Solar Images Thursday, 28 July 2022
‹ 27.07.2022 2022 29.07.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 07:45 UT
- Observer
- Burçin TANIK
- g
- 4
- f
- 8
- R
- 48
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=28.07.2022 Saat=07:45 Gözlemci=Burçin TANIK KontrolEden=Olcay PLEVNE Durumaçısı=9.29 Enlemaçısı=5.48 Boylamaçısı=272.27 Boylamfark=2 GKalite=3 GDurum=G.T , K.T Kuzeyaçısı=-0.3 Sırano=19504 AyRasatNo=27 RasatÖnceki=27.07.2022 RasatSonraki=29.07.2022 [Leke Grupları] Grupsayısı=4:1:3 LekeSayısı=8:3:5 RölatifSayı=48:13:35 01=AX_ 03 +19.134 -49.526 222.744 +0.000 0000 0 +20.440 -48.442 +18.223 -50.609 +00.000 +00.000 +00.000 +00.000 02=HS_ 01 -25.450 +29.806 302.760 +0.000 0000 0 -23.796 +30.821 -26.295 +28.790 -25.450 +30.321 -25.450 +29.291 03=AX_ 02 -15.431 +18.104 290.374 +0.000 0000 0 -15.171 +18.380 -15.690 +17.827 -15.431 +17.881 -15.431 +18.327 04=BXO 02 -15.196 -68.742 203.528 17.797 0000 0 -14.920 -65.667 -16.300 -71.817 -14.404 -66.323 -16.100 -71.61720220728.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 →
2022/20220728_bto · BTO · 7 frames · 150.0 MB · 07:54:57–08:03:51 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.









