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:
   214 hours and 38 minutes ago (2021-07-19 22:18 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 14024
Flare 14024


Details for flare #: 14024          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2021-07-03 14:26:0013.02123.784.40.92, 0.401.0006579356
2021-07-03 14:28:00256.36823.380.20.91, 0.390.9916579357
2021-07-03 14:30:003306.027423.480.70.91, 0.390.99206579358
2021-07-03 14:32:004396.835223.381.10.91, 0.390.99346579359
2021-07-03 14:34:005354.831623.381.50.91, 0.390.99296579360
2021-07-03 14:36:006272.624623.281.80.92, 0.390.99196579361
2021-07-03 14:38:007220.019523.282.10.92, 0.391.00156579362
2021-07-03 14:40:008187.017923.282.40.92, 0.391.00116579363
2021-07-03 14:42:009137.113023.282.80.92, 0.391.0056579364
2021-07-03 14:44:001095.710123.283.20.92, 0.391.0026579365
2021-07-03 14:46:001171.89223.283.50.92, 0.391.0006579366
2021-07-03 14:48:001254.88423.383.70.92, 0.391.0006579367
2021-07-03 14:50:001340.98223.384.00.92, 0.391.0006579368
2021-07-03 14:52:001432.4800.92, 0.391.0006579369
2021-07-03 14:54:001524.6740.92, 0.391.0006579370
2021-07-03 14:56:001619.9740.92, 0.391.0006579371
2021-07-03 14:58:001716.5680.92, 0.391.0006579372
2021-07-03 15:00:001814.4610.92, 0.391.0006579373
2021-07-03 15:02:001914.6640.92, 0.391.0006579374
2021-07-03 15:04:002015.8670.92, 0.391.0006579375

Solar Demon estimated flare class:
M4

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 )