Solar Images Sunday, 23 August 2026

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Photosphere sunspot drawing and RDS evaluation

23.08.2026 photosphere drawing

High-resolution scan (3223 px)

Time
11:30 UT
Observer
Burçin TANIK
g
3
f
37
R
67
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=23.08.2026
Saat=11:30
Gözlemci=Burçin TANIK
KontrolEden=Burçin TANIK
Durumaçısı=18.67
Enlemaçısı=6.98
Boylamaçısı=83.03
Boylamfark=0
GKalite=3
GDurum=G.T
Kuzeyaçısı=-0.5
Sırano=20548
AyRasatNo=21
RasatÖnceki=22.08.2026
RasatSonraki=24.08.2026

[Leke Grupları]
Grupsayısı=3:2:1
LekeSayısı=37:36:1
RölatifSayı=67:56:11
01=DRI 09 +10.341 -19.542 063.488 +0.000 0000 0 +11.930 -16.752 +09.589 -22.331 +10.341 -17.253 +10.341 -21.831
02=EKI 27 +04.386 -33.280 050.200 +0.000 0000 0 +07.690 -26.611 +01.702 -39.445 +04.386 -26.811 +04.386 -39.245
03=HS_ 01 -07.868 -44.794 038.236 -1.000 0000 0 -07.274 -43.995 -08.461 -45.592
20260823.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 →

2026/20260823_bto · BTO · 4 frames · 85.7 MB · 11:39:19–11:44:14 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.