Solar Images Tuesday, 9 April 2024
‹ 08.04.2024 2024 10.04.2024 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 07:45 UT
- Observer
- Ergün EGE
- g
- 3
- f
- 11
- R
- 41
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=9.04.2024 Saat=07:45 Gözlemci=Ergün EGE KontrolEden=Korhan YELKENCİ Durumaçısı=-26.23 Enlemaçısı=-6.02 Boylamaçısı=358.73 Boylamfark=2 GKalite=3 GDurum= Kuzeyaçısı=-0.4 Sırano=19955 AyRasatNo=8 RasatÖnceki=08.04.2024 RasatSonraki=10.04.2024 [Leke Grupları] Grupsayısı=3:2:1 LekeSayısı=11:6:5 RölatifSayı=41:26:15 01=CHO 05 +06.945 +01.385 000.115 +0.000 0000 0 +09.870 +03.617 +04.803 -00.847 +06.945 +03.417 +06.945 -00.647 02=AX_ 01 +25.976 -02.900 355.830 +0.000 0000 0 +26.526 -02.596 +25.426 -03.204 +25.976 -03.960 +25.976 -02.704 03=CSO 05 -09.520 -40.892 317.838 +0.000 0000 0 -07.860 -37.246 -10.243 -44.538 -09.520 -37.446 -09.520 -44.33820240409.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 →
2024/20240409_ee · EE · 10 frames · 214.3 MB · 07:48:17–08:08:37 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.












