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:    
   390 hours and 55 minutes ago (2024-11-26 23:45 UTC)
Last detected flare:
   391 hours and 58 minutes ago (2024-11-26 22:42 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 26335
Flare 26335


Details for flare #: 26335          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2024-11-19 22:33:1216.450-11.475.80.96, -0.210.9803295078
2024-11-19 22:36:00216.8113-11.374.40.95, -0.210.9703295082
2024-11-19 22:39:00327.3159-11.474.90.95, -0.210.9803295083
2024-11-19 22:42:00432.8171-11.575.30.95, -0.210.9803295085
2024-11-19 22:45:12535.8175-11.676.00.96, -0.210.9803295086
2024-11-19 22:48:00636.2176-11.676.50.96, -0.210.9803295090
2024-11-19 22:51:00735.8180-11.777.00.96, -0.210.9803295092
2024-11-19 22:54:00831.5163-11.777.50.96, -0.210.9903295093
2024-11-19 22:57:00926.5142-11.678.10.96, -0.210.9903295094
2024-11-19 23:00:001022.6128-11.678.50.97, -0.210.9903295097
2024-11-19 23:03:001121.1126-11.778.20.97, -0.210.9903295098
2024-11-19 23:06:001219.1120-11.778.10.96, -0.210.9903295101
2024-11-19 23:09:001315.4102-11.778.60.97, -0.210.9903295102
2024-11-19 23:12:001411.482-11.779.00.97, -0.210.9903295105
2024-11-19 23:15:00156.849-11.880.30.97, -0.210.9903295109
2024-11-19 23:18:00164.634-11.881.30.97, -0.211.0003295110
2024-11-19 23:21:00173.023-11.881.70.97, -0.211.0003295111

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 )