Solar Images Friday, 23 July 2021
‹ 22.07.2021 2021 24.07.2021 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 10:55 UT
- Observer
- Burçin TANIK
- g
- 4
- f
- 11
- R
- 51
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=23.07.2021 Saat=10:55 Gözlemci=Burçin TANIK KontrolEden=Oğuzhan ÇAKIR Durumaçısı=7.36 Enlemaçısı=5.1 Boylamaçısı=114.21 Boylamfark=1 GKalite=3 GDurum=G.T , B.A , K.T Kuzeyaçısı=-0.6 Sırano=19224 AyRasatNo=22 RasatÖnceki=22.07.2021 RasatSonraki=24.07.2021 [Leke Grupları] Grupsayısı=4:2:2 LekeSayısı=11:8:3 RölatifSayı=51:28:23 01=BXO 02 +21.623 +02.191 116.401 +0.000 0000 0 +23.180 +03.867 +20.228 +00.514 +21.623 +03.667 +21.623 +00.714 02=HA_ 06 +24.142 -27.965 086.245 +0.000 0000 0 +24.895 -26.809 +23.390 -29.121 +24.142 -27.309 +24.142 -28.621 03=CRO 02 -27.730 -41.852 072.358 +0.000 0000 0 -25.607 -38.400 -28.539 -45.305 -27.730 -38.600 -27.730 -45.105 04=AX_ 01 -16.234 -55.252 058.958 -1.000 0000 0 -16.234 -55.252 -16.234 -55.25220210723.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 →
2021/20210723_bto · BTO · 5 frames · 107.1 MB · 10:58:48–11:07:06 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.







