Solar Images Monday, 16 January 2023
‹ 15.01.2023 2023 18.01.2023 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 10:25 UT
- Observer
- Hikmet ÇAKMAK
- g
- 12
- f
- 89
- R
- 209
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=16.01.2023 Saat=10:25 Gözlemci=Hikmet ÇAKMAK KontrolEden=Olcay PLEVNE Durumaçısı=-5.19 Enlemaçısı=-4.65 Boylamaçısı=161.74 Boylamfark=1 GKalite=3 GDurum=G.T , H.S Kuzeyaçısı=-0.3 Sırano=19639 AyRasatNo=10 RasatÖnceki=15.01.2023 RasatSonraki=18.01.2023 [Leke Grupları] Grupsayısı=12:5:7 LekeSayısı=89:43:46 RölatifSayı=209:93:116 01=EKI 14 +24.112 +06.125 167.865 11.409 0000 0 +26.876 +12.820 +21.347 +00.168 +23.830 +10.839 +25.630 +00.974 02=BXO 04 +20.450 -26.764 134.976 +0.000 0000 0 +20.932 -24.996 +19.967 -28.531 +20.450 -25.497 +20.450 -28.310 03=DAC 12 +10.444 -33.755 127.985 09.463 0000 0 +12.491 -29.232 +08.398 -38.278 +11.152 -30.430 +09.992 -37.405 04=AX_ 01 +10.102 -43.786 117.954 -1.000 0000 0 +10.102 -43.786 +10.102 -43.786 05=CAI 12 +18.302 -48.813 112.927 10.441 0000 0 +21.299 -39.282 +15.306 -58.344 +17.202 -42.300 +19.617 -55.528 06=CAO 03 -15.334 +65.480 227.220 23.272 0000 0 -13.428 +69.722 -17.239 +61.237 -14.113 +67.976 -16.729 +61.878 07=AX_ 01 -23.616 +46.899 208.639 -1.000 0000 0 -23.616 +46.899 -23.616 +46.899 08=CAI 05 -21.959 +34.883 196.623 13.901 0000 0 -20.811 +37.390 -23.107 +32.727 -21.546 +36.168 -22.306 +33.950 09=CAI 08 -12.903 +13.354 175.940 07.306 0000 0 -11.620 +21.162 -14.744 +05.547 -13.272 +18.173 -11.846 +06.976 10=BXI 09 -24.174 -17.211 144.529 09.248 0000 0 -22.851 -14.261 -25.497 -20.160 -24.434 -15.680 -23.646 -19.911 11=BXI 06 -22.782 -33.750 128.665 10.695 0000 0 -21.765 -30.230 -23.800 -35.920 -23.278 -30.817 -22.411 -35.414 12=EKI 14 -14.439 -45.247 116.493 06.515 0000 0 -11.907 -37.627 -16.971 -52.868 -14.306 -40.458 -15.624 -52.80020230116.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 →
2023/20230116_hc · HC · 4 frames · 85.7 MB · 10:25:51–10:42:12 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.






