S17E78 Data 2022-03-27
Long Jupiter 121 area 180
New region 12978 [S17E78] 180 rotated into view and has M class flare potential. C1 flares: C1.2 @ 15:18, C1.2 @ 16:18 UTS17E64 Data 2022-03-28
Long Jupiter 136 area 210
Region 12978 [S17E64] 210 has M class flare potential and was mostly quiet. C1 flares: C1.5 @ 08:41 UT.S17E52 Data 2022-03-29
Long Jupiter 149 area 310
Region 12978 [S17E52] 310 was mostly quiet and stable and has M class flare potential.S17E38 Data 2022-03-30
Long Jupiter 164 area 670
Region 12978 [S17E38] 670 was mostly quiet and stable and has M class flare potential.S17E25 Data 2022-03-31
Long Jupiter 178 area 400
Region 12978 [S17E25] 400 was mostly quiet and stable and has M class flare potential.S17E13 Data 2022-04-01
Long Jupiter -169 area 410
Region 12978 [S17E13] 410 developed as new flux emerged in the intermediate spot section. Flare activity increased. C1 flares: C1.9 @ 08:35, C1.8 @ 16:16, C1.6 @ 20:00 UTS16W14 Data 2022-04-03
Long Jupiter -140 area 440
Region 12978 [S16W14] 440 decayed slowly and was mostly quiet. C1 flares: C1.8 @ 01:30 UTS16W27 Data 2022-04-04
Long Jupiter -127 area 370
Region 12978 [S16W27] 370 was mostly quiet and stable.S17W40 Data 2022-04-05
Long Jupiter -113 area 350
Region 12978 [S17W40] 350 was mostly quiet and stable. C1 flares: C1.2 @ 07:58 UTS17W52 Data 2022-04-06
Long Jupiter -101 area 290
Region 12978 [S17W52] 290 decayed slowly and was mostly quiet. C1 flares: C1.3 @ 04:20 UTRegion 12978 [S17W52] 290 decayed slowly and was mostly quiet. C1 flares: C1.3 @ 04:20 UTS17W67 Data 2022-04-07
Long Jupiter -84 area 260
Region 12978 [S17W67] 260 decayed slowly and quietly.S17W80 Data 2022-04-08
Long Jupiter -70 area 250
Region 12978 [S17W80] 250 decayed slowly. The region was quiet early on, however, a slow increase in activity was noted after noon and during the first half of April 9 with several C flares occurring.
Stefano Zottele - S-Spots Data from Jan Alvested Solen info Position data from Agostino Frosini - Agopax.it Images: Jan Alvested from Solen.info AND Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams. |