Solar Demon Dimming Detection (qlk)

Quick-look! running in real time on SDO/AIA 211 QLK data
3 minute cadence, typical delay 15 minutes
(detection version 1.00)
(view all Solar Demon detection tools)

Overview of dimming 14850
Detector 24h operating status:

Last processed image:    
   0 hours and 18 minutes ago (2026-03-12 13:42 UTC)
Last detected dimming:
   4 hours and 51 minutes ago (2026-03-12 09:09 UTC)


Overview for dimming #:
   14850           back to overview

Animations and graphs
   derotated original images ( non-derotated )
   dimming intensity ( overlaid on HMI )
   dimming mask

   base difference ( percentage )
   running difference ( percentage )

more

more

more


Details for dimming #: 14850          
timeseq #total
intensity
max
intensity
median
intensity
areasizelatlonx,y in R☉dist.
R☉
detectionImg ID
2026-01-12 03:42:1110.00.00.00.00 , 0.003642581
2026-01-12 03:45:1120.00.00.00.00 , 0.003642584
2026-01-12 03:48:1130.00.00.00.00 , 0.003642585
2026-01-12 03:51:1140.00.00.00.00 , 0.003642590
2026-01-12 03:54:115-1.0-6.5-9.20.0106 , 0.003642591
2026-01-12 03:57:116-2.3-10.9-10.20.1209 , 2.943642592
2026-01-12 04:00:117-3.8-12.9-10.51.0345-0.90, -0.471.020.003642593
2026-01-12 04:03:118-4.6-14.9-11.70.5374-0.90, -0.471.020.003642596
2026-01-12 04:06:119-5.8-15.7-11.51.8469-0.90, -0.461.010.003642597
2026-01-12 04:09:1110-7.1-16.8-11.42.0542-0.91, -0.451.010.003642602
2026-01-12 04:12:1111-7.5-17.4-11.91.2526-0.91, -0.451.010.003642603
2026-01-12 04:15:1112-9.2-18.9-11.72.7668-0.90, -0.461.020.003642604
2026-01-12 04:18:1113-9.7-19.8-12.32.9685-0.91, -0.451.010.873642605
2026-01-12 04:21:1114-9.6-20.3-12.42.3685-0.91, -0.461.020.003642609

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 )