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:
   204 hours and 59 minutes ago (2022-05-07 23:22 UTC)

Filters (category)
   All classes
   Only C class flares and above
   -- Only M class flares and above
   Only X class flares and above
Filters (time)
   Show all
   Last week
   -- Last 30 days
   Last 365 days
all detected flares
Flare 17036

Overview of flares
est.
class
startpeakend#latlondist.
R☉
ARest.
flux
GOES
flux
GOES peak
time
COMESEP# det.dimming

May, 2022
 5
M1
14:0614:1215:0016967-30-620.93AR 3006106.9276.214:10-29831028
 4
M2
07:5409:1010:1616940-1690.26AR 3004192.0575.808:59-119831572
-124
 4
M4
00:1600:2201:38169301.03388.6532.200:19-39831042
 3
M4
13:2213:3014:38169191.03434.61,133.613:25-59830939
 3
M1
07:4207:5808:28169151.01114.5136.207:53-59830924

April, 2022
30
M2
10:5813:5417:38168891.03242.61,131.313:47-798363199
30
M2
07:3010:0210:56168871.02206.9482.409:58-498314104
30
M1
04:5005:3806:34168861.03144.5142.605:34-49832053
-24
22
M1
13:2413:2813:42167792200.46AR 2993125.1343.313:25-39830710
-488
21
M7
01:5202:0402:241674123-230.59AR 2993729.0965.801:59-59831017
-1,082
20
M3
03:4804:0204:46167091.01287.72,246.603:57-59831130
-201
20
M1
00:4601:3802:20167051.01107.0729.401:36-29830848
-165
19
M1
20:2020:5822:46166961.02130.7370.820:49-99831673
-349
18
M1
17:1417:2818:56166501.01121.7192.117:24-49831150
-5
17
M7
03:2003:3806:18165971.02660.21,165.003:34-49831490
-1,434
16
M1
16:4002:2203:18165951.01115.6notin range-33298312319
-5

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 )