Solar Images Sunday, 30 January 2022
‹ 29.01.2022 2022 31.01.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:30 UT
- Observer
- Burçin TANIK
- g
- 5
- f
- 40
- R
- 90
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=30.01.2022 Saat=08:30 Gözlemci=Burçin TANIK KontrolEden=Burçin TANIK Durumaçısı=-11.46 Enlemaçısı=-5.89 Boylamaçısı=116.03 Boylamfark=2 GKalite=3 GDurum=G.T , K.T Kuzeyaçısı=-0.7 Sırano=19365 AyRasatNo=15 RasatÖnceki=29.01.2022 RasatSonraki=31.01.2022 [Leke Grupları] Grupsayısı=5:3:2 LekeSayısı=40:38:2 RölatifSayı=90:68:22 01=BXO 03 +32.309 +44.740 160.770 +0.000 0000 0 +33.592 +47.712 +31.250 +41.769 +32.309 +47.512 +32.309 +41.969 02=FHC 30 +16.339 -02.269 113.761 15.463 0000 0 +19.500 +03.885 +13.674 -08.423 +17.364 +03.225 +14.230 -08.191 03=AX_ 05 +17.129 -24.691 091.339 +0.000 0000 0 +18.230 -23.261 +16.234 -26.122 +00.000 +00.000 +00.000 +00.000 04=HS_ 01 -25.179 +51.733 167.763 -1.000 0000 0 -24.151 +52.904 -26.207 +50.563 05=?__ 01 -14.741 -85.779 030.251 -1.000 0000 0 -13.458 -82.207 -16.240 -89.35220220130.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 →
2022/20220130_bto · BTO · 6 frames · 128.6 MB · 08:40:59–08:55:21 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.








