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:
   217 hours and 47 minutes ago (2024-04-11 04:14 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 12198
Flare 12198


Details for flare #: 12198          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2017-09-09 21:06:00123.094-9.479.90.98, -0.180.9904597115
2017-09-09 21:08:00228.8106-9.080.80.98, -0.181.0004597116
2017-09-09 21:10:00336.5133-9.082.00.98, -0.171.0004597117
2017-09-09 21:12:00445.71540.99, -0.171.0004597118
2017-09-09 21:14:00559.11980.99, -0.181.0004597119
2017-09-09 21:16:00669.62250.99, -0.181.0104597120
2017-09-09 21:18:00772.12190.99, -0.171.0104597121
2017-09-09 21:20:00872.12031.00, -0.171.0104597122
2017-09-09 21:22:00971.01891.00, -0.171.0104597123
2017-09-09 21:24:001069.61911.00, -0.171.0104597124
2017-09-09 21:26:001169.92151.00, -0.181.0104597125
2017-09-09 21:28:001262.92011.00, -0.181.0104597126
2017-09-09 21:30:001357.01971.00, -0.181.0104597127
2017-09-09 21:32:001449.01801.00, -0.181.0204597128
2017-09-09 21:34:001541.61651.00, -0.181.0204597129
2017-09-09 21:36:001634.91491.00, -0.181.0204597130
2017-09-09 21:38:001728.51321.00, -0.181.0204597131
2017-09-09 21:40:001824.41241.00, -0.191.0204597132
2017-09-09 21:42:001918.91031.00, -0.191.0204597133
2017-09-09 21:44:002014.6841.00, -0.191.0204597134
2017-09-09 21:46:002111.0651.00, -0.191.0204597135

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 )