Solar Images Saturday, 29 January 2022
‹ 28.01.2022 2022 30.01.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 09:55 UT
- Observer
- Özgecan ÖNALTAŞ
- g
- 4
- f
- 50
- R
- 90
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=29.01.2022 Saat=09:55 Gözlemci=Özgecan ÖNALTAŞ KontrolEden=Burçin TANIK Durumaçısı=-11.07 Enlemaçısı=-5.81 Boylamaçısı=128.42 Boylamfark=1 GKalite=3 GDurum=B.A , Y.B , H.S Kuzeyaçısı=0.0 Sırano=19364 AyRasatNo=14 RasatÖnceki=28.01.2022 RasatSonraki=30.01.2022 [Leke Grupları] Grupsayısı=4:2:2 LekeSayısı=50:44:6 RölatifSayı=90:64:26 01=BXI 04 +27.724 +49.463 177.883 14.394 0000 0 +28.896 +52.804 +26.552 +46.121 +26.841 +51.457 +28.400 +46.919 02=DKC 40 +16.431 -13.617 114.803 08.234 0000 0 +19.176 -08.100 +13.687 -19.133 +17.452 -09.259 +16.237 -17.683 03=HS_ 01 -24.916 +41.269 169.689 +0.000 0000 0 -23.919 +42.130 -25.914 +40.408 -24.916 +41.630 -24.916 +40.908 04=BXI 05 -20.392 +30.417 158.837 19.427 0000 0 -18.168 +34.115 -22.615 +26.719 -19.130 +33.447 -21.810 +27.57020220129.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 →
2022/20220129_ot · OT · 2 frames · 42.9 MB · 10:37:08–10:38:17 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.




