Solar Images Wednesday, 26 October 2022

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Photosphere sunspot drawing and RDS evaluation

26.10.2022 photosphere drawing

High-resolution scan (3230 px)

Time
07:30 UT
Observer
Başar COŞKUNOĞLU
g
5
f
20
R
70
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=26.10.2022
Saat=07:30
Gözlemci=Başar COŞKUNOĞLU
KontrolEden=Burçin TANIK
Durumaçısı=25.31
Enlemaçısı=4.96
Boylamaçısı=163.9
Boylamfark=2
GKalite=3
GDurum=H.S
Kuzeyaçısı=-0.5
Sırano=19584
AyRasatNo=19
RasatÖnceki=25.10.2022
RasatSonraki=27.10.2022

[Leke Grupları]
Grupsayısı=5:2:3
LekeSayısı=20:5:15
RölatifSayı=70:25:45
01=HH_ 01 +23.710 -50.898 113.200 +0.000 0000 0 +25.780 -49.636 +22.341 -52.160 +23.710 -50.136 +23.710 -51.660
02=BXO 04 +27.347 -66.959 096.941 +0.000 0000 0 +28.746 -59.180 +25.948 -74.738 +27.347 -59.380 +27.347 -74.538
03=CSO 05 -08.735 +64.878 228.778 +0.000 0000 0 -06.954 +67.300 -10.516 +62.753 -08.735 +66.803 -08.735 +62.953
04=AX_ 01 -08.382 +20.548 184.448 -1.000 0000 0 -08.382 +20.548 -08.382 +20.548
05=CSI 09 -22.501 +18.587 182.487 +0.000 0000 0 -20.716 +22.589 -24.287 +14.586 -22.501 +22.389 -22.501 +14.786
20221026.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 →

2022/20221026_bc · BC · 6 frames · 128.6 MB · 07:54:51–08:01:50 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.