Solar Images Thursday, 29 September 2022

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Photosphere sunspot drawing and RDS evaluation

29.09.2022 photosphere drawing

High-resolution scan (3235 px)

Time
06:25 UT
Observer
Korhan YELKENCİ
g
4
f
35
R
75
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=29.09.2022
Saat=06:25
Gözlemci=Korhan YELKENCİ
KontrolEden=Başar COŞKUNOĞLU
Durumaçısı=25.81
Enlemaçısı=6.81
Boylamaçısı=160.68
Boylamfark=3
GKalite=3
GDurum=G.T , H.S
Kuzeyaçısı=0.1
Sırano=19564
AyRasatNo=27
RasatÖnceki=28.09.2022
RasatSonraki=30.09.2022

[Leke Grupları]
Grupsayısı=4:2:2
LekeSayısı=35:8:27
RölatifSayı=75:28:47
01=CSO 07 +16.245 -01.783 158.897 03.578 0000 0 +17.718 +03.575 +14.772 -07.141 +16.486 +00.778 +16.942 -06.534
02=HA_ 01 +27.569 -54.772 105.908 +0.000 0000 0 +28.513 -53.203 +26.624 -56.340 +27.569 -53.703 +27.569 -55.840
03=DAO 05 -16.300 +46.500 206.685 19.701 0000 0 -14.683 +49.224 -17.916 +42.787 -15.504 +48.109 -17.290 +43.112
04=CAI 22 -23.448 +28.360 188.716 02.800 0000 0 -21.995 +35.438 -24.901 +20.634 -23.983 +32.939 -23.607 +22.529
20220929.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 →

2022/20220929_ky · KY · 21 frames · 449.9 MB · 06:56:44–07:12:57 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.