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:    
   239 hours and 48 minutes ago (2024-11-26 23:45 UTC)
Last detected flare:
   240 hours and 51 minutes ago (2024-11-26 22:42 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 15197
Flare 15197


Details for flare #: 15197          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2023-09-30 01:00:0012.41615.8-75.0-0.94, 0.240.9702907694
2023-09-30 01:03:0023.42015.9-75.0-0.94, 0.240.9702907695
2023-09-30 01:06:0034.82315.9-74.9-0.94, 0.240.9702907696
2023-09-30 01:09:00410.93615.9-74.7-0.93, 0.240.9702907704
2023-09-30 01:12:00514.53915.8-74.8-0.93, 0.240.9702907705
2023-09-30 01:15:00620.94515.8-75.0-0.94, 0.240.9702907706
2023-09-30 01:18:00729.45915.9-75.2-0.94, 0.240.9702907707
2023-09-30 01:21:00831.26515.9-75.2-0.94, 0.240.9702907714
2023-09-30 01:24:00926.56615.9-75.5-0.94, 0.250.9702907715
2023-09-30 01:27:001021.86415.9-75.8-0.94, 0.250.9702907716
2023-09-30 01:30:001119.05715.9-76.0-0.94, 0.250.9702907717
2023-09-30 01:33:001216.35015.9-76.2-0.94, 0.250.9702907718
2023-09-30 01:36:001313.14315.9-76.3-0.94, 0.250.9702907719
2023-09-30 01:39:00149.83315.9-76.4-0.94, 0.250.9702907720
2023-09-30 01:42:00156.72815.9-76.6-0.94, 0.250.9702907721
2023-09-30 01:45:00164.32115.9-76.8-0.94, 0.250.9702907722
2023-09-30 01:48:00173.21915.9-76.8-0.94, 0.250.9702907723

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 )