Solar Images Saturday, 29 October 2022
‹ 28.10.2022 2022 30.10.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 10:00 UT
- Observer
- Ergün EGE
- g
- 4
- f
- 20
- R
- 60
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=29.10.2022 Saat=10:00 Gözlemci=Ergün EGE KontrolEden=Ergün EGE Durumaçısı=24.89 Enlemaçısı=4.66 Boylamaçısı=122.8 Boylamfark=1 GKalite=3 GDurum=B.A Kuzeyaçısı=-0.5 Sırano=19587 AyRasatNo=22 RasatÖnceki=28.10.2022 RasatSonraki=30.10.2022 [Leke Grupları] Grupsayısı=4:3:1 LekeSayısı=20:17:3 RölatifSayı=60:47:13 01=CSI 03 +23.701 -13.429 109.371 +0.000 0000 0 +26.750 -08.914 +21.327 -17.944 +23.701 -09.114 +23.701 -17.744 02=BXI 10 +26.118 -29.153 093.647 +0.000 0000 0 +27.815 -24.804 +24.420 -33.503 +26.118 -25.400 +26.118 -33.303 03=DRI 04 +27.263 -60.900 062.710 +0.000 0000 0 +28.478 -55.311 +26.470 -64.869 +27.263 -55.511 +27.263 -64.669 04=CRI 03 -23.352 +60.930 183.730 +0.000 0000 0 -22.565 +64.266 -24.138 +57.594 -23.352 +63.766 -23.352 +58.94020221029.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 →
2022/20221029_ee · EE · 8 frames · 171.4 MB · 10:11:41–10:28:29 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.










