Solar Images Tuesday, 13 May 2025
‹ 12.05.2025 2025 14.05.2025 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 11:45 UT
- Observer
- Olcay PLEVNE
- g
- 5
- f
- 8
- R
- 58
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=13.05.2025 Saat=11:45 Gözlemci=Olcay PLEVNE KontrolEden=Burçin TANIK Durumaçısı=-21.31 Enlemaçısı=-2.84 Boylamaçısı=129.9 Boylamfark=0 GKalite=3 GDurum=K.T Kuzeyaçısı=0.0 Sırano=20243 AyRasatNo=9 RasatÖnceki=12.05.2025 RasatSonraki=14.05.2025 [Leke Grupları] Grupsayısı=5:4:1 LekeSayısı=8:7:1 RölatifSayı=58:47:11 01=BXI 02 +08.720 +71.938 201.838 +0.000 0000 0 +09.247 +73.829 +06.898 +70.470 +08.720 +73.629 +08.720 +70.247 02=AX_ 02 +02.294 +09.402 139.302 +0.000 0000 0 +02.957 +09.973 +01.630 +08.831 +02.294 +09.473 +02.294 +09.331 03=AX_ 01 +04.295 -01.250 128.875 -1.000 0000 0 +04.295 -01.250 +04.295 -01.250 04=HS_ 02 +15.298 -73.484 056.416 +0.000 0000 0 +17.493 -68.180 +13.104 -78.949 +15.298 -68.600 +15.298 -78.368 05=HS_ 01 -09.542 +54.641 184.541 +0.000 0000 0 -08.579 +56.500 -10.505 +53.232 -09.542 +55.775 -09.542 +53.50720250513.gzd
Chromosphere (H-α) FITS frames
The images are made automatically with a fixed, gentle rule: uneven illumination and most of the limb darkening are removed, and the brightness is shown on a linear scale (no sharpening); prominences get their own scale outside the limb. Frames are ordered by sharpness (seeing); frames without the Sun (darks, bias) come last. Method →
2025/20250513_op · OP · 4 frames · 85.7 MB · 11:45:04–11:49:53 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.






