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:
   215 hours and 7 minutes ago (2024-04-27 23:32 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 30814
Flare 30814


Details for flare #: 30814          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2024-04-14 06:22:0014.336-0.98, -0.191.0007937724
2024-04-14 06:24:00210.654-0.98, -0.191.0007937725
2024-04-14 06:26:00310.960-0.99, -0.191.0007937726
2024-04-14 06:28:0047.854-0.99, -0.191.0007937727
2024-04-14 06:30:0057.462-0.99, -0.181.0007937728
2024-04-14 06:32:0065.346-0.99, -0.181.0007937729
2024-04-14 06:34:0074.339-0.99, -0.181.0007937730
2024-04-14 06:36:0084.339-0.99, -0.181.0107937731
2024-04-14 06:38:0097.566-0.98, -0.191.0007937732
2024-04-14 06:40:001012.9107-11.5-83.7-0.98, -0.191.0007937733
2024-04-14 06:42:001114.2117-11.5-83.9-0.98, -0.191.0007937734
2024-04-14 06:44:001214.6118-11.5-84.4-0.98, -0.191.0007937735
2024-04-14 06:46:001315.0120-0.98, -0.191.0007937736
2024-04-14 06:48:001412.4101-0.98, -0.191.0007937737
2024-04-14 06:50:001510.083-11.5-84.5-0.98, -0.191.0007937738
2024-04-14 06:52:00167.254-11.7-83.3-0.98, -0.191.0007937739
2024-04-14 06:54:00176.448-11.6-83.3-0.98, -0.191.0007937740
2024-04-14 06:56:00185.744-11.7-83.4-0.98, -0.191.0007937741
2024-04-14 06:58:00193.931-11.7-83.9-0.98, -0.191.0007937742
2024-04-14 07:00:00202.421-11.7-83.9-0.98, -0.191.0007937743

Solar Demon estimated flare class:
B5

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 )