Solar Images Monday, 27 June 2022

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Photosphere sunspot drawing and RDS evaluation

27.06.2022 photosphere drawing

High-resolution scan (3230 px)

Time
09:45 UT
Observer
Hikmet ÇAKMAK
g
4
f
18
R
58
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=27.06.2022
Saat=09:45
Gözlemci=Hikmet ÇAKMAK
KontrolEden=Talar YONTAN
Durumaçısı=-4.35
Enlemaçısı=2.43
Boylamaçısı=321.39
Boylamfark=1
GKalite=3
GDurum=G.T , H.S
Kuzeyaçısı=-0.1
Sırano=19474
AyRasatNo=26
RasatÖnceki=26.06.2022
RasatSonraki=28.06.2022

[Leke Grupları]
Grupsayısı=4:2:2
LekeSayısı=18:8:10
RölatifSayı=58:28:30
01=BXI 06 +15.639 +59.260 020.650 18.221 0000 0 +17.900 +62.403 +14.269 +56.117 +14.820 +61.990 +16.281 +56.657
02=AX_ 02 +08.682 -02.585 318.805 +0.000 0000 0 +08.920 -02.163 +08.443 -03.800 +08.682 -02.266 +08.682 -02.904
03=CAI 08 -12.437 +01.900 323.290 22.380 0000 0 -10.450 +04.571 -14.423 -00.772 -11.944 +03.874 -13.656 -00.288
04=AX_ 02 -19.284 -34.756 286.634 +0.000 0000 0 -18.767 -33.435 -19.800 -36.760 -19.284 -33.594 -19.284 -35.918
20220627.gzd

Chromosphere (H-α) FITS frames

H-α

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 →

2022/20220627_hc · HC · 4 frames · 85.7 MB · 09:46:26–09:57:52 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.