Solar Images Monday, 9 September 2024
‹ 08.09.2024 2024 10.09.2024 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 06:50 UT
- Observer
- Burçin TANIK
- g
- 11
- f
- 68
- R
- 178
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=9.09.2024 Saat=06:50 Gözlemci=Burçin TANIK KontrolEden=Süleyman FİŞEK Durumaçısı=23.03 Enlemaçısı=7.25 Boylamaçısı=136.14 Boylamfark=3 GKalite=3 GDurum=B.A Kuzeyaçısı=0.4 Sırano=20087 AyRasatNo=8 RasatÖnceki=08.09.2024 RasatSonraki=10.09.2024 [Leke Grupları] Grupsayısı=11:4:7 LekeSayısı=68:17:51 RölatifSayı=178:57:121 01=CRO 05 +13.927 +39.982 176.122 28.863 0000 0 +15.287 +42.485 +12.567 +37.479 +13.101 +41.434 +14.763 +38.416 02=CHI 08 +15.205 -22.780 113.360 30.121 0000 0 +17.206 -19.968 +13.204 -25.592 +14.780 -21.306 +15.917 -24.479 03=AX_ 02 +15.900 -27.229 108.911 +0.000 0000 0 +15.640 -26.929 +14.540 -27.529 +15.900 -27.429 +15.900 -27.290 04=BXO 02 +12.964 -33.550 103.850 +0.000 0000 0 +13.188 -31.436 +12.740 -34.675 +12.964 -32.431 +12.964 -34.669 05=AX_ 05 -13.720 +39.826 175.966 +0.000 0000 0 -12.913 +40.963 -14.527 +38.689 +00.000 +00.000 +00.000 +00.000 06=CKO 07 -10.770 +36.324 172.464 28.862 0000 0 -08.900 +39.718 -12.146 +32.930 -08.736 +38.872 -11.294 +34.223 07=AX_ 04 -17.312 +22.508 158.648 +0.000 0000 0 -16.764 +23.203 -17.861 +21.814 -17.312 +22.702 -17.312 +22.313 08=?__ 10 -22.134 +15.336 151.476 +0.000 0000 0 -18.685 +19.940 -25.582 +10.732 -22.134 +19.440 -22.134 +11.232 09=CSI 04 -10.280 +13.353 149.493 +0.000 0000 0 -08.726 +16.219 -11.331 +10.487 -10.280 +16.190 -10.280 +10.687 10=AX_ 06 -09.699 +08.267 144.407 +0.000 0000 0 -08.707 +09.619 -10.691 +06.916 +00.000 +00.000 +00.000 +00.000 11=CHO 15 -24.253 +00.370 136.177 19.950 0000 0 -20.791 +08.833 -27.716 -08.760 -21.976 +08.201 -27.132 -06.90720240909.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 →
2024/20240909_bto · BTO · 4 frames · 85.7 MB · 07:00:46–07:23:39 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.






