Solar Images Friday, 3 January 2025
‹ 02.01.2025 2025 05.01.2025 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:50 UT
- Observer
- Ergün EGE
- g
- 13
- f
- 65
- R
- 195
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=3.01.2025 Saat=08:50 Gözlemci=Ergün EGE KontrolEden=Süleyman FİŞEK Durumaçısı=0.79 Enlemaçısı=-3.3 Boylamaçısı=45.51 Boylamfark=2 GKalite=3 GDurum=B.A Kuzeyaçısı=-0.5 Sırano=20167 AyRasatNo=3 RasatÖnceki=02.01.2025 RasatSonraki=05.01.2025 [Leke Grupları] Grupsayısı=13:4:9 LekeSayısı=65:13:52 RölatifSayı=195:53:142 01=AX_ 01 +13.333 +64.690 110.200 +0.000 0000 0 +13.657 +65.135 +13.100 +64.245 +13.333 +64.635 +13.333 +64.745 02=HS_ 01 +17.159 +55.538 101.480 -1.000 0000 0 +17.750 +56.346 +16.567 +54.730 03=AX_ 02 +14.207 -43.721 001.789 +0.000 0000 0 +14.668 -43.165 +13.747 -44.276 +14.207 -43.666 +14.207 -43.777 04=DAC 09 +11.635 -67.551 337.959 +0.000 0000 0 +13.250 -61.162 +10.190 -73.940 +11.635 -61.362 +11.635 -73.740 05=HR_ 01 -19.534 +81.937 127.447 -1.000 0000 0 -19.156 +85.395 -19.913 +78.478 06=DSO 02 -12.404 +58.320 103.542 +0.000 0000 0 -11.460 +61.841 -13.762 +54.224 -12.404 +61.641 -12.404 +54.424 07=CSO 05 -17.767 +36.387 081.897 +0.000 0000 0 -16.262 +38.468 -19.273 +34.307 -17.767 +38.268 -17.767 +34.507 08=CSI 04 -06.530 +30.740 075.584 +0.000 0000 0 -04.912 +36.752 -08.149 +23.395 -06.530 +36.552 -06.530 +23.595 09=BXO 04 -09.684 +13.173 058.683 +0.000 0000 0 -08.617 +14.952 -10.752 +11.393 -09.684 +14.752 -09.684 +11.593 10=DAI 07 -14.222 -01.964 043.546 +0.000 0000 0 -11.942 +02.213 -16.501 -06.142 -14.222 +02.130 -14.222 -05.942 11=DAI 10 -15.149 -33.458 012.520 +0.000 0000 0 -12.104 -28.553 -18.193 -38.362 -15.149 -28.753 -15.149 -38.162 12=DSI 17 -08.934 -41.354 004.156 25.872 0000 0 -06.185 -37.280 -11.683 -45.680 -07.724 -39.422 -10.203 -44.543 13=HS_ 02 -13.103 -48.230 357.280 -1.000 0000 0 -11.856 -46.895 -14.351 -49.56520250103.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 →
2025/20250103_ee · EE · 8 frames · 171.4 MB · 08:55:42–09:11:46 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.










