Solar Images Sunday, 14 June 2026
‹ 12.06.2026 2026 15.06.2026 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:40 UT
- Observer
- Ergün EGE
- g
- 4
- f
- 20
- R
- 60
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=14.06.2026 Saat=08:40 Gözlemci=Ergün EGE KontrolEden=İrem ÖZDEMİR Durumaçısı=-10.07 Enlemaçısı=0.91 Boylamaçısı=290.46 Boylamfark=2 GKalite=3 GDurum= Kuzeyaçısı=-0.3 Sırano=20485 AyRasatNo=9 RasatÖnceki=12.06.2026 RasatSonraki=15.06.2026 [Leke Grupları] Grupsayısı=4:3:1 LekeSayısı=20:15:5 RölatifSayı=60:45:15 01=HS_ 01 +17.484 +44.103 334.563 +0.000 0000 0 +18.250 +45.870 +16.717 +43.119 +17.484 +44.979 +17.484 +43.228 02=CAI 09 +08.932 +02.950 292.555 +0.000 0000 0 +11.660 +06.946 +06.204 -02.757 +08.932 +06.746 +08.932 -02.557 03=BXO 05 +10.370 -47.252 243.208 +0.000 0000 0 +10.695 -45.606 +09.379 -48.899 +10.370 -46.105 +10.370 -48.398 04=CAO 05 -13.110 +45.791 336.251 +0.000 0000 0 -10.419 +50.670 -15.603 +40.913 -13.110 +50.470 -13.110 +41.11320260614.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 →
2026/20260614 · · 7 frames · 150.0 MB · 08:46:17–08:57:34 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.









