Solar Images Monday, 27 September 2021
‹ 26.09.2021 2021 28.09.2021 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:00 UT
- Observer
- Hikmet ÇAKMAK
- g
- 4
- f
- 15
- R
- 55
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=27.09.2021 Saat=08:00 Gözlemci=Hikmet ÇAKMAK KontrolEden=Korhan YELKENCİ Durumaçısı=25.67 Enlemaçısı=6.88 Boylamaçısı=323.75 Boylamfark=2 GKalite=3 GDurum=G.T , H.S Kuzeyaçısı=-0.3 Sırano=19286 AyRasatNo=23 RasatÖnceki=26.09.2021 RasatSonraki=28.09.2021 [Leke Grupları] Grupsayısı=4:1:3 LekeSayısı=15:1:14 RölatifSayı=55:11:44 01=AX_ 01 +14.210 +20.929 344.679 -1.000 0000 0 +14.210 +20.929 +14.210 +20.929 02=HA_ 06 -27.740 +30.370 353.787 +0.000 0000 0 -25.808 +31.542 -29.672 +28.532 -27.740 +31.375 -27.740 +29.365 03=AX_ 02 -17.728 +03.661 327.411 +0.000 0000 0 -16.692 +04.111 -18.764 +03.211 -17.728 +03.611 -17.728 +03.711 04=BXO 06 -22.500 -31.579 292.171 13.355 0000 0 -21.340 -29.437 -23.670 -33.722 -21.556 -30.121 -22.283 -33.18620210927.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 →
2021/20210927_hc · HC · 11 frames · 235.7 MB · 08:02:02–08:38:17 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.













