Solar Demon Flare Detection (sc)

Science! running on SDO/AIA 94 Synoptic data
2 minute cadence, typical delay 7 days
(detection version 1.00)
(view all Solar Demon detection tools)

Detector 14 day operating status:

Last detected flare:
   209 hours and 12 minutes ago (2024-04-24 23:54 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 26140
Flare 26140


Details for flare #: 26140          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2023-08-05 19:04:0016.43924.543.70.63, 0.350.7207612894
2023-08-05 19:06:00210.16424.043.40.63, 0.340.7207612895
2023-08-05 19:08:00314.08624.243.00.63, 0.340.7107612896
2023-08-05 19:10:00424.614924.743.20.63, 0.350.7207612897
2023-08-05 19:12:00544.827324.644.60.64, 0.350.7307612898
2023-08-05 19:14:00666.433724.744.90.65, 0.350.7407612899
2023-08-05 19:16:00781.336624.745.00.65, 0.350.7407612900
2023-08-05 19:18:00887.837724.645.20.65, 0.350.7407612901
2023-08-05 19:20:00990.138224.645.20.65, 0.350.7407612902
2023-08-05 19:22:001089.438824.745.20.65, 0.350.7407612903
2023-08-05 19:24:001182.737424.745.30.65, 0.350.7407612904
2023-08-05 19:26:001273.235924.745.40.65, 0.350.7407612905
2023-08-05 19:28:001361.232824.845.50.65, 0.350.7407612906
2023-08-05 19:30:001448.628824.945.50.65, 0.350.7407612907
2023-08-05 19:32:001537.425224.945.60.65, 0.360.7407612908
2023-08-05 19:34:001623.416624.946.10.66, 0.350.7507612909
2023-08-05 19:36:001714.010724.846.40.66, 0.350.7507612910
2023-08-05 19:38:00188.16924.746.70.67, 0.350.7507612911
2023-08-05 19:40:00192.82724.747.20.67, 0.350.7607612912

Solar Demon estimated flare class:
C3

Goes X-RAY flux timeline:

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 )