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 4833
Detector 24h operating status:

Last processed image:    
   0 hours and 17 minutes ago (2022-11-30 13:51 UTC)
Last detected dimming:
   1 hours and 44 minutes ago (2022-11-30 12:24 UTC)


Overview for dimming #:
   4833           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 #: 4833          
timeseq #total
intensity
max
intensity
median
intensity
areasizelatlonx,y in R☉dist.
R☉
detectionImg ID
2022-11-23 21:45:1110.00.00.00.00 , 0.002625349
2022-11-23 21:48:1120.00.00.00.00 , 0.002625352
2022-11-23 21:51:1130.00.00.00.00 , 0.002625353
2022-11-23 21:54:1140.00.00.00.00 , 0.002625354
2022-11-23 21:57:1150.00.00.00.00 , 0.002625357
2022-11-23 22:00:116-2.5-10.0-8.90.02631.09, -0.171.101.992625359
2022-11-23 22:03:117-4.9-13.1-9.70.04821.09, -0.171.100.002625361
2022-11-23 22:06:118-6.6-15.0-9.60.06261.09, -0.171.100.002625362
2022-11-23 22:09:119-8.9-16.7-9.90.08111.09, -0.171.100.002625365
2022-11-23 22:12:2310-10.9-18.9-9.90.09791.09, -0.171.100.002625366
2022-11-23 22:15:1111-13.6-20.8-9.80.011981.09, -0.161.100.002625369
2022-11-23 22:18:1112-17.9-23.8-10.10.015121.09, -0.161.100.002625370
2022-11-23 22:21:1113-20.3-25.6-10.50.016561.09, -0.161.100.002625373
2022-11-23 22:24:1114-23.1-27.7-10.00.018611.09, -0.161.100.002625374

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 )