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 10300
Detector 24h operating status:

Last processed image:    
   0 hours and 25 minutes ago (2025-01-18 21:15 UTC)
Last detected dimming:
   1 hours and 1 minutes ago (2025-01-18 20:39 UTC)


Overview for dimming #:
   10300           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 #: 10300          
timeseq #total
intensity
max
intensity
median
intensity
areasizelatlonx,y in R☉dist.
R☉
detectionImg ID
2024-06-02 13:57:1110.00.00.00.00 , 0.003136618
2024-06-02 14:00:1120.00.00.00.00 , 0.003136621
2024-06-02 14:03:1130.00.00.00.00 , 0.003136625
2024-06-02 14:06:1140.00.00.00.00 , 0.003136626
2024-06-02 14:09:1150.00.00.00.00 , 0.003136627
2024-06-02 14:12:116-1.4-8.3-13.50.687 , 0.933136628
2024-06-02 14:15:117-1.1-9.2-14.80.568 , 0.003136629
2024-06-02 14:18:118-1.7-10.7-12.80.8104 , 0.003136637
2024-06-02 14:21:119-2.4-11.1-8.41.31787.0-62.5-0.89, 0.130.900.003136638
2024-06-02 14:24:1110-2.6-11.0-7.72.02277.0-62.2-0.89, 0.130.900.003136639
2024-06-02 14:27:1111-3.3-13.6-7.42.62887.0-62.2-0.89, 0.130.900.003136640
2024-06-02 14:30:1112-3.0-12.6-7.72.42677.0-62.2-0.89, 0.130.900.003136641
2024-06-02 14:33:2313-3.5-12.2-7.62.93336.9-62.1-0.89, 0.120.900.003136642
2024-06-02 14:36:1114-4.4-11.8-7.53.64056.8-62.0-0.89, 0.120.890.003136650

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 )