Solar Images Tuesday, 6 May 2025
‹ 05.05.2025 2025 07.05.2025 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 07:25 UT
- Observer
- Süleyman FİŞEK
- g
- 4
- f
- 44
- R
- 84
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=6.05.2025 Saat=07:25 Gözlemci=Süleyman FİŞEK KontrolEden=Burçin TANIK Durumaçısı=-23.03 Enlemaçısı=-3.63 Boylamaçısı=224.85 Boylamfark=3 GKalite=3 GDurum=K.T Kuzeyaçısı=-0.6 Sırano=20238 AyRasatNo=4 RasatÖnceki=05.05.2025 RasatSonraki=07.05.2025 [Leke Grupları] Grupsayısı=4:3:1 LekeSayısı=44:35:9 RölatifSayı=84:65:19 01=HH_ 01 +05.656 +79.369 304.219 +0.000 0000 0 +06.495 +81.800 +04.818 +77.730 +05.656 +80.904 +05.656 +77.834 02=FKC 27 +07.666 +17.141 241.991 +0.000 0000 0 +11.773 +26.204 +03.559 +08.780 +07.666 +26.400 +07.666 +08.278 03=DAC 07 +06.759 -13.200 211.830 +0.000 0000 0 +07.881 -09.560 +05.637 -16.481 +06.759 -09.760 +06.759 -16.281 04=ESC 09 -10.729 -44.200 180.830 +0.000 0000 0 -09.630 -38.894 -12.395 -49.145 -10.729 -39.940 -10.729 -48.94520250506.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 →
2025/20250506_sf · SF · 6 frames · 128.5 MB · 07:29:42–07:32:12 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.








