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 7842
Detector 24h operating status:

Last processed image:    
   0 hours and 32 minutes ago (2023-12-01 22:54 UTC)
Last detected dimming:
   0 hours and 32 minutes ago (2023-12-01 22:54 UTC)


Overview for dimming #:
   7842           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 #: 7842          
timeseq #total
intensity
max
intensity
median
intensity
areasizelatlonx,y in R☉dist.
R☉
detectionImg ID
2023-09-23 02:09:111-0.7-5.2-7.30.393 , 0.002901499
2023-09-23 02:12:112-11.8-12.5-9.43.812031.11.50.03, -0.110.110.002901500
2023-09-23 02:15:113-20.2-17.2-12.05.116401.61.70.03, -0.100.1022.972901507
2023-09-23 02:18:114-30.2-22.6-14.96.219771.72.70.05, -0.090.1018.322901508
2023-09-23 02:21:115-38.7-27.0-17.66.721541.52.50.04, -0.100.1113.632901509
2023-09-23 02:24:116-46.6-30.3-19.07.624021.52.60.05, -0.100.118.632901510
2023-09-23 02:27:117-55.2-34.2-19.58.726951.62.70.05, -0.100.1110.242901511
2023-09-23 02:30:118-63.3-39.7-19.69.629581.62.80.05, -0.100.110.002901512
2023-09-23 02:33:119-71.6-43.4-20.910.33134 , 0.982901517
2023-09-23 02:36:1110-78.8-49.0-22.810.33165 , 0.002901518
2023-09-23 02:39:1111-85.3-51.2-24.610.43207 , 0.002901519
2023-09-23 02:42:1112-91.0-54.7-25.610.8328442.455.40.61, 0.620.880.002901520

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 )