15:21:00119.456-16.056.10.80, -0.230.8402675364
2023-01-15 15:24:00125.437-15.956.40.81, -0.230.8402675366
2023-01-15 15:27:00133.124-15.956.60.81, -0.230.8402675369
2023-01-15 15:30:00142.419-15.956.60.81, -0.230.8402675371
2023-01-15 15:33:00153.724-15.956.70.81, -0.230.8402675373
2023-01-15 15:36:00163.322-15.956.80.81, -0.230.8402675375
2023-01-15 15:39:00172.016-15.956.90.81, -0.230.8502675376

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 )