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 14250
Detector 24h operating status:

Last processed image:    
   0 hours and 19 minutes ago (2025-10-29 06:48 UTC)
Last detected dimming:
   1 hours and 13 minutes ago (2025-10-29 05:54 UTC)


Overview for dimming #:
   14250           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 #: 14250          
timeseq #total
intensity
max
intensity
median
intensity
areasizelatlonx,y in R☉dist.
R☉
detectionImg ID
2025-10-27 10:51:1110.00.00.00.00 , 0.003570302
2025-10-27 10:54:1120.00.00.00.00 , 0.003570305
2025-10-27 10:57:1130.00.00.00.00 , 0.003570306
2025-10-27 11:00:1140.00.00.00.00 , 1.323570311
2025-10-27 11:03:1150.00.00.00.00 , 2.373570312
2025-10-27 11:06:1160.00.0-10.70.03-15.245.90.70, -0.320.772.583570313
2025-10-27 11:09:117-0.1-0.8-9.90.09-15.145.60.70, -0.320.771.773570314
2025-10-27 11:12:1180.00.0-13.90.03-15.245.90.70, -0.320.770.953570319
2025-10-27 11:15:119-0.2-1.4-16.50.111-15.446.10.70, -0.320.770.003570320
2025-10-27 11:18:11100.00.0-9.40.03-15.245.40.70, -0.320.770.863570321
2025-10-27 11:21:1111-0.1-0.4-10.70.08-15.344.80.69, -0.320.760.003570322
2025-10-27 11:24:11120.00.0-11.90.04 , 0.003570325
2025-10-27 11:27:1113-0.1-0.5-12.20.012 , 0.003570328
2025-10-27 11:30:1114-0.4-2.5-10.30.134 , 0.003570329

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 )