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 10501
Detector 24h operating status:

Last processed image:    
   0 hours and 27 minutes ago (2024-07-03 06:54 UTC)
Last detected dimming:
   0 hours and 27 minutes ago (2024-07-03 06:54 UTC)


Overview for dimming #:
   10501           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 #: 10501          
timeseq #total
intensity
max
intensity
median
intensity
areasizelatlonx,y in R☉dist.
R☉
detectionImg ID
2024-06-22 06:21:1110.00.00.00.00 , 0.003154803
2024-06-22 06:24:1120.00.00.00.00 , 0.003154804
2024-06-22 06:27:1130.00.00.00.00 , 0.003154805
2024-06-22 06:30:114-1.6-10.0-11.20.7131-3.149.20.76, -0.080.770.003154806
2024-06-22 06:33:115-4.4-16.0-14.21.5302-3.249.40.77, -0.080.770.003154807
2024-06-22 06:36:116-10.3-24.5-15.03.3632-3.349.50.77, -0.080.7710.563154808
2024-06-22 06:39:117-14.2-28.3-15.34.3814-3.646.90.74, -0.090.7414.613154815
2024-06-22 06:42:118-16.8-32.0-17.44.7876-3.746.80.74, -0.090.744.443154816
2024-06-22 06:45:119-18.9-35.9-17.55.0930-3.747.20.74, -0.090.750.003154817
2024-06-22 06:48:1110-19.8-38.2-19.74.9911-3.747.30.74, -0.090.750.003154818
2024-06-22 06:51:1111-19.9-37.3-20.64.7885-3.747.00.74, -0.090.740.003154819
2024-06-22 06:54:1112-18.3-36.7-21.04.3800-3.747.10.74, -0.090.750.003154820

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 )