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 6494
Detector 24h operating status:

Last processed image:    
   0 hours and 33 minutes ago (2023-06-08 21:33 UTC)
Last detected dimming:
   0 hours and 33 minutes ago (2023-06-08 21:33 UTC)


Overview for dimming #:
   6494           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 #: 6494          
timeseq #total
intensity
max
intensity
median
intensity
areasizelatlonx,y in R☉dist.
R☉
detectionImg ID
2023-05-23 09:24:1110.00.00.00.00 , 0.002791283
2023-05-23 09:27:1120.00.00.00.00 , 0.002791284
2023-05-23 09:30:1130.00.00.00.00 , 0.002791285
2023-05-23 09:33:1140.00.00.00.00 , 0.002791286
2023-05-23 09:36:1150.00.00.00.00 , 0.932791287
2023-05-23 09:39:1160.00.00.00.00 , 2.632791295
2023-05-23 09:42:1170.00.00.00.00 , 2.582791296
2023-05-23 09:45:1180.00.00.00.00 , 0.002791297
2023-05-23 09:48:1190.00.00.00.00 , 0.002791298
2023-05-23 09:51:11100.00.00.00.00 , 1.542791299
2023-05-23 09:54:11110.00.00.00.00 , 1.722791300
2023-05-23 10:09:1112-0.6-6.1-11.40.24910.4-23.5-0.40, 0.210.450.002791308
2023-05-23 10:12:1113-1.4-9.3-13.80.410713.3-25.9-0.43, 0.260.500.002791309
2023-05-23 10:15:1114-1.8-10.7-13.40.513413.0-25.8-0.43, 0.260.500.002791317
2023-05-23 10:18:1115-2.1-12.6-14.00.514213.0-25.6-0.43, 0.250.500.002791318

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 )