Solar Images Friday, 28 January 2022
‹ 26.01.2022 2022 29.01.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:39 UT
- Observer
- Başar COŞKUNOĞLU
- g
- 4
- f
- 41
- R
- 81
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=28.01.2022 Saat=08:39 Gözlemci=Başar COŞKUNOĞLU KontrolEden=Özgecan ÖNALTAŞ Durumaçısı=-10.62 Enlemaçısı=-5.73 Boylamaçısı=142.28 Boylamfark=2 GKalite=3 GDurum= Kuzeyaçısı=-0.3 Sırano=19363 AyRasatNo=13 RasatÖnceki=26.01.2022 RasatSonraki=29.01.2022 [Leke Grupları] Grupsayısı=4:2:2 LekeSayısı=41:33:8 RölatifSayı=81:53:28 01=AX_ 03 +27.520 +33.365 175.645 +0.000 0000 0 +27.775 +33.813 +26.329 +32.917 +27.520 +33.313 +27.520 +33.417 02=DSC 30 +16.116 -31.312 110.968 +0.000 0000 0 +18.670 -26.397 +13.562 -36.227 +16.116 -26.597 +16.116 -36.270 03=HA_ 02 -25.100 +25.340 167.314 +0.000 0000 0 -24.360 +26.570 -25.984 +24.100 -25.100 +26.750 -25.100 +24.605 04=BXI 06 -20.305 +14.377 156.657 26.711 0000 0 -18.568 +17.325 -22.420 +11.428 -19.900 +16.412 -21.350 +11.75220220128.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 →
2022/20220128_bc · BC · 6 frames · 128.6 MB · 08:27:46–08:31:32 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.








