Solar Images Saturday, 2 November 2024
‹ 01.11.2024 2024 03.11.2024 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 10:50 UT
- Observer
- Korhan YELKENCİ
- g
- 12
- f
- 80
- R
- 200
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=2.11.2024 Saat=10:50 Gözlemci=Korhan YELKENCİ KontrolEden=Burçin TANIK Durumaçısı=24.15 Enlemaçısı=4.21 Boylamaçısı=141.45 Boylamfark=1 GKalite=3 GDurum=K.T Kuzeyaçısı=-0.4 Sırano=20136 AyRasatNo=2 RasatÖnceki=01.11.2024 RasatSonraki=03.11.2024 [Leke Grupları] Grupsayısı=12:6:6 LekeSayısı=80:35:45 RölatifSayı=200:95:105 01=FAI 03 +24.801 +76.685 218.135 12.960 0000 0 +26.652 +84.777 +22.950 +68.593 +26.452 +83.311 +23.150 +68.793 02=DAI 12 +27.746 +57.000 198.450 23.470 0000 0 +30.410 +62.346 +25.450 +51.654 +29.841 +62.146 +25.650 +52.230 03=AX_ 04 +22.835 +46.933 188.383 +0.000 0000 0 +23.574 +48.197 +22.960 +45.669 +22.835 +47.697 +22.835 +46.169 04=EAC 14 +15.577 -05.379 136.710 20.411 0000 0 +18.298 +01.192 +12.855 -11.951 +17.903 +00.745 +11.994 -13.920 05=AX_ 01 +17.617 -23.983 117.467 -1.000 0000 0 +17.617 -23.983 +17.617 -23.983 06=HH_ 01 +14.595 -30.376 111.740 +0.000 0000 0 +16.879 -27.913 +12.311 -32.838 +14.595 -28.413 +14.595 -32.339 07=FAC 08 -09.407 +71.953 213.403 17.971 0000 0 -06.510 +81.978 -12.763 +61.928 -06.338 +81.778 -12.563 +62.128 08=HS_ 02 -02.946 +68.818 210.268 +0.000 0000 0 -02.208 +70.725 -03.685 +66.910 -02.946 +70.226 -02.946 +67.410 09=DAC 10 -18.488 +52.873 194.323 21.394 0000 0 -16.254 +58.504 -20.721 +47.243 -16.454 +57.901 -20.521 +47.443 10=DAI 08 -14.418 +37.836 179.286 41.208 0000 0 -09.148 +44.101 -19.688 +31.571 -09.373 +43.525 -19.488 +31.771 11=DAI 14 -08.365 -19.648 121.802 26.975 0000 0 -06.482 -16.129 -10.249 -23.166 -06.682 -16.329 -10.490 -22.966 12=CAI 03 -05.894 -76.612 064.838 +0.000 0000 0 -05.237 -71.774 -06.551 -81.451 -05.894 -72.273 -05.894 -80.95120241102.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 →
2024/20241102_ky · KY · 14 frames · 299.9 MB · 11:09:05–11:15:35 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.
















