Solar Images Monday, 27 June 2022
‹ 26.06.2022 2022 28.06.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 09:45 UT
- Observer
- Hikmet ÇAKMAK
- g
- 4
- f
- 18
- R
- 58
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=27.06.2022 Saat=09:45 Gözlemci=Hikmet ÇAKMAK KontrolEden=Talar YONTAN Durumaçısı=-4.35 Enlemaçısı=2.43 Boylamaçısı=321.39 Boylamfark=1 GKalite=3 GDurum=G.T , H.S Kuzeyaçısı=-0.1 Sırano=19474 AyRasatNo=26 RasatÖnceki=26.06.2022 RasatSonraki=28.06.2022 [Leke Grupları] Grupsayısı=4:2:2 LekeSayısı=18:8:10 RölatifSayı=58:28:30 01=BXI 06 +15.639 +59.260 020.650 18.221 0000 0 +17.900 +62.403 +14.269 +56.117 +14.820 +61.990 +16.281 +56.657 02=AX_ 02 +08.682 -02.585 318.805 +0.000 0000 0 +08.920 -02.163 +08.443 -03.800 +08.682 -02.266 +08.682 -02.904 03=CAI 08 -12.437 +01.900 323.290 22.380 0000 0 -10.450 +04.571 -14.423 -00.772 -11.944 +03.874 -13.656 -00.288 04=AX_ 02 -19.284 -34.756 286.634 +0.000 0000 0 -18.767 -33.435 -19.800 -36.760 -19.284 -33.594 -19.284 -35.91820220627.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 →
2022/20220627_hc · HC · 4 frames · 85.7 MB · 09:46:26–09:57:52 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.






