Solar Images Monday, 29 August 2022

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Photosphere sunspot drawing and RDS evaluation

29.08.2022 photosphere drawing

High-resolution scan (3230 px)

Time
08:30 UT
Observer
Hikmet ÇAKMAK
g
4
f
40
R
80
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=29.08.2022
Saat=08:30
Gözlemci=Hikmet ÇAKMAK
KontrolEden=Ergün EGE
Durumaçısı=20.33
Enlemaçısı=7.14
Boylamaçısı=208.83
Boylamfark=2
GKalite=3
GDurum=G.T , H.S
Kuzeyaçısı=-0.4
Sırano=19536
AyRasatNo=29
RasatÖnceki=28.08.2022
RasatSonraki=30.08.2022

[Leke Grupları]
Grupsayısı=4:1:3
LekeSayısı=40:2:38
RölatifSayı=80:12:68
01=?__ 02 +31.335 +79.919 288.749 +0.000 0000 0 +32.345 +81.281 +30.324 +78.558 +31.335 +80.781 +31.335 +79.570
02=BXO 03 -23.130 +28.707 237.537 +0.000 0000 0 -22.627 +31.400 -23.398 +26.130 -23.130 +30.842 -23.130 +26.572
03=AX_ 01 -13.231 +03.755 212.585 -1.000 0000 0 -13.231 +03.755 -13.231 +03.755
04=EAC 34 -21.542 -16.337 192.493 13.848 0000 0 -18.611 -09.926 -24.472 -22.747 -23.260 -11.195 -20.754 -21.419
20220829.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 →

2022/20220829_hc · HC · 11 frames · 235.7 MB · 08:23:46–09:27:36 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.