Solar Images Thursday, 6 August 2026

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Photosphere sunspot drawing and RDS evaluation

06.08.2026 photosphere drawing

High-resolution scan (3230 px)

Time
08:45 UT
Observer
Tuğba BOZTEPE
g
4
f
9
R
49
Seeing
4 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=6.08.2026
Saat=08:45
Gözlemci=Tuğba BOZTEPE
KontrolEden=Emre YILMAN
Durumaçısı=12.86
Enlemaçısı=6.13
Boylamaçısı=309.26
Boylamfark=2
GKalite=4
GDurum=G.T
Kuzeyaçısı=-0.4
Sırano=20533
AyRasatNo=6
RasatÖnceki=05.08.2026
RasatSonraki=07.08.2026

[Leke Grupları]
Grupsayısı=4:1:3
LekeSayısı=9:4:5
RölatifSayı=49:14:35
01=CKI 04 +16.385 +45.855 355.115 +0.000 0000 0 +18.972 +48.530 +13.797 +43.181 +16.385 +48.330 +16.385 +43.381
02=CSI 03 -07.327 +45.755 355.150 +0.000 0000 0 -06.430 +47.540 -08.225 +43.970 -07.327 +47.340 -07.327 +44.170
03=AS_ 01 -05.646 +38.743 348.300 +0.000 0000 0 -05.170 +39.494 -06.275 +37.992 -05.646 +38.994 -05.646 +38.492
04=AX_ 01 -15.441 -45.824 263.436 -1.000 0000 0 -15.441 -45.824 -15.441 -45.824
20260806.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 →

2026/20260806_tb · TB · 6 frames · 128.6 MB · 09:22:32–09:25:31 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.