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:
   200 hours and 7 minutes ago (2024-04-10 23:58 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 11294
Flare 11294


Details for flare #: 11294          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2016-02-05 00:54:01118.939-11.5-10.0-0.17, -0.090.2003784998
2016-02-05 00:56:01243.460-11.5-10.0-0.17, -0.090.2003784999
2016-02-05 00:58:01363.169-11.5-10.0-0.17, -0.090.2003785000
2016-02-05 01:00:01462.284-11.4-10.1-0.17, -0.090.2003785001
2016-02-05 01:02:01552.381-11.4-10.1-0.17, -0.090.2003785002
2016-02-05 01:04:01639.573-11.4-10.1-0.17, -0.090.2003785003
2016-02-05 01:06:01729.166-11.4-10.1-0.17, -0.090.2003785004
2016-02-05 01:08:01822.061-11.3-10.1-0.17, -0.090.2003785005
2016-02-05 01:10:01922.778-11.1-10.0-0.17, -0.090.1903785006
2016-02-05 01:12:011020.480-10.9-9.9-0.17, -0.080.1903785007
2016-02-05 01:14:011119.485-10.8-9.8-0.17, -0.080.1903785008
2016-02-05 01:16:011217.986-10.6-9.6-0.17, -0.080.1803785009
2016-02-05 01:18:011315.076-10.5-9.5-0.16, -0.080.1803785010
2016-02-05 01:20:011412.565-10.4-9.4-0.16, -0.070.1803785011
2016-02-05 01:22:011512.261-10.4-9.4-0.16, -0.070.1803785012
2016-02-05 01:24:011612.564-10.3-9.4-0.16, -0.070.1803785013
2016-02-05 01:26:011711.359-10.3-9.4-0.16, -0.070.1803785014
2016-02-05 01:28:011810.355-10.3-9.4-0.16, -0.070.1803785015

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 )