Solar Images Saturday, 8 March 2025
‹ 07.03.2025 2025 09.03.2025 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 09:00 UT
- Observer
- Ergün EGE
- g
- 5
- f
- 27
- R
- 77
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=8.03.2025 Saat=09:00 Gözlemci=Ergün EGE KontrolEden=Korhan YELKENCİ Durumaçısı=-23.23 Enlemaçısı=-7.25 Boylamaçısı=282.62 Boylamfark=2 GKalite=3 GDurum=B.A , H.S Kuzeyaçısı=-0.4 Sırano=20202 AyRasatNo=6 RasatÖnceki=07.03.2025 RasatSonraki=09.03.2025 [Leke Grupları] Grupsayısı=5:1:4 LekeSayısı=27:2:25 RölatifSayı=77:12:65 01=HS_ 02 +05.680 -65.360 217.584 +0.000 0000 0 +06.360 -64.330 +05.000 -66.400 +05.680 -64.825 +05.680 -65.895 02=AX_ 01 -16.655 +24.874 307.494 +0.000 0000 0 -16.311 +25.174 -16.998 +24.573 -16.655 +24.675 -16.655 +25.730 03=EHC 19 -14.249 +12.909 295.529 +0.000 0000 0 -12.134 +20.603 -16.363 +05.216 -14.249 +20.403 -14.249 +05.416 04=AX_ 03 -25.121 -04.744 277.876 +0.000 0000 0 -24.490 -03.820 -25.752 -05.669 -25.121 -04.319 -25.121 -05.168 05=HS_ 02 -20.532 -48.354 234.266 +0.000 0000 0 -19.332 -46.528 -21.732 -50.181 -20.532 -47.280 -20.532 -49.68120250308.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 →
2025/20250308_ee · EE · 3 frames · 64.3 MB · 09:18:52–09:26:37 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.





