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 10240
Detector 24h operating status:

Last processed image:    
   0 hours and 36 minutes ago (2024-06-17 18:33 UTC)
Last detected dimming:
   0 hours and 35 minutes ago (2024-06-17 18:33 UTC)


Overview for dimming #:
   10240           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 #: 10240          
timeseq #total
intensity
max
intensity
median
intensity
areasizelatlonx,y in R☉dist.
R☉
detectionImg ID
2024-05-26 23:36:1110.00.00.00.00 , 0.003130453
2024-05-26 23:39:1120.00.00.00.00 , 0.003130454
2024-05-26 23:42:1130.00.00.00.00 , 0.003130455
2024-05-26 23:45:1140.00.00.00.00 , 0.003130456
2024-05-26 23:48:1150.00.00.00.00 , 0.003130457
2024-05-26 23:51:116-1.5-7.7-7.20.01911.14, 0.411.219.303130458
2024-05-26 23:54:117-3.0-8.1-7.50.03861.14, 0.421.210.003130466
2024-05-26 23:57:118-3.9-9.0-7.70.04881.14, 0.411.210.003130467
2024-05-27 00:00:119-5.3-9.5-8.20.36271.14, 0.411.210.003130468
2024-05-27 00:03:1110-6.8-9.7-8.20.77961.15, 0.401.220.003130469
2024-05-27 00:06:1111-9.3-10.3-8.41.010491.15, 0.401.210.003130470
2024-05-27 00:09:1112-11.0-11.4-8.91.111881.16, 0.391.230.003130471
2024-05-27 00:12:1113-12.9-11.6-9.21.413721.16, 0.391.220.003130472
2024-05-27 00:15:1114-13.1-12.1-9.51.413571.15, 0.391.220.003130473

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 )