Connection failed: SQLSTATE[HY000] [1040] Too many connections Solar Demon Flare Detection (sc)
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:
   212 hours and 27 minutes ago (2022-01-15 23:54 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 2727
Flare 2727


Details for flare #: 2727          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2011-10-22 15:18:03113.95511.2-23.7-0.40, 0.110.4101189573
2011-10-22 15:20:03221.87311.1-23.9-0.40, 0.110.4201189574
2011-10-22 15:22:03328.19711.0-23.9-0.40, 0.110.4201189575
2011-10-22 15:24:03436.915310.8-23.5-0.39, 0.100.4101189576
2011-10-22 15:26:03544.019710.7-22.9-0.39, 0.100.4001189577
2011-10-22 15:28:03645.221310.8-22.3-0.38, 0.100.3901189578
2011-10-22 15:30:03744.820810.8-22.0-0.37, 0.100.3901189579
2011-10-22 15:32:03841.618510.8-21.8-0.37, 0.100.3801189580
2011-10-22 15:34:03940.718610.8-21.8-0.37, 0.100.3801189581
2011-10-22 15:36:031037.317510.7-21.9-0.37, 0.100.3801189582
2011-10-22 15:38:031131.714810.6-22.0-0.37, 0.100.3801189583
2011-10-22 15:40:031227.513210.5-22.0-0.37, 0.100.3801189584
2011-10-22 15:42:031324.512010.5-21.9-0.37, 0.100.3801189585
2011-10-22 15:44:031419.99810.4-22.1-0.37, 0.100.3901189586
2011-10-22 15:46:031516.38410.4-22.1-0.37, 0.100.3901189587
2011-10-22 15:48:031613.06910.4-22.0-0.37, 0.100.3801189588
2011-10-22 15:50:031710.96110.4-21.9-0.37, 0.100.3801189589

Solar Demon estimated flare class:
C2

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 )