Solar Images Sunday, 29 May 2022
‹ 28.05.2022 2022 30.05.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 11:30 UT
- Observer
- Başar COŞKUNOĞLU
- g
- 2
- f
- 3
- R
- 23
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=29.05.2022 Saat=11:30 Gözlemci=Başar COŞKUNOĞLU KontrolEden=Hikmet ÇAKMAK Durumaçısı=-16.37 Enlemaçısı=-1 Boylamaçısı=344.26 Boylamfark=0 GKalite=3 GDurum=G.T , H.S Kuzeyaçısı=-0.4 Sırano=19446 AyRasatNo=26 RasatÖnceki=28.05.2022 RasatSonraki=30.05.2022 [Leke Grupları] Grupsayısı=2:0:2 LekeSayısı=3:0:3 RölatifSayı=23:0:23 01=HA_ 02 -13.508 -21.600 323.254 +0.000 0000 0 -12.440 -19.517 -14.972 -22.495 -13.508 -20.611 -13.508 -22.589 02=HS_ 01 -33.730 -27.857 316.403 +0.000 0000 0 -32.191 -27.400 -33.955 -28.674 -33.730 -27.720 -33.730 -27.99420220529.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 →
2022/20220529_bc · BC · 6 frames · 128.6 MB · 11:53:39–11:58:34 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.