Solar Images Tuesday, 27 April 2021
‹ 26.04.2021 2021 28.04.2021 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:50 UT
- Observer
- Burçin TANIK
- g
- 3
- f
- 26
- R
- 56
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=27.04.2021 Saat=08:50 Gözlemci=Burçin TANIK KontrolEden=Ergün EGE Durumaçısı=-24.69 Enlemaçısı=-4.53 Boylamaçısı=186.45 Boylamfark=2 GKalite=3 GDurum=G.T , K.T Kuzeyaçısı=-0.5 Sırano=19169 AyRasatNo=15 RasatÖnceki=26.04.2021 RasatSonraki=28.04.2021 [Leke Grupları] Grupsayısı=3:0:3 LekeSayısı=26:0:26 RölatifSayı=56:0:56 01=DAI 11 -22.165 +31.879 218.329 11.155 0000 0 -20.613 +36.246 -23.716 +27.512 -21.415 +35.786 -22.940 +28.290 02=DAI 14 -22.820 +21.832 208.282 20.790 0000 0 -19.929 +26.295 -24.234 +17.369 -20.846 +25.962 -23.849 +17.712 03=HS_ 01 -15.994 +16.544 202.994 +0.000 0000 0 -15.371 +17.127 -16.616 +15.960 -15.994 +16.628 -15.994 +16.46120210427.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 →
2021/20210427_bto · BTO · 6 frames · 128.6 MB · 08:59:46–09:10:10 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.