Solar Images Monday, 10 October 2022
‹ 09.10.2022 2022 11.10.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 10:41 UT
- Observer
- Ergün EGE
- g
- 4
- f
- 34
- R
- 74
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=10.10.2022 Saat=10:41 Gözlemci=Ergün EGE KontrolEden=Talar YONTAN Durumaçısı=26.26 Enlemaçısı=6.21 Boylamaçısı=13.19 Boylamfark=1 GKalite=3 GDurum= Kuzeyaçısı=-0.4 Sırano=19571 AyRasatNo=6 RasatÖnceki=09.10.2022 RasatSonraki=11.10.2022 [Leke Grupları] Grupsayısı=4:4:0 LekeSayısı=34:34:0 RölatifSayı=74:74:0 01=FSC 14 +22.352 +31.795 044.985 +0.000 0000 0 +25.738 +43.510 +18.966 +20.540 +22.352 +42.851 +22.352 +20.740 02=CSI 05 +30.604 +28.310 041.221 +0.000 0000 0 +33.660 +34.130 +28.141 +22.490 +30.604 +33.813 +30.604 +22.249 03=ESI 12 +28.726 -05.424 007.766 +0.000 0000 0 +31.171 +00.867 +26.282 -11.715 +28.726 +00.667 +28.726 -11.515 04=AX_ 03 +09.508 -17.639 355.551 +0.000 0000 0 +11.160 -16.549 +08.000 -18.729 +00.000 +00.000 +00.000 +00.00020221010.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 →
2022/20221010_ee · EE · 7 frames · 150.0 MB · 08:27:28–08:35:07 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.









