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 20 minutes ago (2024-06-18 15:33 UTC)
Last detected flare:
   1 hours and 44 minutes ago (2024-06-18 14:09 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 12255
Flare 12255


Details for flare #: 12255          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2023-05-24 18:48:00112.84417.15.80.10, 0.320.3402792547
2023-05-24 18:51:00212.14817.15.70.10, 0.320.3402792548
2023-05-24 18:54:00319.25917.25.60.09, 0.320.3402792555
2023-05-24 18:57:00427.26317.25.40.09, 0.330.3402792556
2023-05-24 19:00:00525.37217.25.50.09, 0.330.3402792557
2023-05-24 19:03:00613.16117.35.50.09, 0.330.3402792558
2023-05-24 19:06:00710.36618.93.20.05, 0.350.3602792559
2023-05-24 19:09:00826.217119.81.90.03, 0.370.3702792560
2023-05-24 19:12:00941.924719.72.20.04, 0.370.3702792561
2023-05-24 19:15:001043.726320.21.50.02, 0.370.3802792568
2023-05-24 19:18:001146.728220.61.00.02, 0.380.3802792569
2023-05-24 19:21:001246.428320.80.90.02, 0.380.3802792570
2023-05-24 19:24:001340.025920.71.20.02, 0.380.3802792571
2023-05-24 19:27:001432.822920.41.80.03, 0.380.3802792572
2023-05-24 19:30:001519.814820.71.80.03, 0.380.3802792573
2023-05-24 19:33:001612.810120.81.70.03, 0.390.3902792574
2023-05-24 19:36:00176.85621.01.60.03, 0.390.3902792575
2023-05-24 19:39:00184.73820.22.40.04, 0.370.3802792583

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 )