S13E84 Data 2022-05-11
Long Jupiter 156 area 30
New region 13010 [S13E84] 30 rotated partly into view on May 11 as S7563 [S13E84]S14E76 Data 2022-05-12
Long Jupiter 165 area 30
New region 13010 [S14E76] 30 rotated partly into view on May 11 and was numbered the next day by SWPC as all spots became visible. There may be a magnetic delta in the southeasternmost penumbra, however, we will have to wait until that spot rotates into better view to be certain. C1 flares: C1.6 @ 17:59 UTS14E64 Data 2022-05-13
Long Jupiter 178 area 90
Region 13010 [S14E64] 90 was mostly quiet and stable. C1 flares: C1.7 at 06:10 UTS14E49 Data 2022-05-14
Long Jupiter -166 area 190
Region 13010 [S14E49] 190 decayed as all but one of the larger spots lost mature penumbra and fragmented into smaller spots.S16E37 Data 2022-05-15
Long Jupiter -153 area 190
Region 13010 [S16E37] 190 decayed slowly and has only tiny spots and small spots with rudimentary penumbra.S17E22 Data 2022-05-16
Long Jupiter -137 area 100
Region 13010 [S17E22] 100 decayed slowly losing spots and area.S17E22 Data 2022-05-17
Long Jupiter -138 area 60
Region 13010 [S17E22] 60 decayed slowly and was mostly quiet.S16W05 Data 2022-05-18
Long Jupiter -110 area 70
Region 13010 [S16W05] 70 gained a few spots as new flux emerged near the center of the region causing polarity intermixing.S16W18 Data 2022-05-19
Long Jupiter -96 area 50
Region 13010 [S16W18] 50 decayed slowly and was mostly quiet.S16W30 Data 2022-05-20
Long Jupiter -83 area 20
Region 13010 [S16W30] 20S16W44 Data 2022-05-21
Long Jupiter -68 area 20
Region 13010 [S16W44] 20 decayed slowly producing a couple of C flares. C1 flares: C1.9 @ 19:06 UTS16W57 Data 2022-05-22
Long Jupiter -54 area 10
Region 13010 [S16W57] 10 decayed slowly and quietly.S16W73 Data 2022-05-23
Long Jupiter -37 area 10
Region 13010 [S16W73] 10 decayed slowly and quietly.
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. |