Solar Images Monday, 29 August 2022
‹ 28.08.2022 2022 30.08.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:30 UT
- Observer
- Hikmet ÇAKMAK
- g
- 4
- f
- 40
- R
- 80
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=29.08.2022 Saat=08:30 Gözlemci=Hikmet ÇAKMAK KontrolEden=Ergün EGE Durumaçısı=20.33 Enlemaçısı=7.14 Boylamaçısı=208.83 Boylamfark=2 GKalite=3 GDurum=G.T , H.S Kuzeyaçısı=-0.4 Sırano=19536 AyRasatNo=29 RasatÖnceki=28.08.2022 RasatSonraki=30.08.2022 [Leke Grupları] Grupsayısı=4:1:3 LekeSayısı=40:2:38 RölatifSayı=80:12:68 01=?__ 02 +31.335 +79.919 288.749 +0.000 0000 0 +32.345 +81.281 +30.324 +78.558 +31.335 +80.781 +31.335 +79.570 02=BXO 03 -23.130 +28.707 237.537 +0.000 0000 0 -22.627 +31.400 -23.398 +26.130 -23.130 +30.842 -23.130 +26.572 03=AX_ 01 -13.231 +03.755 212.585 -1.000 0000 0 -13.231 +03.755 -13.231 +03.755 04=EAC 34 -21.542 -16.337 192.493 13.848 0000 0 -18.611 -09.926 -24.472 -22.747 -23.260 -11.195 -20.754 -21.41920220829.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 →
2022/20220829_hc · HC · 11 frames · 235.7 MB · 08:23:46–09:27:36 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.













