Solar Images Monday, 9 March 2026
‹ 08.03.2026 2026 10.03.2026 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 07:50 UT
- Observer
- Burçin TANIK
- g
- 5
- f
- 15
- R
- 65
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=9.03.2026 Saat=07:50 Gözlemci=Burçin TANIK KontrolEden=İrem ÖZDEMİR Durumaçısı=-23.37 Enlemaçısı=-7.24 Boylamaçısı=132.52 Boylamfark=2 GKalite=3 GDurum=G.T , K.T Kuzeyaçısı=0.6 Sırano=20433 AyRasatNo=7 RasatÖnceki=08.03.2026 RasatSonraki=11.03.2026 [Leke Grupları] Grupsayısı=5:5:0 LekeSayısı=15:15:0 RölatifSayı=65:65:0 01=HH_ 01 +17.345 +79.990 211.619 +0.000 0000 0 +18.842 +82.266 +15.849 +75.933 +17.345 +82.656 +17.345 +77.324 02=CKO 06 +08.681 +46.545 179.650 30.478 0000 0 +10.410 +49.282 +06.951 +43.808 +07.611 +48.230 +09.670 +44.729 03=AX_ 02 +12.419 +33.974 166.494 +0.000 0000 0 +12.745 +34.383 +12.930 +33.565 +12.419 +33.883 +12.419 +34.650 04=CHO 02 +08.889 +18.456 150.976 +0.000 0000 0 +10.150 +23.145 +07.628 +13.768 +08.889 +22.945 +08.889 +13.968 05=BXO 04 +08.843 -61.468 071.520 15.177 0000 0 +10.185 -57.576 +07.501 -65.360 +08.490 -58.651 +09.462 -63.87020260309.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 →
2026/20260309_bto · BTO · 2 frames · 42.9 MB · 07:57:26–07:59:17 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.




