Solar Images Friday, 16 September 2022
‹ 15.09.2022 2022 17.09.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:00 UT
- Observer
- Başar COŞKUNOĞLU
- g
- 4
- f
- 27
- R
- 67
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=16.09.2022 Saat=08:00 Gözlemci=Başar COŞKUNOĞLU KontrolEden=Hikmet ÇAKMAK Durumaçısı=24.24 Enlemaçısı=7.19 Boylamaçısı=331.39 Boylamfark=2 GKalite=3 GDurum=G.T Kuzeyaçısı=-0.6 Sırano=19552 AyRasatNo=15 RasatÖnceki=15.09.2022 RasatSonraki=17.09.2022 [Leke Grupları] Grupsayısı=4:0:4 LekeSayısı=27:0:27 RölatifSayı=67:0:67 01=HS_ 03 -22.586 +23.997 355.387 +0.000 0000 0 -21.645 +25.527 -23.528 +22.467 -22.586 +25.270 -22.586 +22.967 02=DSI 15 -13.702 -02.628 328.762 +0.000 0000 0 -12.521 -00.235 -14.883 -05.200 -13.702 -00.435 -13.702 -04.820 03=DSC 03 -25.635 -30.621 300.769 +0.000 0000 0 -24.505 -28.123 -26.766 -33.120 -25.635 -28.323 -25.635 -32.920 04=BXI 06 -22.801 -38.289 293.101 08.420 0000 0 -21.642 -36.113 -23.959 -40.466 -22.801 -36.313 -23.320 -39.82120220916.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 →
2022/20220916_bc · BC · 6 frames · 128.6 MB · 08:18:49–08:23:45 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.








