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 13 minutes ago (2024-04-22 23:48 UTC)

Animations and brightness graph
   fixed brightness
   adaptive brightness
location of flare 15860
Flare 15860


Details for flare #: 15860          
timeseq #brightnesssizelatlonX,Y in R☉dist.
R☉
BloomingImg ID
2022-02-10 02:04:0012.71616.058.60.83, 0.330.8906894182
2022-02-10 02:06:00212.34915.858.80.83, 0.330.8906894183
2022-02-10 02:08:00322.37115.859.00.83, 0.330.8906894184
2022-02-10 02:10:00427.910115.759.30.83, 0.330.9006894185
2022-02-10 02:12:00533.916315.760.00.84, 0.330.9006894186
2022-02-10 02:14:00635.918115.660.40.84, 0.320.9006894187
2022-02-10 02:16:00737.019515.760.60.85, 0.320.9106894188
2022-02-10 02:18:00835.619515.760.80.85, 0.320.9106894189
2022-02-10 02:20:00932.618715.761.00.85, 0.320.9106894190
2022-02-10 02:22:001029.017515.761.10.85, 0.320.9106894191
2022-02-10 02:24:001124.515415.761.20.85, 0.320.9106894192
2022-02-10 02:26:001220.613415.761.10.85, 0.320.9106894193
2022-02-10 02:28:001316.311115.761.20.85, 0.320.9106894194
2022-02-10 02:30:001413.19615.761.30.85, 0.320.9106894195
2022-02-10 02:32:00159.67415.761.20.85, 0.320.9106894196
2022-02-10 02:34:00167.25815.761.00.85, 0.320.9106894197
2022-02-10 02:36:00174.73715.860.80.85, 0.330.9106894198
2022-02-10 02:38:00183.52715.860.70.85, 0.330.9106894199
2022-02-10 02:40:00192.41915.960.70.84, 0.330.9106894200

Solar Demon estimated flare class:
C1

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 )