Solar Images Monday, 4 November 2024

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Photosphere sunspot drawing and RDS evaluation

04.11.2024 photosphere drawing

High-resolution scan (3231 px)

Time
10:40 UT
Observer
Ergün EGE
g
11
f
47
R
157
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=4.11.2024
Saat=10:40
Gözlemci=Ergün EGE
KontrolEden=Burçin TANIK
Durumaçısı=23.77
Enlemaçısı=4
Boylamaçısı=115.17
Boylamfark=1
GKalite=3
GDurum=
Kuzeyaçısı=-0.3
Sırano=20138
AyRasatNo=4
RasatÖnceki=03.11.2024
RasatSonraki=06.11.2024

[Leke Grupları]
Grupsayısı=11:3:8
LekeSayısı=47:4:43
RölatifSayı=157:34:123
01=AX_ 01 +30.446 +78.546 193.716 +0.000 0000 0 +30.875 +80.250 +30.160 +76.842 +30.446 +79.750 +30.446 +77.342
02=ESI 01 +16.369 +20.318 135.488 +0.000 0000 0 +18.772 +27.150 +13.966 +13.622 +16.369 +26.815 +16.369 +13.822
03=HH_ 02 +15.387 -05.403 109.767 +0.000 0000 0 +17.611 -02.896 +13.164 -07.911 +15.387 -03.395 +15.387 -07.410
04=HS_ 01 -17.600 +76.633 191.803 +0.000 0000 0 -16.933 +79.676 -18.266 +73.590 -17.600 +79.176 -17.600 +74.900
05=HS_ 02 -16.209 +67.452 182.622 +0.000 0000 0 -15.493 +69.448 -16.926 +65.456 -16.209 +68.948 -16.209 +65.956
06=AX_ 01 -09.307 +62.730 177.900 +0.000 0000 0 -08.983 +63.391 -09.630 +62.700 -09.307 +62.576 -09.307 +62.884
07=CRO 05 -09.571 +49.954 165.124 +0.000 0000 0 -08.291 +53.271 -10.851 +46.637 -09.571 +53.710 -09.571 +46.837
08=DAI 10 -08.401 +06.869 122.390 +0.000 0000 0 -06.255 +11.199 -10.547 +02.539 -08.401 +10.999 -08.401 +02.739
09=ESC 12 -05.392 -42.438 072.732 +0.000 0000 0 -03.434 -36.534 -07.350 -48.343 -05.392 -36.734 -05.392 -48.143
10=HR_ 01 -06.543 -60.290 055.141 +0.000 0000 0 -05.887 -59.124 -07.199 -60.934 -06.543 -59.885 -06.543 -60.695
11=EAI 11 -05.550 -74.714 040.456 +0.000 0000 0 -01.945 -66.690 -09.155 -82.738 -05.550 -66.890 -05.550 -82.538
20241104.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 →

2024/20241104_ee · EE · 7 frames · 150.0 MB · 10:40:43–10:56:24 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.