Solar Images Monday, 31 August 2026
‹ 30.08.2026 2026 01.09.2026 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 07:05 UT
- Observer
- Emre YILMAN
- g
- 3
- f
- 16
- R
- 46
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=31.08.2026 Saat=07:05 Gözlemci=Emre YILMAN KontrolEden=Emre YILMAN Durumaçısı=20.84 Enlemaçısı=7.18 Boylamaçısı=339.77 Boylamfark=3 GKalite=3 GDurum=G.T Kuzeyaçısı=-0.4 Sırano=20555 AyRasatNo=28 RasatÖnceki=30.08.2026 RasatSonraki=01.09.2026 [Leke Grupları] Grupsayısı=3:2:1 LekeSayısı=16:9:7 RölatifSayı=46:29:17 01=BXI 08 +07.536 +12.437 352.207 +0.000 0000 0 +09.340 +14.660 +06.390 +10.215 +07.536 +14.460 +07.536 +10.415 02=HS_ 01 +09.243 -75.985 263.785 +0.000 0000 0 +10.466 -74.856 +08.190 -77.114 +09.243 -75.356 +09.243 -76.614 03=DKO 07 -11.247 -03.478 336.292 +0.000 0000 0 -09.893 -00.635 -12.601 -06.321 -11.247 -00.835 -11.247 -06.12120260831.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 →
2026/20260831_ey · EY · 6 frames · 128.6 MB · 07:16:40–07:19:41 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.