Solar Images Saturday, 30 March 2024
‹ 29.03.2024 2024 31.03.2024 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:15 UT
- Observer
- Ergün EGE
- g
- 3
- f
- 9
- R
- 39
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=30.03.2024 Saat=08:15 Gözlemci=Ergün EGE KontrolEden=Süleyman FİŞEK Durumaçısı=-26.08 Enlemaçısı=-6.62 Boylamaçısı=130.56 Boylamfark=2 GKalite=3 GDurum=H.S Kuzeyaçısı=-0.4 Sırano=19946 AyRasatNo=20 RasatÖnceki=29.03.2024 RasatSonraki=31.03.2024 [Leke Grupları] Grupsayısı=3:1:2 LekeSayısı=9:1:8 RölatifSayı=39:11:28 01=HS_ 01 +18.180 +54.865 185.425 +0.000 0000 0 +18.748 +55.726 +17.288 +54.300 +18.180 +55.780 +18.180 +54.652 02=FAC 07 -12.947 +77.937 208.497 +0.000 0000 0 -09.475 +69.833 -16.418 +86.410 -12.947 +85.841 -12.947 +70.330 03=AX_ 01 -13.138 +51.727 182.287 +0.000 0000 0 -12.873 +52.339 -13.404 +51.116 -13.138 +51.839 -13.138 +51.61620240330.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 →
2024/20240330_ee · EE · 4 frames · 85.7 MB · 08:18:48–08:22:16 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.