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 5365
Detector 24h operating status:

Last processed image:    
   0 hours and 29 minutes ago (2024-04-25 22:57 UTC)
Last detected dimming:
   0 hours and 29 minutes ago (2024-04-25 22:57 UTC)


Overview for dimming #:
   5365           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 #: 5365          
timeseq #total
intensity
max
intensity
median
intensity
areasizelatlonx,y in R☉dist.
R☉
detectionImg ID
2023-01-24 00:48:1110.00.00.00.00 , 0.872683380
2023-01-24 00:51:4720.00.00.00.00 , 1.022683381
2023-01-24 00:54:1130.00.00.00.00 , 0.002683385
2023-01-24 00:57:1140.00.00.00.00 , 0.002683386
2023-01-24 01:00:1150.00.00.00.00 , 0.002683388
2023-01-24 01:03:1160.00.00.00.00 , 3.122683391
2023-01-24 01:06:1170.00.00.00.00 , 0.842683392
2023-01-24 01:09:1180.00.00.00.00 , 0.002683395
2023-01-24 01:12:119-0.8-6.4-8.20.38212.1-39.4-0.63, 0.280.692.142683396
2023-01-24 01:15:1110-0.9-5.9-9.80.48812.7-39.5-0.63, 0.290.690.002683399
2023-01-24 01:18:1111-2.4-9.3-8.51.125612.5-39.3-0.63, 0.290.690.002683400
2023-01-24 01:21:1112-3.8-11.8-8.91.738812.1-39.5-0.63, 0.280.690.002683401
2023-01-24 01:24:1113-4.9-12.7-9.32.149112.4-39.2-0.63, 0.290.690.002683404
2023-01-24 01:27:1114-4.6-11.7-9.12.046912.2-40.0-0.64, 0.280.700.002683405

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 )