Solar Images Wednesday, 30 October 2024

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Photosphere sunspot drawing and RDS evaluation

30.10.2024 photosphere drawing

High-resolution scan (3231 px)

Time
10:20 UT
Observer
Burçin TANIK
g
11
f
106
R
216
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=30.10.2024
Saat=10:20
Gözlemci=Burçin TANIK
KontrolEden=Süleyman FİŞEK
Durumaçısı=24.66
Enlemaçısı=4.52
Boylamaçısı=181.28
Boylamfark=1
GKalite=3
GDurum=G.T , B.A
Kuzeyaçısı=-0.7
Sırano=20133
AyRasatNo=26
RasatÖnceki=29.10.2024
RasatSonraki=31.10.2024

[Leke Grupları]
Grupsayısı=11:5:6
LekeSayısı=106:35:71
RölatifSayı=216:85:131
01=EKI 10 +24.274 +38.194 219.474 +0.000 0000 0 +25.836 +44.222 +22.712 +32.165 +24.274 +44.220 +24.274 +32.365
02=BXI 07 +27.792 +19.594 200.874 56.312 0000 0 +29.647 +21.970 +25.938 +18.920 +26.558 +20.253 +28.730 +18.804
03=AX_ 01 +04.468 -24.846 156.434 -1.000 0000 0 +04.468 -24.846 +04.468 -24.846
04=EKC 16 +15.121 -43.735 137.545 16.782 0000 0 +17.847 -37.860 +12.395 -49.611 +16.670 -39.315 +14.593 -46.219
05=HH_ 01 +14.791 -68.385 112.895 +0.000 0000 0 +16.754 -66.400 +12.828 -70.766 +14.791 -66.702 +14.791 -70.680
06=HH_ 01 -11.448 +38.830 219.363 +0.000 0000 0 -09.999 +39.353 -12.896 +36.813 -11.448 +39.600 -11.448 +38.600
07=DKC 34 -05.974 +25.540 206.334 20.566 0000 0 -02.343 +30.180 -09.605 +20.910 -03.710 +28.608 -06.326 +21.613
08=DKC 13 -18.101 +11.946 193.226 +0.000 0000 0 -16.493 +16.241 -19.710 +07.651 -18.101 +16.410 -18.101 +07.851
09=EHI 20 -13.864 -01.872 179.408 30.252 0000 0 -09.873 +04.400 -17.856 -07.784 -16.677 +01.609 -12.665 -05.298
10=AX_ 01 -15.849 -17.453 163.827 -1.000 0000 0 -15.849 -17.453 -15.849 -17.453
11=AX_ 02 -16.930 -22.810 158.470 +0.000 0000 0 -15.829 -22.232 -16.356 -23.388 -16.930 -22.732 -16.930 -22.888
20241030.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 →

2024/20241030_bto · BTO · 2 frames · 42.9 MB · 10:34:51–10:38:29 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.