Solar Images Friday, 23 June 2023
‹ 22.06.2023 2023 24.06.2023 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 10:13 UT
- Observer
- Başar COŞKUNOĞLU
- g
- 12
- f
- 101
- R
- 221
- Seeing
- 4 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=23.06.2023 Saat=10:13 Gözlemci=Başar COŞKUNOĞLU KontrolEden=Başar COŞKUNOĞLU Durumaçısı=-6.24 Enlemaçısı=1.95 Boylamaçısı=236.54 Boylamfark=1 GKalite=4 GDurum= Kuzeyaçısı=-0.4 Sırano=19743 AyRasatNo=21 RasatÖnceki=22.06.2023 RasatSonraki=24.06.2023 [Leke Grupları] Grupsayısı=12:6:6 LekeSayısı=101:46:55 RölatifSayı=221:106:115 01=CSO 04 +10.470 +31.225 267.765 16.596 0000 0 +12.178 +35.210 +08.762 +27.240 +09.246 +34.616 +11.424 +27.393 02=DSI 08 +19.929 +26.661 263.201 23.619 0000 0 +21.429 +30.430 +18.430 +23.279 +18.613 +29.342 +20.792 +24.352 03=DSI 22 +21.587 -05.123 231.417 17.586 0000 0 +25.245 -00.263 +17.928 -09.984 +21.587 -00.463 +24.870 -08.383 04=CSI 06 +09.488 -28.593 207.947 +0.000 0000 0 +10.170 -26.260 +08.806 -31.160 +09.488 -26.643 +09.488 -30.543 05=HS_ 03 +09.779 -48.709 187.831 +0.000 0000 0 +10.746 -46.985 +08.811 -50.433 +09.779 -47.485 +09.779 -49.933 06=AX_ 03 +22.195 -70.878 165.662 +0.000 0000 0 +22.750 -70.730 +21.640 -71.682 +22.195 -70.902 +22.195 -70.854 07=HS_ 15 -14.786 +48.583 285.123 +0.000 0000 0 -12.912 +52.460 -16.660 +45.120 -14.786 +51.753 -14.786 +45.413 08=BXI 09 -18.949 +15.610 251.601 27.849 0000 0 -17.323 +18.800 -20.574 +12.113 -20.119 +17.440 -17.529 +12.529 09=CSI 17 -19.392 +00.498 237.380 34.895 0000 0 -16.439 +04.955 -22.345 -03.959 -18.170 +02.870 -21.443 -02.836 10=HS_ 10 -15.721 -32.627 203.913 +0.000 0000 0 -13.418 -30.492 -18.240 -34.763 -15.721 -30.991 -15.721 -34.262 11=AX_ 01 -10.758 -49.102 187.438 -1.000 0000 0 -10.758 -49.102 -10.758 -49.102 12=BXO 03 -30.297 -58.356 178.184 +0.000 0000 0 -29.773 -54.903 -30.822 -61.809 -30.297 -55.403 -30.297 -61.30920230623.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 →
2023/20230623_bc · BC · 6 frames · 128.6 MB · 10:22:00–10:25:46 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.








