Solar Images Tuesday, 1 November 2022
‹ 31.10.2022 2022 02.11.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:00 UT
- Observer
- Korhan YELKENCİ
- g
- 4
- f
- 19
- R
- 59
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=1.11.2022 Saat=08:00 Gözlemci=Korhan YELKENCİ KontrolEden=Talar YONTAN Durumaçısı=24.44 Enlemaçısı=4.38 Boylamaçısı=84.5 Boylamfark=2 GKalite=3 GDurum=K.T Kuzeyaçısı=-0.5 Sırano=19590 AyRasatNo=1 RasatÖnceki=31.10.2022 RasatSonraki=02.11.2022 [Leke Grupları] Grupsayısı=4:3:1 LekeSayısı=19:12:7 RölatifSayı=59:42:17 01=HH_ 03 +22.646 +24.576 109.760 +0.000 0000 0 +24.110 +26.267 +21.280 +22.884 +22.646 +25.767 +22.646 +23.385 02=DAI 08 +26.670 -23.741 060.759 15.650 0000 0 +27.692 -18.206 +24.441 -29.276 +27.492 -18.412 +24.641 -29.760 03=HS_ 01 +36.726 -73.140 011.360 +0.000 0000 0 +37.294 -71.760 +36.158 -74.520 +36.726 -72.260 +36.726 -74.200 04=BXI 07 -06.814 -47.779 036.721 +0.000 0000 0 -06.130 -45.837 -07.498 -49.722 -06.814 -46.336 -06.814 -49.22220221101.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 →
2022/20221101_ky · KY · 15 frames · 321.4 MB · 08:35:36–08:42:36 UT
08:36:36 UT · 30 ms
08:40:36 UT · 30 ms
08:36:06 UT · 50 ms · over-exposed
08:40:06 UT · 50 ms · over-exposed
08:35:36 UT · 60 ms · over-exposed
08:39:36 UT · 60 ms · over-exposed
08:42:36 UT
08:41:06 UT · 60 ms
08:41:36 UT · 50 ms
08:42:06 UT · 30 ms
08:39:06 UT
08:37:06 UT · 60 ms
08:37:36 UT · 50 ms
08:38:06 UT · 30 ms
08:38:36 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.


