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:
   204 hours and 16 minutes ago (2024-08-31 23:58 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 34576
Flare 34576


Details for flare #: 34576          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2024-07-31 17:12:0012.722-24.0-52.8-0.73, -0.460.8708091929
2024-07-31 17:14:0024.434-24.0-53.1-0.74, -0.460.8708091930
2024-07-31 17:16:0036.843-24.1-53.1-0.74, -0.460.8708091931
2024-07-31 17:18:00410.457-23.9-53.2-0.74, -0.460.8708091932
2024-07-31 17:20:00517.374-23.9-53.4-0.74, -0.460.8708091933
2024-07-31 17:22:00621.781-23.9-53.6-0.74, -0.460.8708091934
2024-07-31 17:24:00722.280-24.0-53.7-0.74, -0.460.8708091935
2024-07-31 17:26:00820.176-24.0-53.8-0.74, -0.460.8808091936
2024-07-31 17:28:00917.471-24.0-53.8-0.74, -0.460.8808091937
2024-07-31 17:30:001014.663-24.0-53.8-0.74, -0.460.8808091938
2024-07-31 17:32:001112.056-24.1-53.8-0.74, -0.460.8808091939
2024-07-31 17:34:00129.851-24.1-53.8-0.74, -0.460.8808091940
2024-07-31 17:36:00137.843-24.0-53.6-0.74, -0.460.8708091941
2024-07-31 17:38:00146.138-24.0-53.6-0.74, -0.460.8708091942
2024-07-31 17:40:00154.831-24.0-53.2-0.74, -0.460.8708091943
2024-07-31 17:42:00163.727-24.0-53.3-0.74, -0.460.8708091944
2024-07-31 17:44:00172.719-23.9-53.1-0.74, -0.460.8708091945
2024-07-31 17:46:00182.316-23.9-52.8-0.73, -0.460.8708091946

Solar Demon estimated flare class:
B7

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 )